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Sizes to scale. Distances between planets are to scale.

Sizes to scale

Earth and moon, with size and distance to scale.

Sizes to scale. Also, the size of a moon is in scale with the distance to its host planet.

Continue to the rest of the "scales of the universe exhibit"


Appendix

Elements

Materials science textbook

Price



Stiffness

For a material, the "stiffness" is characterized by the "Tensile modulus". The stiffer a material, the more force it takes to stretch it.

The plot shows the elastic energy per mass at the breaking point, divided by the density. Alloys are much stronger than pure metals. Kevlar is substantially stronger than metals.

Stiffness tends to go together with density.



The following plot quantifies the elastic strength of materials.

Kevlar is stronger than metals.

Alloys are stronger than pure metals.

The "Yield strength" is the tensile force/area required to break it.


Rivers


Molecules

Atom size

Dot size corresponds to atom size. For gases, the density at boiling point is used.


Hydrogen molecules and valence

LiH
BeH2
BH3
CH4
NH3
H2O
HF

Hydrogen forms molecules with all elements except the noble gases, osmium, iridium, promethium, francium, and radium. This makes it a benchmark for determining the number of bonds that each element forms, as well as the strength of each element's attraction for electrons.


Oxides

Fe2O3  paint

H2O
Li2O
BeO
B2O3
CO2
N2O
O2
OF2


Oxyanions

Water
Carbonic acid
Nitric acid
Nitrous acid
Silicic acid
Phosphoric acid
Sulfuric acid

Hydroxide
Carbonate
Nitrate
Nitrite
Silicate
Phosphate
Sulfate

Type         Example

Hydroxide    HOH          Hydrogen hydroxide
Hypofluorite HFO          Hypoflourous acid
Hypochlorite HClO         Hypochlorous acid

Peroxide     H2O2         Hydrogen peroxide

Carbide      WC           Tungsten carbide
Oxide        H2O          Hydrogen oxide
Fluoride     HF           Hydrogen fluoride
Silicide     H4Si         Hydrogen silicide
Phosphide    H3P          Hydrogen phosphide
Sulfide      H2S          Hydrogen sulfide
Chloride     HCl          Hydrogen chloride
Arsenide     H3As         Hydrogen arsenide
Selenide     H2Se         Hydrogen selenide
Bromide      HBr          Hydrogen bromide

Carbonate    H2CO3        Carbonic acid
Nitrate      HNO3         Nitric acid
Aluminate    H5AlO4       Hydrogen aluminate
Silicate     H4SiO4       Silicic acid
Phosphate    H3PO4        Phosphoric acid
Sulfate      H2SO4        Sulfuric acid
Chlorate     HClO3        Hydrogen chlorate
Perchlorate  HClO4        Hydrogen perchlorate
Germanate    H4GeO4       Hydrogen germanate
Arsenate     H3AsO4       Arsenic acid
Selenate     H2SeO4       Hydrogen selenate
Bromate      HBrO3        Hydrogen bromate
Tellurate    H2TeO4       Hydrogen tellurate
Iodate       HIO3         Hydrogen iodate

Nitrite      HNO2         Nitrous acid
Chlorite     HClO2        Hydrogen chlorite

Carbides

Tungsten carbide drill
Tungsten carbide
Silicon carbide
Boron carbide

      Carbon atoms per metal atom

Boron      1/4
Silicon     1
Titanium    1
Beryllium  1/2
Zirconium  1/2
Tantalum    1
Tungsten    1
Aluminum   3/4

Hydroxide
Water

Carbonate
Carbonic acid

Nitrate
Nitric acid

Nitrite
Nitrous acid

Silicate
Silicic acid

Phosphate
Phosphoric acid

Sulfate
Sulfuric acid
--> 320px-Monophosphan.svg.png 233px-Methane-2D-stereo.svg.png BH3.png 247px-Phosphine-underside-3D-vdW.png Chili-5757_-_Hans_Braxmeier.jpg Hydrogen-fluoride-2D-flat.png Hydrogen_disulfide.png 294px-Phosphine-3D-balls.png Ionic_Bond_1.gif Ionic_Bonds.png 320px-Ammonia-2D.svg.png Ionic_bonding_animation.gif Monophosphan.svg.png 320px-H2O_-_2d.svg.png beryllium.hydride.5.png -->


Electronegativity

Every atom attracts electrons and the electronegativity table shows the relative energy released when the atom captures an electron. The elements in the upper right are the most electron-hungry.

In the reaction   H + H + O   →   H2O,   The oxygen steals an electron from each of the two hydrogens. It is able to do this because the electrons are at a lower energy with oxygen than with hydrogen.

Most chemical reactions involve elements on the left side of the periodic table giving electrons to elements on the right side.


Organic chemistry

Propane with hydrogens included
Propane with hydrogen excluded

A molecule is organic if it contains carbon. Molecules are often depicted with the hydrogens excluded.


Alkanes

Methane
Ethane
Propane
Octane

An "Alkane" is a carbon chain with hydrocarbons attached. At standard temperature (300 K), alkanes are solid if they have more than 20 carbons. This is why lipids (long alkanes) are the optimal form of energy storage. Short alkanes are liquids or gases at STP and are hard to store.

In the following table, the first section shows properties of alkanes and the second section shows properties of other energy sources.

Alkane   Carbons  Energy of   Melt  Boil  Solid    Liquid    Gas       Phase at
type              combustion  (K)   (K)   density  density   density   300 K
                  (MJ/kg)                 (g/cm^3) (g/cm^3)  (g/cm^3)

Hydrogen     0     141.8      14.0   20.3           .07      .000090   Gas
Methane      1      55.5      90.7  111.7           .423     .00070    Gas
Ethane       2      51.9      90.4  184.6           .545     .0013     Gas
Propane      3      50.4      85.5  231.1           .60      .0020     Gas
Butane       4      49.5     136    274             .60      .0025     Gas
Pentane      5      48.6     143.5  309             .63                Liquid
Hexane       6      48.2     178    342             .65                Liquid
Heptane      7      48.0     182.6  371.5           .68                Liquid
Octane       8      47.8     216.3  398.7           .70                Liquid
Dodecain    12      46       263.5  489             .75                Liquid
Hexadecane  16      46       291    560             .77                Liquid
Icosane     20      46       310    616     .79                        Solid
Alkane-30   30      46       339    723     .81                        Solid
Alkane-40   40      46       355    798     .82                        Solid
Alkane-50   50      46       364    848     .82                        Solid
Alkane-60   60      46       373    898     .83                        Solid


Gasoline   ~ 8      47                               .76               Liquid     Mostly alkanes with ~ 8 carbons
Natural gas         54        91    112                                Gas        Mostly methane
Coal                32         -      -                                Solid      Mostly carbon
Wood                22         -      -                                Solid      Carbon, oxygen, hydrogen
Pure carbon  1      32.8       -      -                                Solid      Pure carbon, similar to coal
Methanol     1     175.6  337.8           .79                          Liquid
Ethanol      2     159    351.5           .79                          Liquid
Propanol     3     147    370                                          Liquid

An alkane with 7 or more carbons has a heat of combustion of 46 MJoules/kg.

A nitrogen molecule is more tightly bound than an oxygen molecule, making it impossible to extract energy from hydrocarbons with nitrogen. Few things burn in a nitrogen atmosphere, lithium and magnesium being examples.


Hydrogen saturation

A chain is "saturated" if it contains the maximum number of hydrogen atoms and "unsaturated" if it contains less. Examples of unsaturated carbon chains:

Ethene
Acetylene
Propene
Butadiene

The hydrogens are required to stabilize the carbon chain.


Bond resonance

If there is a double or triple bond then the electrons can be mobile and assume different states. The molecule exists in a quantum-mechanical resonance between the possible states.


Non-carbon chains

Ammonia
Hydrazine
Triazane

Silane, spontaneously ignites in air
Disilane
Trisilane
Silene

Hydrogen peroxide
Diborane
Diphosphan

Suppose we make a chain of atoms that is saturated in hydrogen. The following table gives the longest stable chain for each element, and the longest stable chain in an oxygen environment. Only carbon is capable of making long chains. We can expect that aliens will be carbon-based.

          Stable   Stable in an
                  oxygen environment

Lithium     1            1
Boron       0            0
Carbon      ∞            ∞
Nitrogen    1            1
Oxygen      1            1
Aluminum    1            1
Silicon     2            0
Phosphorus  1            0
Sulfur      1            0

Cycloalkanes

Cyclohexane comes in different conformations with different energies.


Cyclohexene


Benzene

Benzine is a resonance molecule.

Napthaline
Napthaline


3D

Tetrahedrane
Cubane
Methylcyclopropene
Propellane
Pagodane
Pagoda


Functional group

Organic molecules are classified by their functional group. "R" stands for an arbitrary molecule.

Alkyne
Alcohol
Thiol
Carboxyl

Aldehyde
Ketone group
Thial
Thioketone

Ether
Sulfide

Peroxy group
Organice disulfide
Azo group
Methylenedioxy group

Carboxyl group
Nitro group
Phosphate
Phosphonic acid

Phenyl group
Pyridyl group


Fuel

                 MJoules/kg

Antimatter       90 billion
Hydrogen bomb      25000000    theoretical maximum yield
Hydrogen bomb      21700000    highest achieved yield
Uranium            20000000    as nuclear fuel
Hydrogen                143
Natural gas              53.6
Gasoline                 47
Jet fuel                 43
Fat                      37
Coal                     24
Carbohydrates & sugar    17
Protein                  16.8
Wood                     16
Lithium-air battery       9
TNT                       4.6
Gunpowder                 3
Lithium battery           1.3
Lithium-ion battery        .72
Alkaline battery           .59
Compressed air             .5        300 atmospheres
Supercapacitor             .1
Capacitor                  .00036
The chemical energy source with the highest energy/mass is hydrogen+oxygen, but molecular hydrogen is difficult to harness. Hydrocarbons + oxygen is the next best choice. Carbon offers a convenient and lightweight way to carry hydrogen around.

Reacting hydrocarbons in an oxygen atmosphere yields the optimal power-to-weight ratio.

Given the enormous power required by brains, if intelligent life exists in the universe, it likely gets its energy from reacting hydrocarbons in an oxygen atmosphere. Most likely we would be able to eat their food.


Food
        MJ/kg  Calories/gram
Sugar    16        5
Protein  17        5
Alcohol  25        7
Fat      38        9
Humans can metabolize a wide range of fats and sugars.
Elements of single-cellular life

Life appeared on the Earth within a billion years of its formation. http://en.wikipedia.org/wiki/Timeline_of_evolutionary_history_of_life

Shortly after that, between 3500 and 3800 million years ago, the "Last Universal Common Ancestor" lived. http://en.wikipedia.org/wiki/Last_Universal_Common_Ancestor

The LUCA had the following properties: Single-cellular with a bilipid cell wall. ATP to power enzymes. A DNA codon system with 4^3=64 options coding for 20 proteins. This code hasn't changed since.

Building blocks for life
   
        Abundance in  Mass frac in
        Crust (ppm)   Human body
Oxygen      460000     .65
Carbon        1000     .18
Hydrogen      1500     .10
Nitrogen        20     .03
Calcium      45000     .014
Phosphorus    1100     .011
Potassium    20000     .0025
Sulfur         400     .0025
Sodium       25000     .0015
Chlorine       200     .0015
Magnesium    25000     .0005
Iron         60000     .00006
Fluorine       500     .000037
Zinc            75     .000032
Silicon     275000     .00002
Trace elements        <.00001
Among the elements required for life, nitrogen is the scarcest. The nitrogen in the first 250 km of the Earth's crust has the same mass as the nitrogen in the atmosphere.
           Used by   Used by
           humans    bacteria
Hydrogen      *      *
Helium
Lithium
Beryllium
Boron         *      *
Carbon        *      *
Nitrogen      *      *
Oxygen        *      *
Fluorine             *
Neon
Sodium        *      *
Magnesium     *      *
Aluminum
Silicon              *
Phosphorus    *      *
Sulfur        *      *
Chlorine      *      *
Argon
Potassium     *      *
Calcium       *      *
Scandium
Titanium
Vanadium             *
Chromium
Manganese     *      *
Iron          *      *
Cobalt        *      *
Nickel               *
Copper        *      *
Zinc          *      *
Gallium
Germanium
Arsenic              *
Selenium      *      *
Bromine       *      *
Krypton
Molybdenum           *
Tellurium            *
Iodine        *      *
Tungsten             *

Cell walls
Lipids and cell membranes

Cell walls are formed from a double layer of lipids. They are elastic and they self-assemble.

Each lipid has a polar and a non-polar end. The polar end faces the water and the non-polar end faces another lipid.

* Video of the self-assembly of a bilipid layer
* Video of an amoeba

If life were to exist in a non-polar solvent it would have to find another way to make cell walls.


ATP and ATP Synthase

Enzymes use ATP as an energy source to power chemical reactions. ATP and ATP synthase are common to all Earth life.

* Video of the ATP synthase enzyme in action

Amino acids

Amino acids have the above form, where R stands for an arbitrary molecule.

The 21 amino acids used by eucaryote life


Protein

Synthesis of two amino acids. Proteins are chains of animo acids with a backbone of the form:

C-C-N-C-C-N-C-C-N-C-C-N-C-C-N

DNA and the genetic code

DNA codes a sequence of amino acids. The 64-element codon system is universal to Earth life.

The codon ATG both codes for methionine and serves as an initiation site: the first ATG in an mRNA's coding region is where translation into protein begins.

21 amino acids are used by eucaryote. More than 500 amino acids are known.


Sugar

Glucose

A sugar generally has the formula CN H2N ON, where N = 2, 3, etc. The common sugars are hexoses with N=6.

         Number of   Number of
          carbons     sugars
Diose        2          1
Triose       3          2
Tetrose      4          3
Pentose      5          4
Hexose       6         12       At least 6 carbons are required to form a ring
Heptose      7       many       Rarely observed in nature
Octose       8       many       Unstable.  Not observered in nature.
"Number of sugars" refers to the number of different types of sugar molecules for each carbon number.

Each sugar molecule has two mirror-symmetric forms, the "D" and "L" form. Only the D forms are found in nature.

The following figures show all sugars up to 6 carbons. All can be metabolized by humans.

2 carbons:

Glycolaldehyde

3 carbons:

Glyceraldehyde
Dihydroxyacetone

4 carbons:

Erythrose
Threrose
Erythrulose

5 carbons:

Ribose
Arabinose
Lyxose
Xylose

6 carbons:

Glucose
Galactose
Mannose
Allose
Altrose
Gulose
Idose
Talose

Fructose
Sorbose
Psichose
Tagatose

         Energy  Sweetness

Succrose   1.00    1.00      Benchmark
Glucose             .74
Maltose             .32
Galactose           .32
Lactose             .16
Allose
Altrose
Mannose
Fructose           1.73
Psichose            .70
Tagatose    .38     .92
Sorbose            1.0
Honey               .97

Complex sugars
Monosaccharde:   1 sugar molecule
Disaccharide:    2 monosaccharides
Polysaccharide:  More than 2 monosaccharides, such as starch and cellulose
Sucrose
Maltose
Lactose
Lactulose
Trehalose
Sucrose    =  Glucose     + Fructose
Maltose    =  Glucose     + Glucose
Lactose    =  Galactose   + Glucose
Lactulose  =  Galactoce   + Fructose
Trehalose  =  Glucose     + Glucose
Cellobiose =  Glucose     + Glucose
Chitobiose =  Glucosamine + Glucosamine
Starch and cellulose are long chains of glucose molecules.

Starch
Cellulose


Synthesis


Metabolism

Fatty acid with 16 carbons
Sugar (glucose)
Acetyl
Pyruvic acid
H2O
CO2

Fatty acids and sugars are metabolized in the following stages, with each stage yielding energy.

Fatty acid    →     Acetyl      →     CO2 and H2O

Sugar         →     Pyruvate    →     CO2 and H2O

Blood delivers fatty acids to cells.

The citric acid cycle (Krebs cycle) converts acetyl or pyrovate into H2O and CO2. Coenzyme-A carries the acetyl around.


Fat metabolism

A fat molecule is converted into a fatty acid by lipolysis, and then the fatty acid is converted into acetyl by beta oxydation, and then the acetyl is converted into H2O and CO2 by the citric acid cycle.

Beta oxidation cleaves 2 carbons from a fatty acid, which becomes acetyl. This process is repeated until te entire fatty acid has been converted into acetyls.

The steps of beta oxidation are:


Sugar metabolism (glycolysis)

Glycolysis converts a glucose molecule into 2 pyrovate molecules. A summary of the reaction showing only the starting and ending points is:

The full reaction is:


Citric acid cycle

Citric acid

The citric acid cycle (Krebs cycle) converts acetyl or pyrovate into H2O and CO2.

Fat metabolism oxidizes a carbon chain so that the chain can be split into acetyl. The strategy of the citric acid cycle is to further oxidize the acetyl (now a part of citrate) so that the remaining carbon bonds in the acetyl can be broken.


Alcohol

An alcohol is a carbon chain with one OH attached.

Methanol
Ethanol
Propanol
Isopropanol
Butanol

          Carbons
Methanol     1       Toxic
Ethanol      2       Inebriating
Propanol     3       3 times more inebriating than ethanol
Isopropanol  3       Toxic
Butanol      4       6 times more inebriating than ethanol

Fatty acids (carboxylic acids)

Formic acid
Acetic acid
Palmitic acid

Palmitic acid has 16 carbons and is the most common fatty acid found in food.

Carbons
   1
   2    Vinegar
   3
   4    Found in butter
   8    Found in coconuts
  10    Found in coconuts
  12    Found in coconuts
  16    Most common fatty acid.  Found in palm oil
  18    Found in chocolate
  20    Found in peanut oil

Metabolism molecules

NADH
FAD
Guanosine triphosphate
Glucosamine
Acetic acid
Citric acid
Vitamin C


Toxic molecules

Formaldehyde

             LD50
            (mg/kg)
CO                     Carbon monoxide
HCN             6.4    Hydrogen cyanide
CH2O                   Methanol
CH2O                   Formaldehyde
H2S                    Hydrogen sulfide
NO2                    Nitrite
Cl2                    Chlorine
Fl2                    Fluorine
Ethanol      7060
Salt         3000
Caffeine      192
Aspirin       200
NaNO2         180      Sodium nitrite
Cobalt         80
NaF            52
Capsaicin      47      Chili pepper
Mercury        41
Arsenic        13
Nicotine         .8
Bromine
C2N2
PH3
SiCl4
Almost anything with fluorine or bromine is toxic.

Weakly toxic:

C2H2          Acetylene.  Inebriating
C3H6          Propene.  Inebriating

Opsins

Opsin         Wavelength  Humans
                 (nm)
RH1               500     White  Black/White
RH2               600            Black/White.  Extinct in mammals
OPN1LW            564     Red    Once possessed by mammals, then lost by most
OPN1MW            534     Green  All mammals
OPN1SW            440     Blue   All mammals
SWS2              480            Extinct in mammals
VA                500            Vertebrates except mammals.  Vertebrae ancient opsin.
Parapinopsin UV   365            Catfish
Parapinopsin Blue 470            Catfish and lamphrey
Pareitopsin       522            Lizards
Panopsin Cyan     500            Fish vision.  Found in the brains of humans
Panopsin Blue     450            Fish vision.  Found in the brains of humans
Neuropsin         380            Bird vision.  Found in the brains of humans
Melanopsin        480            Found in the brains of humans
Retinal G                        Found in the brains of humans

Porphyrins

Heme cofactor carrying an iron atom
Pyrrole

Metals are held by a cofactor, which is held by a protein. Many cofactors are porphyrin rings conposed of 4 pyrroles. Examples of porphyrins:

Porphin (Iron)
Corrin (Cobalt)
Corphin (Nickel)
Chlorophyll building blocks (Magnesium)

Porphin resonance
Porphin is an aromatic molecule because it is flat and because it resonates between different electronic states.


Hemoglobin

Heme A
Heme B
Heme C
Heme O
Hemo B
Hemoglobin
Myoglobin

Superoxide

Oxygen bonds to the iron in a heme molecule and becomes superoxide.
Hemoglobin is a set of 4 helix proteins that carry 4 iron ligands, and each iron ligand carries 1 oxygen molecule.
Human hemoglobin is composed mostly of heme B.
The oxygen density of hemoglobin is 70 times the solubility of oxygen in water.

Hemoglobin fraction of red blood cells   =  .96      (dry weight)
Hemoglobin fraction of red blood cells   =  .35      (including water)
Oxygen capacity of hemoglobin            = 1.34 Liters of oxygen / kg hemoglobin
Iron ligands per hemoglobin              =    4
O2 molecules per ion ligand              =    1

Chlorophyll

Chlorophyll A

Chlorophyll A
Chlorophyll B
Chlorophyll D

Chlorophyll C1
Chlorophyll C2
Chlorophyll F

All chlorophyll uses magnesium.

A      Universal
B      Plants
C1     Algae
C2     Algae
D      Cyanobacteria
F      Cyanobacteria

Zinc fingers

Zinc stabilizes the proteins that manipulate DNA and RNA.


Metal
Carbonic anhydrase
Element   Humans  Cofactor  Function

Hydrogen    *
Helium                      No biological role
Lithium                     No biological role
Beryllium                   Toxic becauseit displaces magnesium in proteins
Boron       *               Plant cell walls.  Metabolism of calcium in plants & animals
Magnesium   *     Chlorin   Chlorophyll
Scandium                    No biological role
Titanium                    No biological role
Vanadium                    Found only in rare bacteria.
Chromium                    No biological role
Manganese   *               Superoxide dimutase.  Converts superoxide to oxygen
Iron        *     Porphin   Hemoglobin
Cobalt      *     Corrin    Cobalamin (Vitamin B12)
Nickel            Corphin   Coenzyme F430 (Creates methane. Found only in archaea)
Copper      *     Heme      Cytochrome C oxidase. Electron transport chain
                            Hemocyanin, an alternative to hemoglobin used by some animals
                            Hemoglobin carries 4 times as much oxygen as hemocyanin
                            Plastocyanin protein, used in photosynthesis
                            Sometimes used in superoxide dimutase
Zinc        *               Component of proteins that manipulate DNA and RNA (Zinc fingers)
                            Component of carbonic anhydrase, which interconverts CO2 and HCO3
                            Metallothionein proteins, which bind to metals such as
                            zinc, copper, selenium cadmium, mercury, silver, and arsenic
Molybdenum                  Nitrogen fixase. Convert N2 to NH3
Selenium    *               Component of the amino acide selenocysteine
Bromine     *               Limited role
Iodine      *               Component of thyroxine and triiodotyronine, which
                            regulate metabolic rate
Lead                        Toxic because it displaces calcium in bones
Thyroxine
Triiodothyronine

Antioxidation

Superoxide dimutase
Superoxide dimutase, manganese in purple
Peroxidase

Bicarbonate
Carbonic acid
Hydrogen peroxide

Superoxide dimutase converts superoxide to oxygen or hydrogen peroxide.

The peroxidase enzyme decomposes hydrogen peroxide to water. Peroxidase contains the selenocysteine amino acid, which contains selenium.


Nitrogen fixation

Nitrogen fixase uses an iron-molybdenum cofactor.


Selenium

Selenocysteine

Selenium is a component of the amino acid selenocysteine.


Copper
Hemocyanin
Copper group without an oxygen
Copper group with an oxygen

The hemocyanin protein uses copper to carry oxygen. It has an oxygen density that is 1/4 of hemoglobin.

Plastocyanin is a copper-containing protein used in photosynthesis.

Plastocyanin


Lignin

Lignin is the structural component of wood.


Oxidizer clusters

Ozone
Trisulfur

Nitric oxide
Nitrous oxide (laughing gas)
Dinitrogen dioxide

Dinitrogen trioxide crystal

Sulfur monoxide
Sulfur dioxide
Disulfur dioxide

Phosphorus trioxide crystal
Phosphorus pentoxide

Potassium oxide
Selenium oxide


Ancient metallurgy

Stone
Copper
Bronze
Iron
Carbon

Gold and silver were known since antiquity because they occur naturally in pure form. Gold mining started in 6000 BCE and silver smelting started in 4000 BCE.

Iron can occasionally be found as iron meteorites.

Gold nugget
Silver nugget
Iron meteorite

Copper was discovered around 7500 BCE by smelting copper minerals in a wood fire. Around 3200 BCE it was found that copper is strenghened by tin, and this is bronze. Around 2000 BCE it was found that copper is also strengthed by zinc, and this is brass.

The earliest metals were smeltable with a wood fire and they consist of copper, lead, silver, tin, zinc, and mercury. They come from the following minerals:

Lead. Galena. PbS
Copper. Chalcocite. Cu2S
Silver. Acanthite. Ag2S
Tin. Cassiterite. SnO2
Zinc. Sphalerite. ZnS
Mercury. Cinnabar. HgS

The next metal to be discovered was iron (c. 1200 BC), which requires a bellows-fed coal fire to smelt.

Iron. Hematite. Fe2O3
Iron. Pyrite. FeS2

No new metals were discovered until cobalt in 1735. Once cobalt was discovered, it was realized that new minerals may have new metals, and the race was on to find new minerals. This gave nickel, chromium, manganese, molybdenum, and tungsten.

Cobalt. Cobaltite. CoAsS
Nickel. Millerite. NiS
Chromium. Chromite. FeCr2O4
Manganese. Pyrolusite. MnO2
Molybdenum. Molybdenite. MoS2
Tungsten. Wolframite. FeWO4

Chromium is lighter and stronger than steel and was discovered in 1797. It satisfies the properties of mithril from "Lord of the Rings" and Valyrian steel from "Game of Thrones". There's no reason chromium couldn't have been discovered earlier.

Coal smelting can't produce the metals lighter than chromium. These need electrolysis. The battery was invented in 1799, enabling electrolysis, and the lighter metals were discovered shortly after. These include aluminum, magnesium, titanium, and beryllium. Once you have

Aluminum. Bauxite. Al(OH)3 and AlO(OH)
Mangesium. Magnesite. MgCO3
Titanium. Rutile. TiO2
Beryllium. Beryl. Be3Al2(SiO3)6

Carbon fiber eclipses metals. The present age could be called the carbon age. The carbon age became mature in 1987 when Jimmy Connors switched from a wood to a carbon racket.

The plot shows the strength of materials.

Alloys can be much stronger than pure metals.

Wood rivals alloys for strength.


Currency

Gold was the densest element known until the discovery of platinun in 1735. It was useful as an uncounterfeitable currency until the discovery of tungsten in 1783, which has the same density as gold. Today, we could use iridium, platinum, or rhenium as an uncounterfeitable currency.


Modern chemistry and the discovery of elements

Prior to 1800, metals were obtained by smelting minerals, and the known metals were gold, silver, copper, iron, tin, zinc, mercury, cobalt, manganese, chromium, molybdenum, and tungsten. Elements to the left of chromium titanium and scandium cant's be obtained by smelting, and neither can aluminum, magnesium, and beryllium. They require electrolysis, which was enabled by Volta's invention of the battery in 1799.

Prior to 1800, few elements were known in pure form. Electrolyis enabled the isolation of most of the rest of the elements. The periodic table then became obvious and was discovered by Mendeleev 1871. The battery launched modern chemistry, and the battery could potentially have been invented much earlier.

Electrolysis enabled the isolation of sodium and potassium in 1807, and these were used to smelt metals that can't be smelted with carbon.

         Discovery   Method of             Source
          (year)     discovery

Carbon     Ancient   Naturally occuring
Gold       Ancient   Naturally occuring
Silver     Ancient   Naturally occuring
Sulfur     Ancient   Naturally occuring
Lead         -6500   Smelt with carbon     Galena       PbS
Copper       -5000   Smelt with carbon     Chalcocite   Cu2S
Bronze (As)  -4200   Copper + Arsenic      Realgar      As4S4
Tin          -3200   Smelt with carbon     Calamine     ZnCO3
Bronze (Sn)  -3200   Copper + Tin
Brass        -2000   Copper + Zinc         Sphalerite   ZnS
Mercury      -2000   Heat the sulfide      Cinnabar     HgS
Iron         -1200   Smelt with carbon     Hematite     Fe2O3
Arsenic       1250   Heat the sulfide      Orpiment     As2S3
Zinc          1300   Smelt with wool       Calamine     ZnCO3 (smithsonite) & Zn4Si2O7(OH)2·H2O (hemimorphite)
Antimony      1540   Smelt with iron       Stibnite     Sb2S3
Phosphorus    1669   Heat NaPO3 Excrement
Cobalt        1735   Smelt with carbon     Cobaltite    CoAsS
Platinum      1735   Naturally occuring
Nickel        1751   Smelt with carbon     Nickeline    NiAs
Bismuth       1753   Isolated from lead
Hydrogen      1766   Hot iron + steam      Water
Oxygen        1771   Heat HgO
Nitrogen      1772   Isolated from air
Manganese     1774   Smelt with carbon     Pyrolusite   MnO2
Molybdenum    1781   Smelt with carbon     Molybdenite  MoS2
Tungsten      1783   Smelt with carbon     Wolframite   (Fe,Mn)WO4
Chromium      1797   Smelt with carbon     Crocoite     PbCrO4
Palladium     1802   Isolated from Pt
Osmium        1803   Isolated from Pt
Iridium       1803   Isolated from Pt
Rhodium       1804   Isolated from Pt
Sodium        1807   Electrolysis
Potassium     1807   Electrolysis
Magnesium     1808   Electrolysis          Magnesia     MgCO3
Cadmium       1817   Isolated from zinc
Lithium       1821   Electrolysis of LiO2  Petalite     LiAlSi4O10
Zirconium     1824   Smelt with potassium  Zircon       ZrSiO4
Aluminum      1827   Smelt with potassium
Silicon       1823   Smelt with potassium
Beryllium     1828   Smelt with potassium  Beryl        Be3Al2Si6O18
Thorium       1929   Smelt with potassium  Gadolinite   (Ce,La,Nd,Y)2FeBe2Si2O10
Vanadium      1831   Smelt VCl2 with H2    Vanadinite   Pb5(VO4)3Cl
Uranium       1841   Smelt with potassium  Uranite      UO2
Ruthenium     1844   Isolated from Pt
Tantalum      1864   Smelt with hydrogen   Tantalite    [(Fe,Mn)Ta2O6]
Niobium       1864   Smelt with hydrogen   Tantalite    [(Fe,Mn)Ta2O6]
Fluorine      1886   Electrolysis
Helium        1895   From uranium ore
Titanium      1910   Smelt with sodium     Ilmenite     FeTiO3
Hafnium       1924   Isolated from zirconium
Rhenium       1928   Isolated from Pt
Scandium      1937   Electrolysis          Gadolinite   FeTiO3

History of mineralogy

 -384  -322   Aristotle. Wrote "Meteorology"
 -370  -285   Theophrastus. Wrote "De Mineralibus"
         77   Pliny the Elder publishes "Natural History"
  973  1050   Al Biruni. Published "Gems"
       1546   Georgius Agricola publishes "On the Nature of Rocks"
       1556   Georgius Agricola publishes "On Metals"
       1609   de Boodt publishes a catalog of minerals
       1669   Brand: Discovery of phosphorus
       1714   John Woodward publishes "Naturalis historia telluris illustrata & aucta", a mineral catalog
       1735   Brandt: Discovery of cobalt
       1777   Lavoisier: Discovery of sulfur
       1778   Lavoisier: Discovery of oxygen and prediction of silicon
       1783   Lavoisier: Discovery of hydrogen
       1784   T. Olof Bergman publishes "Manuel du mineralogiste, ou sciagraphie du regne mineral",
              and founds analytical chemistry
       1778   Lavoisier: Discovery of oxygen
       1801   Rene Just Huay publishes "Traite de Mineralogie", founding crystallography
       1811   Avogadro publishes "Avogadro's law"
       1860   The Karlsruhe Congress publishes a table of atomic weights
       1869   Mendeleev publishes the periodic table

Metals known since antiquity

For a metal, the stiffness is characterized by the "shear strength" and the sword worthiness is characterized by the shear strength over the density (the "strength to weight ratio"). For example for iron,

Shear modulus    =  S         =   82 GJoules/meter3
Density          =  D         = 7900 kg/meter3
Sword worthiness =  Q  = S/D  = 10.4 MJoules/kg

Metals

This plot includes all metals with a strength/density at least as large as lead, plus mercury. Beryllium is beyond the top of the plot.


Wootz steel

-600  Wootz steel developed in India and is renowned as the finest steel in the world.
1700  The technique for making Wootz steel is lost.
1790  Wootz steel begins to be studied by the British Royal Society.
1838  Anosov replicates Wootz steel.
Wootz steel is a mix of two phases: martensite (crystalline iron with .5% carbon), and cementite (iron carbide, Fe, 6.7% carbon).

Iron meteorites

In prehistoric times iron meteorites were the only source of metallic iron. They consist of 90% iron and 10% nickel.


Alloys

Copper
Orichalcum (gold + copper)
Gold

Alloy of gold, silver, and copper


Superstrong amorphous alloys

Crystal, polycrystal, amorphous

New alloys have been discovered that are stronger and ligher than diamond. These alloys have an amorphous structure rather than the crystalline structure of conventional alloys. A crystaline alloy tends to be weak at the boundaries between crystals and this limits its strength. Amorphous alloys don't have these weaknesses and can be stronger.

Pure metals and alloys consisting of 2 or 3 different metals tend to be crystaline while alloys with 5 or more metals tend to be amorphous. The new superalloys are mixes of at least 5 different metals.

A material's strength is characterized by the "yield strength" and the quality is the ratio of the yield strength to the density. This is often referred to as the "strength to weight ratio".

Yield strength  =  Y            (Pascals)
Density         =  D            (kg/meter3)
Quality         =  Q  =  Y/D    (Joules/kg)
The strongest allyos are:
       Yield strength   Density   Quality
       (GPa)        (g/cm3)    (MJoule/kg)

Magnesium + Lithium             .14        1.43        98
Magnesium + Y2O3                .31        1.76       177
Aluminum  + Beryllium           .41        2.27       181
Amorphous LiMgAlScTi           1.97        2.67       738
Diamond                        1.6         3.5        457
Titanium  + AlVCrMo            1.3         4.6        261
Amorphous AlCrFeCoNiTi         2.26        6.5        377
Steel     + Cobalt, Nickel     2.07        8.6        241
Amorphous VNbMoTaW             1.22       12.3         99
Molybdenum+ Tungsten, Hafnium  1.8        14.3        126
The strongest pure metals are weaker than the strongest alloys.
       Yield strength   Density   Quality
       (GPa)        (g/cm3)    (MJoule/kg)

Magnesium                        .10       1.74        57
Beryllium                        .34       1.85       184
Aluminum                         .02       2.70         7
Titanium                         .22       4.51        49
Chromium                         .14       7.15        20
Iron                             .10       7.87        13
Cobalt                           .48       8.90        54
Molybdenum                       .25      10.28        24
Tungsten                         .95      19.25        49

Alloy types
Beryllium + Li           →  Doesn't exist. The atoms don't mix
Beryllium + Al           →  Improves strength
Magnesium + Li           →  Weaker and lighter than pure Mg. Lightest existing alloy
Magnesium + Be           →  Only tiny amounts of beryllium can be added to magnesium
Magnesium + Carbon tubes →  Improves strength, with an optimal tube fraction of 1%
Aluminum  + Li,Mg,Be,Sc  →  Stronger and lighter than aluminum
Titanium  + Li,Mg,Sc     →  Stronger and lighter than titanium
Steel     + Cr,Mo        →  Stronger and more uncorrodable than steel. "Chromoly"
Copper    + Be           →  Stronger than beryllium and is unsparkable

High-temperature metals (refractory metals)
          Melting point (Celsius)

Tungsten    3422
Rhenium     3186
Osmium      3033
Tantalum    3017
Molybdenum  2623
Niobium     2477
Iridium     2446
Ruthenium   2334
Hafnium     2233
Technetium  2157
Rhodium     1964
Vanadium    1910
Chromium    1907

High-temperature superalloys

Most alloys weaken with increasing temperature except for a small subset called "superalloys" that strengthen with temperature, such as Ni3Al and Co3Al. This is called the "yield strength anomaly".

Nickel alloys in jet engines have a surface temperature of 1150 Celsius and a bulk temperature of 980 Celsius. This is the limiting element for jet engine performance. Half the mass of a jet engine is superalloy.

Current engines use Nickel superalloys and Cobalt superalloys are under development that will perform even better.

Yield strength in GPa as a function of Celsius temperature.

                   20   600   800  900  1000  1100 1200  1400  1600 1800  1900  Celsius

VNbMoTaW          1.22         .84        .82       .75  .66   .48   .4
AlMohNbTahTiZr    2.0   1.87  1.60  1.2   .74  .7   .25
Nickel superalloy 1.05        1.20   .90  .60  .38  .15
Tungsten           .95   .42   .39        .34  .31  .28  .25   .10   .08  .04
Below 1100 Celsius AlMohNbTahTiZr has the best strength-to-mass ratio and above this VNbMoTaW has the best ratio. Both alloys supersede nickel superalloy and both outperform tungsten, the metal with the highest melting point. Data:   
Entropy, nickel superalloy
Copper alloys
                  Yield strength (GPa)

Copper                  .27
Brass                   .41     30% zinc
Bronze                  .30     5% tin
Phosphor bronze         .69     10% tin, .25% phosphorus
Copper + beryllium     1.2      2% beryllium, .3% cobalt
Copper + nickel + zinc  .48     18% nickel, 17% zinc
Copper + nickel         .40     10% nickel, 1.25% iron, .4% manganese
Copper + aluminum       .17     8% aluminum

Bells and cymbals

Bells and cymbals are made from bell bronze, 4 parts copper and 1 part tin.


Bonds

Bond energy

The "atomization energy" is the energy required to extract an atom from an element in its raw form. For example,

Atom     Form of     Atomization energy
       raw element     kJoules/mole

 H         H2            218
 He        He              0       Noble elements are already atomized
 Be        Metal         159
 Li        Metal         324
 B         Boron solid   563
 C         Graphite      717
 N         N2            473
 O         O2            249
 F         F2             79
 Ne        Ne              0
 Na        Metal         107
 Mg        Metal         146
 Al        Metal         326
 Si        Crystal       456
 P         Solid         315
 S         Solid         279
 Cl        Cl2           122
 Fe        Metal         415

Gibbs energy, enthalpy, and entropy

Pressure         =  P
Volume           =  V
Entropy          =  S
Temperature      =  T
Internal energy  =  E
Enthalpy         =  H  =  E + P V
Gibbs energy     =  G  =  E + P V - T S
Helmholtz energy =  A  =  E - T S
The Gibbs energy is the energy required to assemble a molecule from raw elements at standard temperatue (298.2 Kelvin) and pressure (1 bar). The Gibbs energy of raw elements is defined as zero.
Units

Energy             =  E                Joules
Electron volt      =  e  =  1.602e-19  Joules          =  96.47 kJoules/mole
Avogadro number    =  A  =  6.0221e23  particles/mole
Atomic mass unit   =  m  =  1.6605e-27 kg
Boltzmann constant =  k  =  1.3806e-23 Joules/Kelvin

Energy of molecules

The atomization energy of H2O is -971 kJ/mole.

H2O   →   H2  +  ½ O2  -  286 kJ/mole
      →   2 H +  O            -  286 - 2*218 - 249 kJ/mole
      →   2 H +  O            -  971 kJ/mole

Gibbs energy, enthalpy, and entropy

         Gibbs   Enthalpy    Entropy    Atomize
        kJ/mole  kJ/mole    kJ/mole/K   kJ/mole

H2          0        0      .131         -436
C graphite  0        0      .00574       -717
N2          0        0      .1915        -946
O2          0        0      .2050        -498

H2O      -237.24  -285.83   .06995       -716        -286 - 2*218 - 249
CO2      -394.4   -393.5    .214        -1609        -394 - 717 - 498

CH4                -74.87   .1862       -1664         -75 - 717 - 872
C2H6               -83.7
C3H8              -104.6
C4H10             -125.5
C5H12             -146.9
C6H14             -167.4
C7H16             -187.9
C8H18             -208.4
C12H26            -352.1    .4907
C16H34            -456.3    .5862


Bond energies
                eV   kJoules/mole

H     -  H
HO    -  H             493.4
O     -  H             424.4
CH3   -  H     4.52    435
CH2   -  H             444
CH    -  H             444
C     -  H             339
C2H5  -  H             423
C2H   -  H             556
C6H5  -  H             473
CH3   -  CH3   3.64    351
CH2   =  CH2           622
CH    ≡  CH            837
C2H3  -  H             464
CH2CHCH2 - H           372

Table of energies
        Gibbs      Enthalpy       Entropy
     kJoule/mole  kJoule/mole  kJoule/mole/K

H2          0          0      .131
C graphite  0          0      .00574
C diamond   2.90       1.90   .00238
N2          0          0      .1915
O2          0          0      .2050
Ne          0          0      .1464
Na          0          0      .0512
Mg          0          0      .0327
Al          0          0      .0283
Al          0          0      .0283
Si          0          0      .0188
P4          0          0      .1644
S           0          0      .0318
Cl2         0          0      .223
K           0          0      .0642
Ca          0          0      .0414
Ar          0          0      .155
Cr          0          0      .0238
Mn          0          0      .0327
Fe          0          0      .0273
Ni          0          0      .0299
Cu          0          0      .0332
Zn          0          0      .0416
Ag          0          0      .0426
Sn          0          0      .0516
Hg          0          0      .0760
Pb          0          0      .0648

H2O      -237.24   -285.83    .06995
CH4                 -74.87    .1862         Combustion =  -890.7
C2H6                -83.7                   Combustion = -1561
C3H8               -104.6
C4H10              -125.5
C5H12              -146.9
C6H14              -167.4
C7H16              -187.9
C8H18              -208.4
C12H26             -352.1     .4907         Combustion =-7901.7
C16H34             -456.3     .5862         Combustion =-10699
N2O                  82.05    .2200
H2O2               -187.80
N2O4                  9.16    .3043
N2H4                 50.63    .1215
NH4NO3
NH4ClO4
HNO3               -207       .146
Li2O     -561.9     -20.01    .03789
C4H8N8O8                                     HMX explosive
BeO      -579.1
B2O3    -1184
CO2      -394.4    -393.5     .214
CO       -137.2    -110.5     .198
NO                   90.2     .211
NO2                  33.2     .240
Na2O     -377
MgO      -596.3    -601.6     .0269
Al2O3   -1582.3    -1675.7    .0509
SiO2     -856.6    -910.9     .0418          Quartz
P2O5
SO2                -296.8     .2481
SO3                -395.7     .2567
K2O      -322.2
CaO      -533.0    -634.9     .0398
TiO2     -852.7
Ti2O3   -1448
VO       -404.2
V2O3    -1139.3
V2O4    -1318.4
Cr2O3   -1053.1   -1139.7     .0812
MnO2     -465.2
MnO      -362.9    -385.2     .0597
MnO2               -520.0     .0530
Fe2O3    -741.0    -824.2     .0874
Fe3O4   -1014     -1118.4     .0146
CoO      -214.2
Co3O4    -795.0
NiO      -211.7    -239.7     .0380
CuO      -129.7    -157.3     .0426
Cu2O     -146.0    -168.6     .0931
ZnO      -318.2    -350.5     .0436
MoO2     -533.0
MoO3     -668.0
Ag2O      -11.2
PdO
SnO2               -577.6     .0523
CdO      -228.4
WO2      -533.9
WO3      -764.1
HgO       -58.5     -90.8     .0703
PbO                -219.0     .0665
PbO2     -219.0    -277.4     .0686
UO2

CuS                  -53.1    .0665
Cu2S                 -79.5    .1209
ZnS2                -206.0    .0577

CaCO3   -1128      -1207      .090

H+ (aq)     0          0      0
OH- (aq) -157.2     -230.0   -.0108
H2O (l)  -237.2     -285.8    .0699
H2O (g)  -228.6     -241.8    .1888
Cu+                   71.7    .0406
Cu+2                  64.8   -.0996
Ca+2                -543.0   -.0531
Ag+ (aq)             105.8    .0727
Al+3 (aq)           -538.4   -.3217
CO3-2               -675.2   -.0569
NH3 (g)   -16.4      -46.1
NaCl (s) -384.1     -411.2    .0721

        Gibbs      Enthalpy       Entropy
     kJoule/mole  kJoule/mole  kJoule/mole/K

Bond energy of hydrides
Target  Molecule  Bonds  Bond   1st   2nd   3rd   4th
 atom                   energy  bond  bond  bond  bond
                         (eV)   (eV)  (eV)  (eV)  (eV)

  H      H2         1    4.52   4.52
  He     -          0     -      -
  Li     LiH        1    2.56   2.56
  Be     BeH2       2     ?     2.35   ?
  B      BH3        3     ?     3.43   ?     ?
  C      CH4        4    4.31   3.52  4.61  4.61  4.52
  N      NH3        3    3.90   3.26  3.91  4.52
  O      H2O        2    4.76   4.41  5.12
  F      HF         1    5.90   4.90
  Ne     -          0     -      -
  Na     NaH        1    2.09   2.09
  Mg     MgH2       2     ?     2.04   ?
  Al     AlH3       3     ?     2.96   ?     ?
  Si     SiH4       4     ?     3.10   ?     ?    4.08
  P      PH3        3     ?     3.56   ?     ?
  S      H2S        2    3.76   3.57  3.95
  Cl     HCl        1    4.48   4.48
  Ar     -          0     -      -
  K      KH         i    1.90   1.90
  Ca     CaH2       i     ?     1.74   ?
  Ga                      ?      ?     ?     ?
  Ge                      ?     3.36   ?     ?     ?
  As                      ?     2.82   ?     ?
  Se     SeH2       2     ?     3.17   ?
  Br     HBr        1    3.80   3.80
  Kr     -          0     -      -
  In                      ?      ?     ?     ?
  Sn                      ?     2.77   ?     ?     ?
  Sb                      ?      ?     ?     ?
  Te     TeH2       2     ?     2.78   ?
  I      HI         1    3.10   3.10
  Xe     -          0     -      -

Bond energies in eV
      Single  Double  Triple  Quadruple

B  B    3.04
B  C    3.69
B  O    5.56
C  C    3.65   6.45    8.68   6.32
C  N    3.19   6.38    9.19
C  O    3.73   7.7    11.11
C  Si   3.30
C  P    2.74
C  S    2.82   5.94
N  N    1.76   4.33    9.79
N  O    2.08   6.29
N  Si   3.70
N  P
N  S
O  O    1.50   5.15
O  Si   4.69
O  P    3.47   5.64
O  S           5.41
Si Si   2.30
Si S    3.04
Si P
P  P    2.08
P  S           3.47
S  S    2.34   4.41
H  H    4.52
H  C    4.25
H  N    4.05
H  O    3.79
H  F    5.89
H  Si   3.30
H  P    3.34
H  S    3.76
H  Cl   4.48

Fuel for oxygen
       Enthalpy
       kJ/mole

H2O     -285.83
Li2O     -20.01
BeO     -609.4
CO2     -393.5
MgO     -601.6
Al2O3  -1675.7
Fe2O3   -824.2

Oxidizer
       Enthalpy  Entropy   Boil   Density
       kJ/mole   kJ/mole  Kelvin

O2          0       .2050
O3        142.67    .2389   161
H2O2     -187.80
NO         90.2     .211
NO2        33.2     .240
HNO3     -207       .146    356    1.51
N2O3       91.20    .3146   277    1.45
N2O4        9.16
N2O5      -43.1     .1782   320    1.64     solid
N2O        82.05    .2200
SO2      -296.8     .2481   265
SO3      -395.7     .2567
N2H4       50.63    .1215
NH4NO3   -365.6             483    1.72
NH4ClO4  -295.77    .1842
C4H8N8O8  296.16                            HMX explosive
NH3OHNO3

Metal smelting

Prehistoric-style smelter

Most metals are in oxidized form. The only metals that can be found in pure form are gold, silver, copper, platinum, palladium, osmium, and iridium.

Smelting is a process for removing the oxygen to produce pure metal. The ore is heated in a coal furnace and the carbon seizes the oxygen from the metal. For copper,

Cu2O + C  →  2 Cu + CO
At low temperature copper stays in the form of Cu2O and at high temperature it gives the oxygen to carbon and becomes pure copper.

For iron, the oxidation state is reduced in 3 stages until the pure iron is left behind.

3 Fe2O3 + C  →  2 Fe3O4 + CO
Fe3O4   + C  →  3 FeO   + CO
FeO     + C  →    Fe   + CO
Oxidation state  =  Number of electrons each iron atom gives to oxygen

       Oxidation state
CuO          2
Cu2O         1
Cu           0
Fe2O3        3
Fe3O4       8/3
FeO          2
Fe           0

Smelting temperature

The following table gives the temperature required to smelt each element with carbon.

        Smelt  Method  Year  Abundance
         (C)                   (ppm)

Gold        <0   *   Ancient      .0031
Silver      <0   *   Ancient      .08
Platinum    <0   *    1735        .0037
Mercury     <0  heat -2000        .067
Palladium   <0  chem  1802        .0063
Copper      80   C   -5000      68
Sulfur     200   *   Ancient   420
Lead       350   C   -6500      10
Nickel     500   C    1751      90
Cadmium    500   C    1817        .15
Cobalt     525   ?    1735      30
Tin        725   C   -3200       2.2
Iron       750   C   -1000   63000
Phosphorus 750  heat  1669   10000
Tungsten   850   C    1783    1100
Potassium  850   e-   1807   15000
Zinc       975   C    1746      79
Sodium    1000   e-   1807   23000
Chromium  1250   C    1797     140
Niobium   1300   H    1864      17
Manganese 1450   C    1774    1120
Vanadium  1550   ?    1831     190
Silicon   1575   K    1823  270000
Titanium  1650   Na   1910   66000
Magnesium 1875   e-   1808   29000
Lithium   1900   e-   1821      17
Aluminum  2000   K    1827   82000
Uranium   2000   K    1841       1.8
Beryllium 2350   K    1828       1.9

Smelt:      Temperature required to smelt with carbon
Method:     Method used to purify the metal when it was first discovered
            *:  The element occurs in its pure form naturally
            C:  Smelt with carbon
            K:  Smelt with potassium
            Na: Smelt with sodium
            H:  Smelt with hydrogen
            e-: Electrolysis
            heat:  Heat causes the oxide to decompose into pure metal. No carbon required.
            chem:  Chemical separation
Discovery:  Year the element was first obtained in pure form
Abundance:  Abundance in the Earth's crust in parts per million
Elements with a low carbon smelting temperature were discovered in ancient times unless the element was rare. Cobalt was discovered in 1735, the first new metal since antiquity, and this inspired scientists to smelt every known mineral in the hope that it would yield a new metal. By 1800 all the rare elements that were carbon smeltable were discovered.

The farther to the right on the periodic table, the lower the smelting temperature, a consequence of "electronegativity".

The battery was invented in 1800, launching the field of electrochemistry and enabling the the isolation of non-carbon-smeltable elements. Davy used electrolysis in 1807 to isolate sodium and potassium and then he used these metals to smelt other metals. To smelt beryllium with potassium, BeO + 2 K ↔ Be + K2O.

Titanium can't be carbon smelted because it forms the carbide Ti3C.

Data

For an expanded discussion of smelting physics, see jaymaron.com/metallurgy.html.


Thermite

Thermite is smelting with aluminum. For example, to smelt iron with aluminum,

Fe2O3 + 2 Al  →  2 Fe + Al2O3

Smelting reactions

The following table shows reactions that change the oxidation state of a metal. "M" stands for an arbitrary metal and the magnitudes are scaled to one mole of O2. The last two columns give the oxidation state of the metal on the left and right side of the reaction. An oxidation state of "0" is the pure metal and "M2O" has an oxidation state of "1".

                            Oxidation state   Oxidation state
                                at left          at right
 2  M2O   ↔  4  M     + O2        1                0
 4  MO    ↔  2  M2O   + O2        2                1
 2  M3O4  ↔  6  MO    + O2       8/3               2
 6  M2O3  ↔  4  M3O4  + O2        3               8/3
 2  M2O3  ↔  4  MO    + O2        3                2
 2  MO    ↔  2  M     + O2        2                0
2/3 M2O3  ↔ 4/3 M     + O2        3                0
 1  MO2   ↔  1  M     + O2        4                0
 2  MO2   ↔  2  MO    + O2        4                2

Minerals

These elements are not necessarily on the Science Olympiad list.

We list minerals by element, with the most abundant mineral for each element listed first.

Lithium

Spodumene: LiAl(SiO3)2
Stilbite: LiAlSi2O6
Tourmaline: (Ca,Na,K,)(Li,Mg,Fe+2,Fe+3,Mn+2,Al,Cr+3,V+3)3(Mg,Al,Fe+3,V+3,Cr+3)6((Si,Al,B)6O18)(BO3)3(OH,O)3(OH,F,O)

Beryllium

Beryl: Be3Al2(SiO3)6
Morganite: Be3Al2(SiO3)6
Emerald

Carbon

Diamond: C

Sodium

Halite: NaCl

Magnesium

Periclase: MgO
Magnesite: MgCO3
Dolomite: CaMg(CO3)2
Peridot: (Mg,Fe)2SiO4
Spinel: MgAl2O4
Spinel: MgAl2O4

Aluminum

Bauxite: Al(OH)3 and AlO(OH)
Alumstone: KAl3(SO4)2(OH)6
Muscovite mica: KAl2(AlSi3O10)(F,OH)2 or KF2(Al2O3)3(SiO2)6(H2O)
Corundum: Al2O3
Topaz: Al2SiO4(F,OH)2

Epidote: Ca2(Al2,Fe)(SiO4)(Si2O7)O(OH)
Jadeite: NaAlSi2O6
Albite: NaAlSi3O8
Amazonite: KAlSi3O8
Labradorite: (Na,Ca)(Al,Si)4O8

Silicon

Amethyst: SiO2
Quartz: SiO2
Citrine: SiO2
Opal: SiO2·nH2O
Agate: SiO2

Sulfur

Volcanic sulfur

Calcium

Fluorite: CaF2
Calcite: CaCO3
Satin Spar: CaSO4 · 2H2O
Selenite: CaSO4 · 2H2O
Aragonite: CaCO3
Pearl: CaCO3
Calcite: CaCO3

Titanium, vanadium, chomium, and manganese

Rutile: TiO2
Vanadinite: Pb5(VO4)3Cl
Chromite: FeCr2O4
Pyrolusite: MnO2
Rhodonite: MnSiO3
Rhodochrosite: MnCO3

Iron

Hematite: Fe2O3
Hematite: Fe2O3
Pyrite: FeS2
Iron meteorite
Goethite: FeO(OH)

Cobalt and nickel

Cobaltite: CoAsS
Millerite: NiS

Copper

Chalcocite: Cu2S
Chalcopyrite: CuFeS2
Malachite: Cu2CO3(OH)l2
Azurite: Cu3(CO3)2(OH)2
Bornite: Cu5FeS4
Turquoise: CuAl6(PO4)4(OH)8•4(H2O)

Zinc and germanium

Sphalerite: ZnS
Germanite: Cu26Fe4Ge4S32

Strontium, zirconium, molybdenum

Celestine: SrSO4
Strontianite: SrCO3
Zircon: ZrSiO4
Molybdenite: MoS2

Silver

Argentite: Ag2S
Acanthite: Ag2S
Silver nugget

Tin

Cassiterite: SnO2

Caesium, barium, rare-earths

Pollucite: (Cs,Na)2Al2Si4O12·2H2O
Barite: BaSO4
Monazite: (Ce,La,Nd,Th)PO4

Tungsten

Wolframite: FeWO4
Scheelite: WCaO4
Hubnerite: WMnO4

Platinum, gold, mercury, lead

Sperrylite: PtAs2
Platinum nugget
Gold nugget
Cinnabar: HgS
Galena: PbS
Anglesite: PbSO4
Thorite: (Th,U)SiO4


Spices

Cumin
Fennel
Caraway
Coriander
Cardamom
Fenugreek
Cubeb

Cashew
Pistachio
Walnut
Hazelnut
Peanut
Almond
Pine

Sesame
Poppy
Chia
Flax
Sunflower
Lotus

Black pepper
Mustard

Cumin
Turmermic
Paprika
Chili

Oregano
Basil
Bay
Coriander
Curry
Sage

Chive
Lemongrass
Tarragon
Arugula
Mint
Dill
Marjoram

Rosemary
Parsley
Saffron
Juniper

Bell pepper
Chili
Jalapeno
Cayenne
Habanero

Onion
Garlic
Clove
Galangal
Cinnamon
Vanilla

Portobello
Shiitake
Oyster
Morel
Enoki
Porcini
Truffle

Olea europaea
Kalamata
Arbequina
Belice

Grapefruit
Orange
Tangerine
Lemon
Lime
Kaffir lime
Key lime
Kiwi

Tomato
Avocado
Coconut
Egg
Olive oil

Milk cream
Sour cream
Butter
Cream cheese
Yogurt

Parmesan
Mozzarella
Reggiano
Asiago

Adzuki
Kidney
Red
Black
Pinto

Coffee
Cacao
Kola

Salt
Monosodium glutamate


Spices

Turmeric: curcumin
Cumin: cuminaldehyde
Chili: capsaicin
Mustard: allyl isotyiolcyanate

Bay: myrcene
Garlic and onion: allicin
Clove: eugenol

Raspberry ketone
Tangerine: tangeritin
Lemon: citral
Lemon peel: limonene

Chocolate: theobromine
Smoke: guaiacol
Cardamom: terpineol
Wintergreen: methyl salicylate

Hydrogen   White
Carbon     Black
Nitrogen   Blue
Oxygen     Red
Sulfur     Yellow
        Scoville scale (relative capsaicin content)

Ghost pepper     1000000
Trinidad         1000000      Trinidad moruga scorpion
Naga Morich      1000000
Habanero          250000
Cayenne pepper     40000
Malagueta pepper   40000
Tabasco            40000
Jalapeno            5000
Guajillo pepper     5000
Cubanelle            500
Banana pepper        500
Bell pepper           50
Pimento               50

Molecule        Relative hotness

Rresiniferatoxin   16000
Tinyatoxin          5300
Capsaicin             16         Chili pepper
Nonivamide             9.2       Chili pepper
Shogaol                 .16      Ginger
Piperine                .1       Black pepper
Gingerol                .06      Ginger
Capsiate                .016     Chili pepper
Caraway: carvone
Black tea: theaflavin
Cinnamon: cinnamaldehyde
Citrus: hesperidin
Fruit: quercetin

Mint: menthol
Juniper: pinene
Saffron: picrocrocin
Saffron: safranal
Wine: tannic acid

Black pepper: piperine
Oregano: carvacrol
Sesame: sesamol
Curry leaf: girinimbine
Aloe emodin
Whiskey lactone


Signalling molecules

Alcohol
Caffeine
Tetrahydrocannabinol
Nicotine

Adrenaline
Noadrenaline
Dopamine
Seratonin

Aspirin
Ibuprofen
Hydrocodone
Morphone

Vitamin A (beta carotene)
Vitamin A (retinol)
Vitamin C (ascorbic acid)
Vitamin D (cholecalciferol)


Opium

Opium poppies
Opium poppy

              Strength   Half life   Dose
                           hours      mg

Carfentanil     30000        7.7       .0003
Ohmefentanil     6300
Dihydroetorphine 4000                  .03
Etorphine        2000                  .006
Sufentanil        750        4.4       .015
Ocfentanil        180                  .06
Fentanyl           75         .04      .1
Oxymorphone         7        8       10
Hydromorphone       5        2.5      1.5    Dilaudid
Heroine             4.5      <.6      2.2    Diamorphine
Methadone           3.5     30       35
Oxycodone           1.5      4        6.7
Morphine            1        2.5     10
Hydrocodone         1        5       10      Vicodin
Codeine              .1      2.8    180
Naproxen             .0072  18     1380
Ibuprofen            .0045   2     2220
Aspirin              .0028   6     3600

Strength data


Poppy

The composition of a typical opium poppy is:

                %    First isolated

Morphine        10       1817          Used to produce heroine
Codeine          2       1832
Thebaine         8                     Used to produce hydrocodone and hydromorphone
Papaverine      14       1848          Not psychoactive
Noscapine        5       1820          Not psychoactive
Other alkaloiods  .1

Opioids

Codein
Hydrocodone
Hydrocodone
Morphine
Morphine
Oxycodone
Oxycodone

Methadone
methadone
Heroine
Heroine
Hydromorphone
Oxymorphone
Oxymorphone

Fentanyl
Fentanyl
Ocfentanil
Sufentanil
Sufentanil
Etorphine
Etorphine

Dihydroetorphine
Carfentanil


Explosives

Medieval-style black powder
Modern smokeless powder

               MJoules  Rocket  Shock  Density  Boil
                 /kg     km/s   km/s   g/cm3  Kelvin 

Beryllium+ O2    23.2   5.3
Aluminum + O2    15.5
Magnesium+ O2    14.8
Hydrogen + O2    13.2   4.56             .07    20
Kerosene + O3    12.9 
Octanitrocubane  11.2          10.6     1.95
Methane  + O2    11.1   3.80             .42   112  CH4
Octane   + O2    10.4                    .70   399  C8H18
Kerosene + O2    10.3   3.52             .80   410  C12H26
Dinitrodiazeno.   9.2          10.0     1.98
C6H6N12O12        9.1                   1.96        China Lake compound
Kerosene + H2O2   8.1   3.2
Kerosene + N2O4   8.0   2.62
HMX (Octogen)     8.0   3.05    9.1     1.86
RDX (Hexagen)     7.5   2.5     8.7     1.78
Al + NH4NO3       6.9
Nitroglycerine    7.2           8.1     1.59        Unstable
PLX               6.5                   1.14        95% CH3NO2 + 5% C2H4(NH2)2
Composition 4     6.3           8.04    1.59        91% RDX. "Plastic explosive"
Kerosene + N2O    6.18
Dynamite          5.9           7.2     1.48        75% Nitroglycerine + stabilizer
PETN              5.8           8.35    1.77
Smokeless powder  5.2           6.4     1.4         Used after 1884. Nitrocellulose
TNT               4.7           6.9     1.65        Trinitrotoluene
Al + Fe2O3        4.0                               Thermite
H2O2              2.7   1.59            1.45   423  Hydrogen peroxide
Black powder      2.6            .6     1.65        Used before 1884
Al + NH4ClO4            2.6
NH4ClO4                 2.5
N2O               1.86  1.76
N2H4              1.6   2.2             1.02   387  Hydrazine
Bombardier beetle  .4                               Hydroquinone + H2O2 + protein catalyst
N2O4               .10                  1.45   294

Rocket: Rocket exhaust speed
Shock:  Shock speed
Nitrocellulose
TNT
RDX
HMX
PETN
Octanitrocubane

Nitrocellulose
TNT
RDX
HMX
PETN
Octanitrocubane

Dinitrodiazenofuroxan
Nitromethane


High explosives

High explosives have a large shock velocity.


                MJoules   Shock  Density
                  /kg     km/s    g/cm3

Octanitrocubane    11.2   10.6     1.95
Dinitrodiazeno.     9.2   10.0     1.98
C6H6N12O12          9.1            1.96    China Lake compound
HMX (Octogen)       8.0    9.1     1.86
RDX (Hexagen)       7.5    8.7     1.78
PLX                 6.5            1.14    95% CH3NO2 + 5% C2H4(NH2)2
Composition 4       6.3    8.04    1.59    91% RDX. "Plastic explosive"
Dynamite            5.9    7.2     1.48    75% Nitroglycerine + stabilizer
PETN                5.8    8.35    1.77

Liquid oxygen

The best oxidizer is liquid oxygen, and the exhaust speed for various fuels when burned with oxygen is:

                Exhaust  Energy   Density of fuel + oxidizer
                 speed   /mass
                 km/s    MJ/kg      g/cm3

Hydrogen   H2      4.46   13.2    .32
Methane    CH4     3.80   11.1    .83
Ethane     C2H6    3.58   10.5    .9
Kerosene   C12H26  3.52   10.3   1.03
Hydrazine  N2H4    3.46          1.07
Liquid hydrogen is usually not used for the ground stage of rockets because of its low density.
Oxidizer

We use kerosene as a standard fuel and show the rocket speed for various oxidizers. Some of the oxidizers can be used by themselves as monopropellants.

    Energy/Mass       Energy/Mass        Rocket           Rocket         Boil    Density
   with kerosene   as monopropellant  with kerosene  as monopropellant  Kelvin   g/cm3
       MJoule/kg         MJoule/kg          km/s             km/s

O3        12.9           2.97                                              161
O2        10.3           0                  3.52             0             110     1.14
H2O2       8.1           2.7                3.2              1.6           423     1.45
N2O4       8.00           .10               2.62                           294     1.44
N2O        6.18          1.86                                1.76          185
N2H4       -             1.58                                2.2           387     1.02

Solid rocket fuel
               MJoules  Rocket   Density
                 /kg     km/s    g/cm3

C6H6N12O12        9.1             1.96        China Lake compound
HMX (Octogen)     8.0   3.05      1.86
RDX (Hexagen)     7.5   2.5       1.78
Al + NH4ClO4            2.6
NH4ClO4                 2.5
NH3OHNO3                2.5       1.84        Hydrxyammonium nitrate
Al + NH4NO3       6.9
NH4NO3            1.4   2.0       1.12        Ammonium nitrate

History
~808  Qing Xuzi publishes a formula resembling gunpower, consisting of
      6 parts sulfur, 6 parts saltpeter, and 1 part birthwort herb (for carbon).
~850  Incendiary property of gunpower discovered
1132  "Fire lances" used in the siege of De'an, China
1220  al-Rammah of Syria publishes "Military Horsemanship and Ingenious War
        Devices", describes the purification of potassium nitrate by
        adding potassium carbonate with boiling water, to precipitate out
        magnesium carbonate and calcium carbonate.
1241  Mongols use firearms at the Battle of Mohi, Hungary
1338  Battle of Arnemuiden.  First naval battle involving cannons.
1346  Cannons used in the Siege of Calais and the Battle of Crecy
1540  Biringuccio publishes "De la pirotechnia", giving recipes for gunpowder
1610  First flintlock rifle
1661  Boyle publishes "The Sceptical Chymist", a treatise on the
      distinction between chemistry and alchemy.  It contains some of the
      earliest modern ideas of atoms, molecules, and chemical reaction,
      and marks the beginning of the history of modern chemistry.
1669  Phosphorus discovered
1774  Lavoisier appointed to develop the French gunpowder program.  By 1788
         French gunpowder was the best in the world.
1832  Braconnot synthesizes the first nitrocellulose (guncotton)
1846  Nitrocellulose published
1847  Sobrero discovers nitroglycerine
1862  LeConte publishes simple recipes for producing potassium nitrate.
1865  Abel develops a safe synthesis of nitrocellulose
1867  Nobel develops dynamite, the first explosive more powerful than black powder
      It uses diatomaceous earth to stabilize nitroglycerine
1884  Vieille invents smokeless gunpowder (nitrocellulose), which is 3 times
         more powerful than black powder and less of a nuisance on the battlefield.
1902  TNT first used in the military.  TNT is much safer than dynamite
1930  RDX appears in military applications
1942  Napalm developed
1949  Discovery that HMX can be synthesized from RDX
1956  C-4 explosive developed (based on RDX)
1999  Eaton and Zhang synthesize octanitrocubane and heptanitrocubane

Black powder           =  .75 KNO3  +  .19 Carbon  +  .06 Sulfur

Above 550 Celsius, potassium nitrate decomposes. 2 KNO3 ↔ 2 KNO2 + O2.


Black powder

Sulfur
Sulfur
Saltpeter
Saltpeter

Charcoal
Icing sugar and KNO3
Mortar and pestle
Mortar and pestle

Potassium nitrate  KNO3     75%       (Saltpeter)
Charcoal           C7H4O    15%
Sulfur             S        10%

Oversimplified equation:  2 KNO3 + 3 C + S  →  K2S + N2 + 3 CO2

Realistic equation:       6 KNO3 + C7H4O + 2 S  →  KCO3 + K2SO4 + K2S + 4 CO2 + 2 CO + 2 H2O + 3 N2
Nitrite (NO3) is the oxidizer and sulfur lowers the ignition temperature.
Fuel air explosives
                   MJoules
                     /kg

Hydrogen + Oxygen     13.16
Gasoline + Oxygen     10.4


        Mass   Energy    Energy/Mass
         kg      MJ         MJ/kg

MOAB    9800   46000        4.7               8500 kg of fuel

Phosphorus
White phosphorus
White, red, violet, and black phosphorus
Red phosphorus

Violet phosphorus
Black phosphorus
Black phosphorus

Form      Ignition    Density
          (Celsius)

White        30        1.83
Red         240        1.88
Violet      300        2.36
Black                  2.69
Red phosphorus is formed by heating white phosphorus to 250 Celsius or by exposing it to sunlight. Violet phosphorus is formed by heating red phosphorus to 550 Celsius. Black phosphorus is formed by heating white phosphorus at a pressure of 12000 atmospheres. Black phosphorus is least reactive form and it is stable below 550 Celsius.
Matches

Striking surface
P4S3

The safety match was invented in 1844 by Pasch. The match head cannot ignite by itself. Ignitition is achieved by striking it on a rough surface that contains red phosphorus. When the match is struck, potassium chlorate in the match head mixes with red phosphorus in the abrasive to produce a mixture that is easily ignited by friction. Antimony trisulfide is added to increase the burn rate.

Match head                 Fraction             Striking surface   Fraction

Potassium chlorate    KClO3  .50                Red phosphorus      .5
Silicon filler        Si     .4                 Abrasive            .25
Sulfur                S      small              Binder              .16
Antimony3 trisulfide  Sb2S3  small              Neutralizer         .05
Neutralizer                  small              Carbon              .04
Glue                         small
A "strike anywhere" match has phosphorus in the match head in the form of phosphorus sesquisulfide (P4S3) and doesn't need red phosphorus in the striking surface. P4S3 has an ignition temperature of 100 Celsius.
Flint

Before the invention of iron, fires were started by striking flint (quartz) with pyrite to generate sparks. Flintlock rifles work by striking flint with iron. With the discovery of cerium, ferrocerium replaced iron and modern butane lighters use ferrocerium, which is still referred to as "flint".

Cerium        .38      Ignition temperature of 165 Celsius
Lanthanum     .22
Iron          .19
Neodymium2    .04
Praseodymium  .04
Magnesium     .04

Nitrous oxide engine

Nitrous oxide is stored as a cryogenic liquid and injected along with gaoline into the combustion chamber. Upon heating to 300 Celsius the nitrous oxide decomposes into nitrogen and oxygen gas and releases energy. The oxygen fraction in this gas is higher than that in air (1/3 vs. .21) and the higher faction allows for more fuel to be consumed per cylinder firing.

Air density                  =  .00122 g/cm3
Nitrous oxide gas density    =  .00198 g/cm3
Diesel density               =  .832   g/cm3
Gasoline density             =  .745   g/cm3
Diesel energy/mass           =  43.1   MJoules/kg
Gasoline energy/mass         =  43.2   MJoules/kg
Nitrous oxide boiling point  = -88.5   Celsius
Air oxygen fraction          =  .21
Nitrous oxide oxygen fraction=  .33
Nitrous oxide decompose temp =  300    Celsius
Nitrous oxide liquid pressure=   52.4  Bars     Pressure required to liquefy N2O at room temperature

Bombardier beetle

Hydroquinone
P-quinone

Hydroquinone and peroxide are stored in 2 separate compartments are pumped into the reaction chamber where they explode with the help of protein catalysts. The explosion vaporizes 1/5 of the liquid and expels the rest as a boiling drop of water, and the p-quinone in the liquid damages the foe's eyes. The energy of expulsion pumps new material into the reaction chamber and the process repeats at a rate of 500 pulses per second and a total of 70 pulses. The beetle has enough ammunition for 20 barrages.

2 H2O2  →  2 H2O +  O2           (with protein catalyst)
C6H4(OH)2  →  C6H4O2 + H2        (with protein catalyst)
O2 + 2 H2  →  2 H2O

Firing rate                     = 500 pulses/second
Number of pulses in one barrage =  70
Firing time                     = .14 seconds
Number of barrages              =  20

Flame speed

A turbojet engine compresses air before burning it to increase the flame speed and make it burn explosively. A ramjet engine moving supersonically doesn't need a turbine to achieve compression.

Turbojet
Ramjet

Airbus A350 compression ratio  =  52
Air density at sea level       = 1    bar
Air density at 15 km altitude  =  .25 bar
Air density in A350 engine     =  13  bar
From the thermal flame theory of Mallard and Le Chatelier,
Temperature of burnt material    =  Tb
Temperature of unburnt material  =  Tu
Temperature of ignition          =  Ti
Fuel density                     =  Dfuel
Oxygen density                   =  Doxygen
Reaction coefficient             =  C
Reaction rate                    =  R  =  C Dfuel Doxygen
Thermal diffusivity              =  Q  = 1.9⋅10-5 m2/s
Flame speed                      =  V

V2  =  Q C Dfuel Doxygen (Tb - Ti) / (Ti - Tu)

Shocks

Spherical implosion
Mach < 1,    Mach = 1,     Mach > 1

If the pressure front moves supersonically then the front forms a discontinuous shock, where the pressure makes a sudden jump as the shock passes.


Energy boost

Metal powder is often included with explosives.

        Energy/mass    Energy/mass
        not including  including
        oxygen         oxygen
        (MJoule/kg)    (MJoule/kg)

Hydrogen    113.4      12.7
Gasoline     46.0      10.2
Beryllium    64.3      23.2
Aluminum     29.3      15.5                                      
Magnesium    24.5      14.8                                      
Carbon       12.0       3.3
Lithium       6.9       3.2
Iron          6.6       4.6                                      
Copper        2.0       1.6

Fireworks

Li
B
Na
Mg
K
Ca
Fe

Cu
Zn
As
Sr
Sb
Rb
Pb

BaCl (green), CuCl (blue), SrCl (red)
Zero gravity
Bunsen burner, O2 increases rightward
Methane


Oxygen candle

Sodium chlorate

An oxygen candle is a mixture of sodium chlorate and iron powder, which when ignited smolders at 600 Celsius and produces oxygen at a rate of 6.5 man-hours of oxygen per kilogram of mixture. Thermal decomposition releases the oxygen and the burning iron provides the heat. The products of the reaction are NaCl and iron oxide.


Firearms

Walther PPK/E 9 mm
FN SCAR-H 7.6 mm

Barrett M82 13 mm
M2 Bradley, M242 Bushmaster 25 mm
GAU-8 Avenger 30 mm

A-10 Warthog, GAU-8 Avenger
M1 Abrams 120 mm
M777 howitzer 155 mm

M777 Howitzer
U.S.S. Iowa 406 mm

                Bullet  Bullet   Speed   Energy   Barrel    Gun     Fire   Vehicle   Cartridge
                 diam    mass                                       rate    mass
                  mm      kg      m/s    kJoule   meters     kg     Hertz   tons

Swiss Mini Gun      2.3    .00013  122       .00097 .0018      .020
Chiappa 17          4.4    .0010   560       .16    .121                            .17 PMC/Aguila
Chiappa 17          4.4    .0010   640       .20    .121                            .17 HM2
SPP-1               4.5    .0128   245       .38               .95                  4.5x40mmR
Heckler Koch MP7    4.6    .0020   735       .54    .180      1.9                   HK 4.6x30mm
Walther PPK         5.6    .0020   530       .281   .083       .560
Walther PPK         5.6    .0030   370       .141   .083       .560
Walther PPK/S       7.65   .0050   318       .240   .083       .630
Walther PPK/E       9.0    .0065   323       .338   .083       .665
Luger 9mm           9.0    .0081   354              .102
Winchester 9x23     9.0    .0081   442
Colt 45            11.4    .0100   262              .127
Magnum 44          11.2    .0156   448              .165
Smith Wesson 460   11.5    .019    630      3.77    .213                            .460 SW Magnum
Magnum DesertEagle 12.7    .019    470              .254      1.996                 .50 Action Express
Smith Wesson 50mag 12.7    .026    550              .267      2.26
Smith Wesson 50mag 12.7    .029    520      3.92    .267      2.26
Smith Wesson 50mag 12.7    .032    434      3.01    .267      2.26                  .500 SW Magnum
MagnumResearch BFR 12.7    .026    550      3.93    .254      2.40                  .50 Beowulf

Ruger 96            4.4    .0013   720       .34    .47       2.38                  .17 HMR
Ruger M77           5.2    .0026  1200      1.83    .61       3.74                  .204 Ruger
CMMG MK47 Mutant    5.6    .0036   975                                              Remmington 22
Remmington 9mm      9.0    .0091   975
M4 Carbine          5.56   .0041   936      1.80    .370      2.88    15.8
FN SCAR-H Rifle     7.62   .011    790      3.51    .400      3.58    10.4          20 round magazine
Barrett M82        13.0    .045    908     18.9     .74      14.0                   10 round magazine
Hannibal           14.9    .049    750     13.8
CZ-550             15.2    .065    914     27.2                                     .600 Overkill
Vidhwansak         20      .13     720     33.7    1.0       26                     20x81 mm. 3 round magazine
RT-20              20      .13     850     47       .92      19.2                   1 round magazine
M621 cannon        20      .102   1005     51.5              45.5     13.3          20x102 mm
M61 Vulcan         20      .102   1050     56.2              92      110            20x102. 6 barrels
Oerlikon KBA       25      .184   1335    164      2.888    112       10
M242 Bushmaster    25      .184   1100    111      2.175    119        8.3    27.6  M2 Bradley
GAU-12 Equalizer   25      .184   1040     99.5             122       70       6.3  Harrier 2. 5 barrels
M230 chain gun     30      .395    805    128                55.9     10.4     5.2  Apache. 30x113 mm
Mk44 Bushmaster 2  30      .395   1080    230      2.41     160        3.3    27.6  M2 Bradley. 30x173 mm
GAU-8 Avenger      30      .395   1070    226      2.30     281       70      11.3  A-10 Warthog. 30x173 mm. 7 barrels
Bushmaster III     35             1180                      218        3.3          35x228 mm
Bushmaster IV      40     1.08                              198        3.3          40x365 mm
Rheinmetall 120   120     8.350   1750  12800      6.6     4500         .1    62    M1 Abrams tank
M777 Howitzer     155    48        827  16400      5.08    4200         .083
Iowa Battleship   406   862        820 290000     20.3   121500         .033  45000

2 bore rifle       33.7    .225    460     23.7     .711      4.5                   Historical big-game rifle
Cannonball 6 lb    87     2.72     438    261      2.4
Cannonball 9 lb    96     4.08     440    395      2.7
Cannonball 12 lb  110     5.44     453    558      2.4
Cannonball 18 lb  125     8.16     524   1120      2.6     2060
Cannonball 24 lb  138    10.89     524   1495      3.0     2500
Cannonball 32 lb  152    14.5      518   1945      3.4     2540
Cannonball 36 lb  158    16.33     450   1653      2.9     3250
Cannonball diameters are calculated from the mass assuming a density of 7.9 g/cm3.
For a pistol or rifle, the "vehicle mass" is the mass of the person wielding it. We use the mass of a typical person.
The "Metal Storm" gun has 36 barrels, 5 bullets per barrel, and fires all bullets in .01 seconds. The bullets are stacked in the barrel end-to-end and fired sequentially.

12 pound cannonballs
24 pound cannonballs


Bullet speed

25 mm
25 mm rocket propelled gernade
Excalibur 155 mm

The energy distribution for a 7.62 mm Hawk bullet is

Bullet energy    .32
Hot gas          .34
Barrel heat      .30
Barrel friction  .02
Unburnt powder   .01
To estimate the velocity of a bullet,
Energy efficiency  =  e  =  .32    (Efficiency for converting powder energy to bullet enery)
Bullet mass        =  M
Powder mass        =  m
Powder energy/mass =  Q  =  5.2 MJoules/kg
Bullet velocity    =  V
Bullet energy      =  E  =  ½ M V2  =  e Q m    (Kinetic energy = Efficiency * Powder energy)

V  =  (2 e Q m / M)2  =  1820 (m/M)½  meters/second

Muzzle break

M777 Howitzer
XD-40 V-10

The muzzle break at the end of the barrel deflects gas sideways to reduce recoil.


Gems

Ruby
Diamond
Topaz
Zircon: ZrSiO4
Spinel: MgAl2O4

Sapphire
Sapphire
Sapphire

Emerald
Beryl: Be3Al2(SiO3)6
Morganite

Quartz
Amethyst: SiO2
Amethyst: SiO2
Citrine: SiO2

Garnet: [Mg,Fe,Mn]3Al2(SiO4)3 & Ca3[Cr,Al,Fe]2(SiO4)3
Peridot: (Mg,Fe)2SiO4
Opal: SiO2·nH2O
Jadeite: NaAlSi2O6
Pearl: CaCO3
Amber: Resin

Corundum is a crystalline form of aluminium oxide (Al2O3). It is transparent in its pure form and can have different colors when metal impurities are present.

             Color    Colorant  carat ($)

Painite                          55000  CaZrAl9O15(BO3)
Diamond      Clear                1400  C
Ruby         Red      Chromium   15000  Al2O3
Sapphire     Blue     Iron         650  Al2O3
Sapphire     yellow   Titanium          Al2O3
Sapphire     Orange   Copper            Al2O3
Sapphire     Green    Magnesium         Al2O3
Emerald      Green    Chromium          Be3Al2(SiO3)6
Beryl        Aqua     Iron              Be3Al2(SiO3)6   AKA "aquamarine"
Morganite    Orange   Manganese    300  Be3Al2(SiO3)6
Topaz        Topaz                      Al2SiO4(F,OH)2
Spinel       Red      Red               MgAl2O4
Quartz       Clear                      SiO2
Amethyst     Purple   Iron              SiO2
Citrine      Yellow                     SiO2
Zircon       Red                        ZrSiO4
Garnet       Orange                     [Mg,Fe,Mn]3Al2(SiO4)3 & Ca3[Cr,Al,Fe]2(SiO4)3
Garnet       Blue                 1500  [Mg,Fe,Mn]3Al2(SiO4)3 & Ca3[Cr,Al,Fe]2(SiO4)3
Opal                                    SiO2·nH2O
Opal         Black               11000  SiO2·nH2O
Jet          Black                      Lignite
Peridot      Green                      (Mg,Fe)2SiO4
Pearl        White                      CaCO3
Jade         Green                      NaAlSi2O6
Amber        Orange                     Resin

Crystals
Crystal, polycrystal, and amorphous

Diamond
Carbon phase diagram

Corundum (Al2O3)
Corundum unit cell
Corundum

Metal lattice
Salt (NaCl)
Tungsten Carbide

Alpha quartz (SiO2)
Beta quartz
Glass (SiO2)
Ice


Fullerines

Buckyball with 540 atoms
Buckyball with 60 atoms
Buckyballs in the liquid phase

Nanotube

Buckyballs in a nanotube
Graphene


Polymers

Zylon
Vectran
Aramid (Kevlar)
Polyethylene

Aramid
Nylon
Hydrogen bonds in Nylon

Spider silk
Lignin

Lignin comprises 30 percent of wood and it is the principal structural element.


Rope

               Year   Young  Tensile  Strain  Density   Common
                      (GPa)  strength         (g/cm3)   name
                              (GPa)
Gut           Ancient           .2
Cotton        Ancient                   .1       1.5
Hemp          Ancient   10      .3      .023
Duct tape                       .015
Gorilla tape                    .030
Polyamide      1939      5     1.0      .2       1.14    Nylon, Perlon
Polyethylene   1939    117                       1.4     Dacron
Polyester      1941     15     1.0      .067     1.38
Polypropylene  1957                               .91
Carbon fiber   1968            3.0               1.75
Aramid         1973    135     3.0      .022     1.43    Kevlar
HMPE           1975    100     2.4      .024      .97    Dyneema, Spectra
PBO            1985    280     5.8      .021     1.52    Zylon
LCAP           1990     65     3.8      .058     1.4     Vectran
Vectran HT              75     3.2      .043     1.41    Vectran
Vectran NT              52     1.1      .021     1.41    Vectran
Vectran UM             103     3.0      .029     1.41    Vectran
Nanorope             ~1000     3.6      .0036    1.3
Nanotube              1000    63        .063     1.34
Graphene              1050   160        .152     1.0


Strain  =  Strength / Young
Carbon fiber is not useful as a rope.

A string ideally has both large strength and large strain, which favors Vectran.

Suppose Batman has a rope made out of Zylon, the strongest known polymer.

Batman mass            =  M         =    100 kg               (includes suit and gear)
Gravity constant       =  g         =     10 meters/second2
Batman weight          =  F         =   1000 Newtons
Zylon density          =  D         =   1520 kg/meter3
Zylon tensile strength =  Pz        = 5.8⋅109 Newtons/meter2
Rope load              =  P         = 1.0⋅109 Newtons/meter2   (safety margin)
Rope length            =  L              100 meters
Rope cross section     =  A  = F/P  =1.0⋅10-6 meters2
Rope radius            =  R  =(A/π)½=     .56 mm
Rope mass              =  Mr = DAL  =     .15 kg

Wood

         Density   Tensile   Young
                   strength
         (g/cm^3)  (Gpa)     (Gpa)

Balsa         .12    .020      3.7
Corkwood      .21
Cedar         .32    .046      5.7     Northern white
Poplar        .33    .048      7.2     Balsam
Cedar         .34    .054      8.2     Western red
Pine          .37    .063      9.0     Eastern white
Buckeye       .38    .054      8.3     Yellow
Butternut     .40    .057      8.3
Basswood      .40    .061     10.3
Spruce, red   .41    .072     10.7
Aspen         .41    .064     10.0
Fir, silver   .42    .067     10.8
Hemlock       .43    .061      8.5     Eastern
Redwood       .44    .076      9.6
Ash, black    .53    .090     11.3
Birch, gray   .55    .069      8.0
Walnut, black .56    .104     11.8
Ash, green    .61    .100     11.7
Ash, white    .64    .110     12.5
Oak, red      .66    .100     12.7
Elm, rock     .66    .106     10.9
Beech         .66    .102     11.8
Birch, yellow .67    .119
Mahogany      .67    .124     10.8     West Africa
Locust        .71    .136     14.5     Black or Yellow
Persimmon     .78    .127     14.4
Oak, swamp    .79    .124     14.5     Swamp white
Gum, blue     .80    .118     16.8
Hickory       .81    .144     15.2     Shagbark
Eucalyptus    .83    .122     18.8
Bamboo        .85    .169     20.0
Oak, live     .98    .130     13.8
Ironwood     1.1     .181     21.0
Lignum Vitae 1.26    .127     14.1
Data #1     Data #2
Plastic

           Density   Tensile   Young
                     strength
           (g/cm^3)  (Gpa)     (Gpa)


Polyamide            .11       4.5
Polyimide            .085      2.5
Acrylic              .07       3.2
Polycarbonate        .07       2.6
Acetyl copoly        .06       2.7
ABS                  .04       2.3
Polypropylene  .91   .04       1.9
Polystyrene          .04       3.0
Polyethylene   .95   .015       .8

Valyrian steel

"Ice" is the sword with the red handle

Valyrian steel is a fictional substance from "Game of Thrones" that is stronger, lighter, and harder than steel. The only elements that qualify are beryllium, titanium, and vanadium, none of which were known in Earth history until the 18th century. Valyrian steel could be of these elements, an alloy, or a magical substance. According to George Martin, magic is involved.

The fact that it is less dense than steel means that it can't be a fancy form of steel such as Damascus steel or Wootz steel. Also, fancy steel loses its special properties if melted and hence cannot be reforged, whereas Valyrian steel swords can be reforged.

In Earth history, the first metal discovered since iron was cobalt in 1735. This launched a frenzy to smelt all known minerals and most of the smeltable metals were discovered by 1800. Then the battery and electrochemstry were discovered in 1800 and these were used to obtain the unsmeltable metals, which are lithium, beryllium, magnesium, aluminum, titanium, vanadium, niobium, and Uranium. Almost all of the strong alloys use these metals, and so the Valyrians must have used either electrochemistry or magic to make Valyrian steel.


Candidates for Valyrian steel

The following metals and alloys are both stronger and lighter than steel and could hypothetically be Valyrian steel.

                Yield     Density  Strength/Density
                strength  (g/cm3)   (GJoule/kg)
                (GPascal)
Beryllium            .34     1.85     .186
Aluminum + Be        .41     2.27     .181
LiMgAlScTi          1.97     2.67     .738
Titanium             .22     4.51     .050
Titanium + AlVCrMo  1.20     4.6      .261
Vanadium             .53     6.0      .076
AlCrFeCoNiTi        2.26     6.5      .377
AlCrFeCoNiMo        2.76     7.1      .394
Steel                .25     7.9      .032     Iron plus carbon
Copper               .12     9.0      .013
"Yield strength" is the maximum pressure a material can sustain before deforming. "Strength/Density" is the strength-to-weight ratio. Steel is stronger and lighter than copper.
Lore

Petyr Baelish: Nothing holds an edge like Valyrian steel.

Tyrion Lannister: Valyrian steel blades were scarce and costly, yet thousands remained in the world, perhaps two hundred in the Seven Kingdoms alone.

George Martin: Valyrian steel is a fantasy metal. Which means it has magical characteristics, and magic plays a role in its forging.

George Martin: Valyrian steel was always costly, but it became considerably more so when there was no more Valyria, and the secret of its making were lost.

Ned Stark's stord "Ice" is melted down and reforged into two smaller swords, "Oathkeeper" and "Widow's Wail". This rules out Valyrian steel being Wootz steel because Wootz steel loses its special properties when reforged.

Appearances of Valyrian steel in Game of Thrones:

        Name          Owner

Sword   Longclaw      Jon Snow
Sword   Heartsbane    Samwell Tarly
Dagger                Arya
Sword   Ice           Eddard Stark         Reforged into Oathkeeper and Widow's Wail
Sword   Oathkeeper    Brienne of Tarth
Sword   Widow's Wail  The Crown
Sword   Lady Forlorn  Ser Lyn Corbray
Sword   Nightfall     Ser Harras Harlow
Sword   Red Rain      Lord Dunstan Drumm
Arakh                 Caggo
Armor                 Euron Greyjoy
Horn    Dragonbinder  The Citadel of The Maesters
Some Maesters carry links of Valyrian steel, a symbol of mastery of the highest arts.
Wildire

Copper

The burn rate of gasoline is limited by the supply of oxygen.

C8H18 + 12.5 O2  →  8 CO2 + 9 H2O
Gunpowder has oxygen in the mixture in the form of KNO3 which makes it burn faster.
3 C + S + 2 KNO3  →  K2S + N2 + 3 CO2
We know that wildfire contains an oxidizer otherwise it wouldn't be able to explode as it did on the show. Wildfire is made from manure, which contains KNO3.

Copper burns with a green flame. Adding copper powder to the explosive adds energy to the blast.

Three types of incendiaries are:

Gasoline:          Flame spreads slowly. Needs oxygen from the air.
Gunpowder:         Contains oxygen. Buns faster than gasoline. Subsonic pressure wave.
Plastic explosive: Pressure wave spreads supersonically as a shock.

Chemistry
~808    Qing Xuzi publishes a formula resembling gunpower, consisting of
        6 parts sulfur, 6 parts saltpeter, and 1 part birthwort herb (for carbon).
~850    Incendiary property of gunpower discovered
1540    Biringuccio publishes "De la pirotechnia", giving recipes for gunpowder
1661    Boyle publishes "The Sceptical Chymist", a treatise on the
        distinction between chemistry and alchemy.  It contains some of the
        earliest modern ideas of atoms, molecules, and chemical reaction,
        and marks the beginning of the history of modern chemistry.
1662    Boyle discovers that for air at fixed temperature,
        Pressure * Volume = Constant
1663    Guericke invents the first electrostatic generator, which uses
        mechanical work to separate charge.  Generators were refined until
        they were superceded by the battery.
1671    Boyle discovers that combining iron filings and acid produces hydrogen gas.
1754    Black isolates CO2
1758    Black formulates the concept of latent heat to explain phase transitions
1766    Cavendish identifies hydrogen as a colorless, odourless gas that burns
        in air.
1772    Scheele produces pure oxygen gas by heating HgO.
1774    Priestly produces pure oxygen gas by focusing sunlight on HgO.
        He noted that it is combustible and that it gives energy when breathed.
1745    von Kleist invents the capacitor, a device for storing charge generated
        by an electrostatic generator.
1746    van Musschenbroek refines the capacitor, which comes to be known as a
        "Leyden jar".
1777    Lavoisier finds that in the reaction tin+oxygen, mass is conserved.
        He also finds that oxygen is not the only component of air, that air also
        consists of something else.
1780    Galvani observes that when a frog leg is touched by an iron scalpel,
        it twitches.  This was the inspiration for Volta to invent the battery.
1781    Cavendish finds that buring hydrogen + oxygen produces water.
1787    Charles finds that for air at constant pressure,
        Volume = Constant * Temperature
        He also finds that this applies for O2, N2, H2, and CO2.
1789    Lavoisier publishes "Traite Elementaire de Chimie", the first modern
        chemistry textbook.  It is a complete survey of (at that time) modern
        chemistry, the law of conservation of mass.
1791    Volta develops the first electrochemical cell, consisting of two different
        metals separated by a moist intermediary.
1797    Proust proposes the law of definite proportions, that elements
        combine in small whole number ratios to form compounds.
1800    Volta constructs the first "battery" by connecting multiple electrochemical
        cells in parallel, increasing the output power and voltage.
1801    Dalton publishes the law of partial pressures.
        The pressure of a mix of gases is equal to the sum of the pressures
        of the components.  He also finds that when a light and heavy gas are mixed,
        the heavy gas does not drift to the bottom but rather fills the space
        uniformly.
1805    Gay-Lussac and Humboldt find that water is formed of two volumes of
        hydrogen gas and one volume of oxygen gas.
1809    Gay-Lussac finds that for an ideal gas at constant volume,
        Pressure = Constant * Temperature
1811    Avogadro finds that equal volumes of different gases have the same number
        of particles.  At constant temperature and pressure,
        Volume = Constant * NumberOfParticles
1811    Avogadro arrives at the correct interpretation of water's composition,
        based on what is now called Avogadro's law and the assumption of diatomic
        elemental molecules
1840    Hess finds that energy is conserved in chemical reactions
1848    Lord Kelvin establishes concept of absolute zero, the temperature at
        which all molecular motion ceases.
1860    Cannizzaro publishes a table of atomic weights of the known elements
1864    Gulberg and Waage propose the law of mass action
1869    Mendeleev publishes a periodic table containing the 66 known elements
1876    Gibbs publishes the concept of "Gibbs free energy"
1877    Boltzmann defines entropy and develops thermodynamics
1877    Pictet freezes CO2 and liquefies oxygen.
        Liquification enables the purification of gases.
1894    Ramsay discovers the noble gases, filling a large and unexpected gap in
        the periodic table

Atoms
1635   Gassendi measures the speed of sound to be 478 m/s with 25% error.
1660   Viviani and Borelli produce the first accurate measurement of the speed of
       sound, giving a value of 350 m/s.
1660   Hooke's law published.  The force on a spring is proportional to the change
       in length.
1662   Boyle discovers that for air at fixed temperature,
       Pressure * Volume = Constant
       Hence, air obey's Hooke's law
1687   Newton publishes the Principia Mathematica, which contains the first analytic
       calculation of the speed of sound.  The calculated value was 290 m/s
       and the true value is 342 m/s (at 20 Celsius).
Newton's result was the first solid evidence for the existence of atoms. His result differed from the correct value because it had not yet been discovered that air heats when compressed. If you add this effect you get the right value.

The reason air heats when compressed is because it is composed of atoms. You can see this in action with the "Gas" simulation at phet.colorado.edu. You can also see how atoms in a gas can carry a sound wave, and why the sound speed has the same order-of-magnitude as the thermal velocity of the atoms.

1789  Lavoisier publishes "Traite Elementaire de Chimie", the first modern
      chemistry textbook.  It is a complete survey of (at that time) modern
      chemistry, the law of conservation of mass.
1797  Proust proposes the law of definite proportions, that elements
      combine in small whole number ratios to form compounds.
1801  Dalton publishes the law of partial pressures.
      The pressure of a mix of gases is equal to the sum of the pressures
      of the components.  He also finds that when a light and heavy gas are mixed,
      the heavy gas does not drift to the bottom but rather fills the space
      uniformly.
1805  Gay-Lussac and Humboldt find that water is formed of two volumes of
      hydrogen gas and one volume of oxygen gas.
1809  Gay-Lussac finds that for an ideal gas at constant volume,
      Pressure = Constant * Temperature
1811  Avogadro finds that equal volumes of different gases have the same number
      of particles.  At constant temperature and pressure,
      Volume = Constant * NumberOfParticles
1811  Avogadro arrives at the correct interpretation of water's composition,
      based on what is now called Avogadro's law and the assumption of diatomic
      elemental molecules
1860  Cannizzaro publishes a table of atomic weights of the known elements
1869  Mendeleev publishes a periodic table containing the 66 known elements
1877  Boltzmann defines entropy and develops thermodynamics
All of these results support the hypothesis that matter is composed of atoms, but there was no known experiment sensitive enough to measure the size and mass of an individual atom.
Wavelength of violet light = 4e-7 meters
Diameter of an iron atom   = 2e-10 meters
Violet photons are much larger than atoms and so you can't see atoms in an optical microscope.
1905  Einstein publishes a method for measuring the mass of an atom using
      Brownian motion
1908  Perrin uses Einstein's method to produce the first measurement of the mass of
      an atom.  This is equivalent to measuring the value of Avogadro's number.
Minutephysics atoms
Periodic table of cupcakes


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Astrobiology
Dr. Jay Maron


Timeline of the universe


                Millions of years ago

Big bang             13700
First planets formed 13000
Earth formed          4500
Photosynthesis        3000
Oxygen atmosphere      600
Multicellular life     600
Vertebrates            480
Tetrapod vertebrates   400
Mammals                170
Dinosaur extinction     66
Cats                    25
Cheetahs                 6
Tigers                   1.8
Humans                   1
Lions                     .9
Agriculture               .01
Civilization              .005
Calculus                  .0004
An alien planet could conceivably have formed as early as 1 billion years after the big bang, meaning that there are likely aliens with a head start on us by billions of years.

An alien civilization could easily build a rocket that travels at 1/10 the speed of light, which would take 1 million years to cross the galaxy. The aliens have plenty of time to get here.

Dinosaurs and birds


Tetrapods

                                            ->  Reptiles  ->  Dinosaurs  ->  Birds
                                           /
Vertebrates   ->   Tetrapod vertebrates  --
                                           \
                                            ->  Mammals
A tetrapod is a vertebrate with four limbs. Reptiles, dinosaurs, birds and mammals all evolved from tetrapods, and the essential elements of the tetrapod design haven't changed since its emergence. Elements of the tetrapod design include:

A spine
A skull
A ribcage
Four limbs
One bone in the upper limb and two bones in the lower limb.

Humans have the most complex wrists and hands in the animal kingdom.

Bruce Lee: There is only one type of body, 2 arms, 2 legs, etc that make up the human body. Therefore, there can only be one style of fighting. If the other guy had 4 arms and 2 legs, there might have to be a different one. Forget the belief that one style is better than the other, the point of someone that does not just believe in tradition, but actually wants to know how to fight is to take what you need from every martial art and incorporate it into your own. Make it effective and very powerful, but don't worry if you are taking moves from many different arts, that is a good thing.

Not a tetrapod
Not a tetrapod


Oxygen cycle

Earth photosynthesis
Banded iron formation

Define one "Earth Atmosphere Oxygen Mass" (EAOM) as the mass of the oxygen in the Earth's atmosphere, equal to 1.4*10^18 kg.


Oxygen          Mass        Flux        Half life
Reservoir      (EAOM)    (EAOM/year)

Atmosphere        1        .000214      4500 years
Biosphere          .0114   .000214        50 years
Lithosphere     207        4.3*10^-7     400 million years

Land photosynthesis   = .000118 EAOM/year = 165*10^12 kg Oxygen / year
Ocean photosynthesis  = .000096 EAOM/year = 135*10^12 kg Oxygen / year
The time required by photosynthesis to generate one EAOM is 4700 years.

Early in the Earth's history, oxygen produced by photosynthesis was absorbed by iron dissolved in the oceans, creating "banded iron formations". Once photosynthesis overwhelmed the ocean's iron, an oxygen atmosphere became possible.

California
Tatooine

A desert planet like Tatooine would have a hard time generating an oxygen atmosphere.


Carbon cycle

This diagram of the fast carbon cycle shows the motion of carbon between land, atmosphere, and oceans, in billions of tons of carbon per year. Yellow numbers are natural fluxes, red are human contributions in billions of tons of carbon per year. White numbers indicate stored carbon.

Carbon content of the Earth, with the atmosphere normalized to 1

Atmosphere      1.00
Biomass          .62
Surface ocean   1.25
Deep ocean     46.2
Ocean sediment  7.5
Soil            2.88
Fossil carbon  12.5
Given the global rate of fossil fuel burning, it would take ~ 89 years to double the atmosphere's carbon.

Photosynthesis moves carbon from the atmosphere to plants, and the carbon returns to the atmosphere through plant respiration and through microbial decomposition of dead plants. Given the global rate of photosynthesis, it takes photosynthesis ~ 7 years to cycle through the atmosphere's carbon.


Ozone cycle

Ozone cycle
Radiation as a function of altitude
Ozone distribution

Ozone production from solar radiation          =  400 million tons / day
Ozone loss from combining with oxygen radicals =  400 million tons / day
Total atmospheric ozone                        = 3000 million tons
The Sun produces 12% of the ozone layer each day.

Water absorption spectrum

Before the Earth had oxygen and ozone, the continents were uninhabitable and the only place photosynthesis could take place was underwater. Water is more transparent to visible light than to ultraviolet light.


Nitrogen cycle

Cyanobacteria can fix 1.8 kg of nitrogen per hectare per day. Nitrogen can be fixed in the ocean at twice the rate than what is possible on land.


Global temperature


History of atmospheric carbon dioxide


Sea level


World totals
Atmosphere temperature rise=   .017 Kelvin/year      (.9 Kelvin since 1800)
Sea level rise             =  2.8   mm/year          (225 mm since 1800)
Atmosphere CO2 frac        =   .0035                 (.0027 in 1800)
Atmosphere carbon          =720     Gtons
Photosynthesis of carbon   =120     Gtons/year
Human carbon emissions     =  9     Gtons/year   = 1240   kg/person/year
Energy produced            =   .57  ZJoules/year =   78.6 GJoules/person/year
Electricity produced       =   .067 ZJoules/year =    9.2 GJoules/person/year
Food                       =   .027 ZJoules/year =    3.7 GJoules/person/year = 2500 Cal/person/day
Sunlight energy            =3850    ZJoules/year
Wind energy                =  2.25  ZJoules/year
Photosynthesis of biomass  =  3.00  ZJoules/year
Ocean heat gain            =  7.5   ZJoules/year
World power                = 18     TWatts       = 4500   Watts/person
Energy cost                = 16     T$/year      = 2210   $/person/year   (27.8 $/GJoule)
Population                 =  7.254 billion
Food                       =  1.58  Tkg/year     =  218   kg/person/year  (As carbs)
Earth land area            =148.9   Mkm2         =    2.0 Hectares/person
Rainfall over land         =107000  km3/year     =   14.8 tons/person/year
River flow                 = 37300  km3/year     = 5140   tons/person/year
Water total use            =  9700  km3/year     = 1390   tons/person/year
Water for agriculture      =  1526  km3/year     =  218   tons/person/year
Water for home use         =   776  km3/year     =  111   tons/person/year
Water desalinated          =    36  km3/year     =    5   tons/person/year

Greenhouse gases

       Contribution to    Half life in the atmosphere
     greenhouse warming
H2O    36-72%
CO2     9-26%             90 years
CH4     4-9%              12 years
Ozone   3-7%               1 week

The importance of oxygen

Oxygen clan
Sulfur clan

Oxygen clan vs. Sulfur clan
                       Chuck                    Sulfur-reducing bacteria
                       (Oxygen Clan)            (Sulfur Clan)

Mass                   100 kg                   single-cellular
Power source           Hydrocarbons + oxygen    Hydrocarbons + sulfur
ATP per glucose        30                       2
Resting power          100 Watts                tiny
Peak power             kilowatts                tiny
Peak power/weight      10 Watts/kg              tiny
Strength               Kilonewtons              tiny
Computation            10^14 synapses           -
Brain power            20 Watts                 -
Achilles heel          H2S                      Oxygen

Aerobic organisms have an energy advantage over anaerobic organisms.

Aerobic respiration:     Glucose  +  Oxygen   -->   H2O  + 30 ATP of energy
Anaerobic respiration:   Glucose  +  Sulfur   -->   H2S  +  2 ATP of energy
Aerobic organisms also have a weight advantage over anaerobic organisms. Aerobic organisms can get oxygen from the air whereas anaerobic organisms have to carry their oxidizer.
For the reaction
Hydrocarbons  +  Oxygen  -->  H2O  +  CO2  +  energy
Mass of oxygen / Mass of hydrocarbons ~ 8
These two factors give aerobic organisms an overwhelming energy advantage over anaerobic ones, and this is the reason why nearly all multi-cellular organisms are aerobic.

Oxygen is usually toxic to anaerobic organisms.

Anaerobic organisms produce H2S and CS2, which is toxic to most aerobic organisms.

Before the Earth had an oxygen atmosphere, sulfur-reducing bacteria ruled the Earth. When oxygen appeared, aerobic organisms took over because of the energy advantage. Sulfur-reducing bacteria retreated underground where there is no oxygen. On occasion the sulfur bacteria make a comeback, such as during the runaway global warming event 251 million years ago. During this episode, the atmosphere became flooded with H2S, causing a mass extinction of aerobic species.

Peter Ward's book "The Medea Hypothesis" has a nice discussion of the rivalry between aerobic and anaerobic organisms, and of the interaction between the Earth's geology and biology.

In the film "Avatar", the atmosphere of Pandora is toxic to humans because of H2S.


Electronegativity

Oxygen is more electronegative than sulfur, which is why reacting hydrocarbons with oxygen yields more energy than by reacting them with sulfur.

The only element that rivals oxygen's electronegativity is fluorine, but fluorine gas is highly reactive and HF is a strong acid.


Brain to body mass ratio

The human brain consumes 20 Watts.

Even though the brain is a power-hungry organ, organisms take the trouble to develop large brains.

                 Brain    Total    Brain/
                 mass     mass     body
                 (kg)     (kg)
Sperm whale         8
Orca whale          6
Elephant            5     2800      .0018
Blue whale          4
Bottlenose dolphin  1.7
Neanderthal         1.9
Human               1.6     64      .025
Gorilla              .6
Chimpanzee           .4
Orangutan            .4
Horse                .4    235     .0017
Pig                  .20
Dog                  .10    12     .0080
Cat                  .04     4     .0091
Squirrel             .009    1.4   .0067
Mouse                .001     .04  .025
Shrew                .0002    .002 .1
Bat                  .0001
Frog                               .0058
Small bird                         .071
Shark                              .0004
Ant                                .14
"The body cannot exist without the mind" - Morpheus
Fuel

                 MJoules/kg

Antimatter       90 billion
Hydrogen bomb      25000000    theoretical maximum yield
Hydrogen bomb      21700000    highest achieved yield
Uranium            20000000    as nuclear fuel
Hydrogen                143
Natural gas              53.6
Gasoline                 47
Jet fuel                 43
Fat                      37
Coal                     24
Carbohydrates & sugar    17
Protein                  16.8
Wood                     16
Lithium-air battery       9
TNT                       4.6
Gunpowder                 3
Lithium battery           1.3
Lithium-ion battery        .72
Alkaline battery           .59
Compressed air             .5        300 atmospheres
Supercapacitor             .1
Capacitor                  .00036
The chemical energy source with the highest energy/mass is hydrogen+oxygen, but molecular hydrogen is difficult to harness. Hydrocarbons + oxygen is the next best choice. Carbon offers a convenient and lightweight way to carry hydrogen around.

Reacting hydrocarbons in an oxygen atmosphere yields the optimal power-to-weight ratio.

Given the enormous power required by brains, if intelligent life exists in the universe, it likely gets its energy from reacting hydrocarbons in an oxygen atmosphere. Most likely we would be able to eat their food.


Food
        MJ/kg  Calories/gram
Sugar    16        5
Protein  17        5
Alcohol  25        7
Fat      38        9

Breathing

Bruce Lee: When the opponent expands I contract, when he contracts I expand, and when there is an opportunity, I do not hit, it hits all by itself.

The diaphragm creates pressure in the abdomen, which expands the ribcage and creates negative pressure for inhalation. Any air-breathing alien has to find a way to generate negative pressure. The ribcage expansion also puts tension energy into the rib muscles, which can be released in a sudden pulse to launch motion of the limbs.

Breathing is coordinated with skeletal motion to minimize energy expenditure. Motion cycles between the following two columns.

Breathe in                Breathe out
Diaphram contracts        Diaphram expands
Ribcage expands           Ribcage contracts
Spine muscles contract    Spine muscles release
Arms rotate out           Arms rotate in
Elbows rotate out         Elbows rotate in
Thumbs rotate out         Thumbs rotate in
Head rises                Head descends
Lower back arches         Lower back sags
Legs rotate out           Legs rotate in
Gut squashed by diaphram  Gut expands
Daydream                  Focus
Rebalance                 Exertion
Arms out                  Arms in
High moment of inertia    Low moment of inertia
Discard angular momentum  Discard pressure
When you are in action, your breathing adjusts to support the timing of your skeletal motion, and if it has any spare time, it sucks in as much air as possible.

When you are relaxing, your breathing adjusts to minimize energy, coordinate cycles, and smooth transitions.


Mechanics

Tetrapod limbs have 2 long bones. A limb with only one long bone is obviously insufficient and 2 long bones are sufficient to support 3D motion of the hand. 3 long bones is probably unnecessary.

There is 1 bone in the upper limb and 2 bones in the lower limb, with a universal joint at the shoulder/hip, a locking joint at the knee/elbow, and a universal joint at the wrist/ankle. The shoulder/hip universal joints can be realistically supported because the torso has abundant muscle mass and torque. The locking joint is harder to support because the upper limb has less muscles and torque than the torso. This is why the lower limb has 2 bones, to help with torque and to stabilize the hand.

The hand is small enough that it can be supported by a univeral joint (the wrist).

The length of limbs is limited by the ability of the torso to deliver force and torque to the hands and feet.

Humans have the most complex wrists in the animal kingdom. Only humans can fully exploit the universal joint of the wrist.

Humans are one of the only animals capable of good balance while on one foot.


Ulna and tibia

Ulna
Tibia
Tibia
Tibia

In your forearm, the ulna is the large bone and the radius is the small bone. The forearm should ideally rotate around the large bone.

The ulna connects to your hand on the pinky side and the radius connects to the thumb side. Your hand should rotate about the pivot point where your ulna connects to your wrist.

In your lower leg the tibia is the large bone and the fibula is the small bone.

The tibia connects to your foot at the big toe side and the fibula connects at the little toe site.


Shoulders and hips

The lower limbs are connected directly to the spine so that the can deliver force from the ground to the spine. The upper limbs are not directly connected to the spine so that they can absorb shock and move with precision. If an organism has no collarbone then there is no skeletal connection between the limbs and spine at all. If an organism has a colarbone then the connection sequences is:

Spine  -  Ribs  -  Breatbone  -  Collarbone  -  Shoulder blade  -  Humerus
The function of the spine is to smooth out angular momentum generated by the limbs.
Atmospheres

Earth
Titan
Veuns
Mars

      Density  Pressure Escape Gravity   N2     O2    N2    CO2     Ar    H2   H3   CH4  Temp
      kg/m^3    (Bar)    km/s   m/s^2  kg/m^3  frac  frac   frac   frac  frac frac  frac (K)
Venus    67     92.1     10.36   8.87  2.34           .035  .965                          735
Titan     5.3    1.46     2.64   1.35  5.22           .984                          .014   94
Earth     1.2    1       11.2    9.78   .94    .209   .781  .00039 .0093                  287
Mars       .020   .0063    .64   5.03   3.8    .00054 .0013  .027  .953   .016                   210


        Gravity    H2      He    CH4  Escape
        m/s^2     frac    frac  frac  speed (km/s)
Sun    279.4      .735     .248       617.7
Jupiter 24.79     .90      .10  .003   59.5
Saturn  10.44     .96      .03  .004   35.5
Uranus   8.69     .83      .15  .023   21.3
Neptune 11.15     .80      .19  .015   23.5
Titan is the smallest object with an atmosphere and Mercury is the largest object without an atmosphere.


Terraforming

      Atmos                                                                Atmos    Max     Min
      Density  Pressure  Gravity   N2      O2     N2    CO2   Temp  Lapse  Height  height  Height
      kg/m^3    (Bar)     m/s^2  kg/m^3   frac   frac   frac   (K)  (K/km)  (km)    (km)
Mars     .020    .0063   3.71     .00054  .0013  .027  .953    210   4.5    15      22     -7.15
Titan   5.3     1.46     1.35    5.22            .984           94   1.3    14        .5   -2
Venus  67      92.1      8.87    2.34            .035  .965    735  10.5     7      11
Earth   1.28    1.0      9.78     .94     .209   .781  .00039  287   9.8     9       8.8   -0.8
Moon    0       0        1.62                                  220                   8     -6
Ceres   0       0         .27                                  168
"Atmospheric height" is the height at which the atmosphere density is exp(-1) times the density at sea level.

"Lapse" is the adiabatic lapse rate.

"Max height" is the maximum elevation.

"Min height" is the minimum elevation.

The atmosphere of Titan is non-toxic and there is enough atmospheric pressure that you don't need a pressure suit. You can roam around Titan with a ski suit and scuba gear. Gravity is so low that human-powered flight is easy.


Radioactive heating of the Earth

Moon
Io

              Watts/kg     half life  mantle      Watts/kg
              of isotope   (years)    abundance   of mantle
uranium-238    9.46e-5       4.47e9    30.8 e-9   2.91 e-12
uranium-235   56.9 e-5        .70e9      .22e-9    .125e-12
thorium-232    2.64e-5      14.0 e9   124   e-9   3.27 e-12
potassium-40   2.92e-5       1.25e9    36.9 e-9   1.08 e-12
The Earth loses heat at a rate of .087 Watts/m^2, for a global heat los of 4.42e13 Watts.

80% of the Earth's heat is from radioactivity and 20% is from accretion.

The radioactive heating rate 3 billion years ago is twice that of today.

The Earth's core temperature is ~ 7000 K.

Io is heated by tidal forces from Jupiter.


Magnetic fields

Solar wind
Jupiter

          Dipole     Field at  Magnetopause  Axis     Rotation  Volcanic
          moment     equator   (planet       angle    (days)
         (Earth=1)   (Gauss)    radii)     (degrees)
Sun      5 million                                      25.0
Mercury       .0007   .003         1.5      14          58.6    No
Venus        <.0004  <.00003       -         -         243.0    Yes
Earth        1        .305        10        10.8         1.00   Yes
Mars         <.0002  <.0003        -         -           1.03   No
Jupiter  20000       4.28         80         9.6          .41
Saturn     600        .22         20        <1            .44
Uranus      50        .23         20        58.6          .72
Neptune     25        .14         25        47            .67
Io                                                              Yes
Europa        .0016   .0072        4.5

Habitable zone
Hoth
The "Goldilocks Zone"
Antarctica

Expanded discussion of the habitable zone

Stability of the solar system

Expanded discussion of orbital stability

Planet migration

Io, Europa, Ganymede, Callisto
Jupiter and its moons
Io, Europa, Ganymede

Goldreich & Tremaine (1980): "We present an illustrative application of our results to the interaction between Jupiter and the plantary disk. The angular momentum transfer is shown to be so rapid that substantial changes in both the structure of the disk and the orbit of Jupiter must have taken place on a time scale of a few thousand years."


Extrasolar planetary systems

This is a plot of all known planetary systems with at least 3 planets.

Each row corresponds to a planetary system and the solar system is 2/3 of the way down.

Dot size          =  (Planet Mass)^(1/3)
Dot X coordinate  =  Log(distance from star)
Yellow dot        =  Planets orbit a star with high metallicity
Red dot           =  Plaents orbit a star with low metallicity
The magenta dot indicates the location of the Goldilocks zone. For a given star, Radius of Goldilocks zone ~ (1 AU) * (Star luminosity / Sun luminosity)^(-1/2)

Horizontal cyan lines indicate the range between the planet's perigee and apogee.

Horizontal green lines correspond to 6 times the planet's Hill radius, a measure of the planet's zone of gravitational dominance.

Vertical blue lines indicate the planet's orbital inclination.

Same as above except for:

Horizontal yellow line  =  Range from perigee to apogee
Horizontal red line     =  6 times the planet's Hill radius
The planets of the solar system are smaller and more widely spaced than what is typical for exoplanetary systems. In the Galactic Museum of Natural History, the solar system might be classified as a "Dwarf planetary system".

What could go wrong?

Meteor Crater, Arizona


Planet property   If too little                           If too much


Mass              Cannot capture atmosphere               Becomes gas giant
                  No volcanism
                  Cannot generate a magnetic field

Distance from     Too hot                                 Too cold for surface water
star              Inside the snow line

Atmospheric       Cosmic rays reach the surface           Blocks too much sunlight
thickness         Atmosphere loses heat at night          for photosynthesis

Water content     If you don't have oceans then you       No dry land
                  don't have enough photosynthesis
                  to generate an oxygen atmosphere

Planet spin       Does not generate a large-scale
                  magnetic field

Planet spin tilt                                          Extreme seasons


Star temperature  Not enough blue light for               Too much UV light
                  photosynthesis

Star metallicity  Small planets                           Too many gas giants

Star mass         Planet is so close to the star that it
                  is tidally locked to the star

Moon mass         Planet tilt becomes unstable, causing
                  extreme seasons

A moon of a gas giant can potentially be protected from the solar wind by the gas giant's magnetic field. It can also potentially have volcanism from tidal heating by the gas giant.
Mass extinctions

The Earth has been beset by asteroids, supervolcanoes, global ice ages, runaway global warming, supernovae, gamma ray bursts, and the industrial age.

Millions of
years ago

   66          Cretaceous–Paleogene extinction, caused by a 10 km asteroid.
               Dinosaurs become extinct.
  201          Triassic-Jurassic extinction.  Cause unknown.
  252          Permian-Triassic extinction.  Runaway global warming
  370          Late-Devonian extinction.  Cause unknown.
  445          Ordovician-Silurian extinction events.  Global glaciation.

Organic chemistry

Propane with hydrogens included
Propane with hydrogen excluded

Molecules are often depicted with the hydrogens excluded.

Functional    Organic
group         molecule

C-H3          Alkane (lipid)
C-H2OH        Alcohol
C-OOH         Fatty acid (carboxylic acid)
C=O           Carbonyl group.  Aldehyde if at end, ketone if not at end
Humans can metabolize just about any chain hydrocarbon and any sugar.

Phenol
Tyrosine, an amino acid with a phenol


Opsins

Opsin         Wavelength  Humans   Notes
                 (nm)

Parapinopsin UV   365              Catfish
Neuropsin         380              Bird vision.  Found in the brains of humans
OPN1SW            440     Blue     All mammals
Panopsin Blue     450              Fish vision.  Found in the brains of humans
Parapinopsin Blue 470              Catfish and lamphrey
SWS2              480              Extinct in mammals
Melanopsin        480              Found in the brains of humans
VA                500              Vertebrates except mammals.  Vertebrae ancient opsin.
RH1               500     White    Black/White
Panopsin Cyan     500              Fish vision.  Found in the brains of humans
Pareitopsin       522              Lizards
OPN1MW            534     Green    All mammals
OPN1LW            564     Red      Once possessed by mammals, then lost by most
RH2               600              Black/White.  Extinct in mammals
NeoR              690              Fungus
Retinal G                          Found in the brains of humans

Porphyrins

Heme cofactor carrying an iron atom
Pyrrole

Metals are held by a cofactor, which is held by a protein. Many cofactors are porphyrin rings conposed of 4 pyrroles. Examples of porphyrins:

Porphin (Iron)
Corrin (Cobalt)
Corphin (Nickel)
Chlorophyll building blocks (Magnesium)

Porphin resonance
Porphin is an aromatic molecule because it is flat and because it resonates between different electronic states.


Hemoglobin

Heme A
Heme B
Heme C
Heme O
Hemo B
Hemoglobin
Myoglobin

Superoxide

Oxygen bonds to the iron in a heme molecule and becomes superoxide.
Hemoglobin is a set of 4 helix proteins that carry 4 iron ligands, and each iron ligand carries 1 oxygen molecule.
Human hemoglobin is composed mostly of heme B.
The oxygen density of hemoglobin is 70 times the solubility of oxygen in water.

Hemoglobin fraction of red blood cells   =  .96      (dry weight)
Hemoglobin fraction of red blood cells   =  .35      (including water)
Oxygen capacity of hemoglobin            = 1.34 Liters of oxygen / kg hemoglobin
Iron ligands per hemoglobin              =    4
O2 molecules per ion ligand              =    1

Chlorophyll

Chlorophyll A

Chlorophyll A
Chlorophyll B
Chlorophyll D

Chlorophyll C1
Chlorophyll C2
Chlorophyll F

All chlorophyll uses magnesium.

A      Universal
B      Plants
C1     Algae
C2     Algae
D      Cyanobacteria
F      Cyanobacteria

Zinc fingers

Zinc stabilizes the proteins that manipulate DNA and RNA.


Metal
Carbonic anhydrase
Element   Humans  Cofactor  Function

Hydrogen    *
Helium                      No biological role
Lithium                     No biological role
Beryllium                   Toxic becauseit displaces magnesium in proteins
Boron       *               Plant cell walls.  Metabolism of calcium in plants & animals
Magnesium   *     Chlorin   Chlorophyll
Scandium                    No biological role
Titanium                    No biological role
Vanadium                    Found only in rare bacteria.
Chromium                    No biological role
Manganese   *               Superoxide dimutase.  Converts superoxide to oxygen
Iron        *     Porphin   Hemoglobin
Cobalt      *     Corrin    Cobalamin (Vitamin B12)
Nickel            Corphin   Coenzyme F430 (Creates methane. Found only in archaea)
Copper      *     Heme      Cytochrome C oxidase. Electron transport chain
                            Hemocyanin, an alternative to hemoglobin used by some animals
                            Hemoglobin carries 4 times as much oxygen as hemocyanin
                            Plastocyanin protein, used in photosynthesis
                            Sometimes used in superoxide dimutase
Zinc        *               Component of proteins that manipulate DNA and RNA (Zinc fingers)
                            Component of carbonic anhydrase, which interconverts CO2 and HCO3
                            Metallothionein proteins, which bind to metals such as
                            zinc, copper, selenium cadmium, mercury, silver, and arsenic
Molybdenum                  Nitrogen fixase. Convert N2 to NH3
Selenium    *               Component of the amino acide selenocysteine
Bromine     *               Limited role
Iodine      *               Component of thyroxine and triiodotyronine, which
                            regulate metabolic rate
Lead                        Toxic because it displaces calcium in bones
Thyroxine
Triiodothyronine

Antioxidation

Superoxide dimutase
Superoxide dimutase, manganese in purple
Peroxidase

Bicarbonate
Carbonic acid
Hydrogen peroxide

Superoxide dimutase converts superoxide to oxygen or hydrogen peroxide.

The peroxidase enzyme decomposes hydrogen peroxide to water. Peroxidase contains the selenocysteine amino acid, which contains selenium.


Nitrogen fixation

Nitrogen fixase uses an iron-molybdenum cofactor.


Selenium

Selenocysteine

Selenium is a component of the amino acid selenocysteine.


Copper
Hemocyanin
Copper group without an oxygen
Copper group with an oxygen

The hemocyanin protein uses copper to carry oxygen. It has an oxygen density that is 1/4 of hemoglobin.

Plastocyanin is a copper-containing protein used in photosynthesis.

Plastocyanin


Oxides

Hydroxide
Water

Carbonate
Carbonic acid

Nitrate
Nitric acid

Nitrite
Nitrous acid

Silicate
Silicic acid

Phosphate
Phosphoric acid

Sulfate
Sulfuric acid

Potassium oxide
Selenium oxide
Fe2O3

OH-
CO3--
NO3-
NO2-
SiO4----
PO4---
SO4--

Iron(III) Oxide         Fe2O3        Ferric oxide.  Most common form
Iron(II) Oxide          FeO          Rare
Iron(II,III) Oxide      Fe3O4        Magnetite
Copper(I) Oxide         Cu2O         Cuprous oxide
Copper(II) Oxide        CuO          Cupric oxide
Copper(III) Oxide       Cu2O3

Lignin

Lignin is the structural component of wood.


Badass organisms

Extremophiles
Audax bacteria
Conan the Bacterium
Tardigrade

Audax: Lives underground, eats rock, and gets its energy from molecules generated by radioactivity. It can colonize a planet from scratch.

Conan: Survives radioactivity, outer space, acid, and freezing. It has four independent sets of chromosomes with active repair mechanisms.

Tardigrade (water bear): Survives temperatures from absolute zero to 161 C. Survives outer space. Found everywhere on the Earth from Mount Everest to the bottom of the ocean.

Colossal Squid

The colossal squid is up to 14 meters long, has eyes up to 27 cm in diameter, and inhabits the ocean at depths of up to 2 km.

Mantis Shrimp

The eyes of a Mantis shrimp have 12 color channels, including UV, and they are sensitive to linear and circular polarization. Each eye is trinocular, giving it a total of 6 channels for depth perception.

The Mantis shrimp has two clubs for striking.

Impact speed = 23 m/s
Acceleration = 10400 g  (similar to a .22 calibre bullet)
Impact force = 1500 Newtons
The strike produces cavitation bubbles that add to the damage.

Cheetah

Top speed of 33 meters/second
Accelerates from 0 to 28 meters/second in 3 seconds

White-throated Needletail

Fastest bird. Top horizontal speed of 45 meters/second.

Andean Condor

Mass of up to 15 kg
Wingspan of up to 3.1 meters

Argentavis

Mass of 75 kg
Wingspan of 7 meters
Wing loading of 85 Newtons/meter^2
Wing area of 8.1 meters^2
Extinct


Edward Lasker: While the Baroque rules of Chess could only have been created by humans, the rules of Go are so elegant, organic, and rigorously logical that if intelligent life forms exist elsewhere in the universe, they almost certainly play Go.


Astromusicology

          Red = equal tuning           Orange = just tuning

Just tuning is based on integer ratios and equal tuning is based on logarithms, and there is no direct connection between them. Fortuitously, 12-tone equal tuning gives a set of notes that are nearly identical to those for just tuning. The correspondence is close, but not exact, and violinists use a compromise between just and equal tuning that is situation dependent.

The synthesis of just and equal tuning offers rich contrapuntal possibilities, as was explored during the Baroque age by composers such as Vivaldi, Bach, and Handel.


                         Just and equal tuning

Note  Index  Interval      Equal  Just tuning  Major  Minor  Pythagorean
                           tuning              scale  scale  tuning
A       0   Unison         1.000  1.000 = 1/1    *      *      1/1
Bflat   1   Minor second   1.059                             256/243
B       2   Major second   1.122  1.125 = 9/8    *      *      9/8
C       3   Minor third    1.189  1.200 = 6/5           *     32/27
C#      4   Major third    1.260  1.250 = 5/4    *            81/64
D       5   Fourth         1.335  1.333 = 4/3    *      *      4/3
Eflat   6   Tritone        1.414                              729/512
E       7   Fifth          1.498  1.500 = 3/2    *      *      3/2
F       8   Minor sixth    1.587                        *    128/81
F#      9   Sixth          1.682  1.667 = 5/3    *            27/16
G      10   Minor seventh  1.782                        *     16/9
Aflat  11   Major seventh  1.888                 *           243/128
A      12   Octave         2.000  2.000 = 2/1    *      *      2/1
In equal tuning, the frequency ratio of an interval is

exp(Index/12)

Equal tuning is based on equal frequency ratios. Just tuning adjusts the frequencies to correspond to the nearest convenient integer ratio. For example, in equal tuning, the frequency ratio of a fifth is 1.498. Just tuning changes it to 1.500 = 3/2.

The 12-tone scale is ubiquitous in Earth music and it arises from elegant mathematics. If alien life plays music, they likely use the 12-tone scale.

The major and minor scales select 8 notes from the 12 note scale, favoring notes that have nice integer ratios.

Expanded discussion of just and equal tuning

History of music and mathematics

In the 6th century BCE, Pythagoras developed a 12-tone scale based on the ratios 2/1 and 3/2. This tuning was widely used until the 16th century CE. Pythagoriean tuning gives good results for fourths and fifths but poor results for thirds.

1572  Bombelli publishes complex numbers

1523  Pietro Anon introduced "meantone tuning" to fix the thirds, using a
      frequency ratio of 5/4 for major thirds.  His treatise "Thoscanello de la
      musica" expanded the possibilities for chords and harmony.

1555  Andrea Amati develops the four-string violin.

1584  "Equal tuning" introduced. Equal tuning divides the octave logarithmically.
      The first known examples of equal tuning were:
      Vincenzo Galilei in 1584  (Father of Galileo Galilei)
      Zhu Zaiyu in 1584
      Simon Stevens in 1585

1585  Simon Stevin introduces decimal numbers (For example, writing 1/8 as 0.125).
      This greatly expanded the calculational power of numbers.

1586  Simon Stevin drops objects of varying mass from a church tower to demonstrate that
      they accelerate uniformly.

1604  Galileo publishes a mathematical description of acceleration.

1614  Logarithms invented by John Napier, making possible precise calculations
      of equal tuning ratios.  Stevin's calculations were mathematically sound but
      the frequencies couldn't be calculated with precision until logarithms were
      developed.

1637  Cartesian geometry developed by Fermat and Descartes

1684  Leibniz publishes The Calculus

1687  Newton publishes the "Principia Mathematica"

1722  Bach publishes the "Well Tempered Clavier"
      Until ~ 1650, most keyboards used meantone tuning. This tuning gives good results if you
      confine yourself to a small number of keys and use few accidentals but it can't be made
      to work for all keys.
      J.S. Bach tuned his own harpsichords and clavichords and he customized the tuning to
      work in all 24 keys ("well temperament").  He demonstrated its effectiveness
      in "The Well Tempered Clavier".

1821  Cauchy publishes the "Cours d'Analyse", introducing rigor to mathematics.

Vibrato

Leopold Auer
Albert Einstein
Jascha Heifetz
Yehudi Menuhin

In the baroque age, violinists played with a pure, vibratoless tune, using bow speed rather than vibrato for expressivity. After the baroque age, an epidemic of vibrato emerged and is still with us, especially at Juilliard and Lincoln Center. Vibrato obstructs the resonances of just intonation.

"There are performers who tremble consistently on each note as if they had the permanent fever" - Leopold Mozart, 1756

The violinist and teacher Leopold Auer, in his book "Violin Playing as I Teach It" (1920), advised violinists to practise playing completely without vibrato, and to stop playing for a few minutes as soon as they noticed themselves playing with vibrato in order for them to gain complete control over their technique.

From the Wikipedia page on Yehudi Menuhin: After building early success, he experienced considerable physical and artistic difficulties caused by overwork during the war as well as unfocused and unstructured early training (reportedly he said "I watched myself on film and realized that for 30 years I'd been holding the bow wrong"). Careful practice and study combined with meditation and yoga helped him overcome many of these problems. When he finally resumed recording, he was known for practising by analyzing music phrases one note at a time.


Human skeleton


Atlas vertebra

Axis vertebra

Altazimuth telescope mount
Keck telescope altazimuth mount

The atlas vertebra functions like a telescope altazimuth mount

Roll
Pitch
Yaw

The Atlas-Skull joint controls pitch and the Axis-Atlas joint controls yaw.

Alexander Technique emphasizes gaining an awareness of these motions.

Neck ligaments
Neck muscles


Vision

Visual pathway
Motor cortex
Motor cortex

Visual information passes through the motor cortex before being combined at the rear of the brain. The brain and body are an image stabilization system for the eyes.


The muscles of the back are continuously connected between the shoulder blades and the hips, to coordinate motion of the limbs.


Balance

Bruce Lee: "Balance is the all-important factor in a fighter's attitude or stance. Without balance at all times, he can never be effective."

Jascha Heifetz masterclass In this clip, at time=5:45-6:15, Heifetz emphasizes the importance of balance and posture.

* Marie Daniels illustrates the importance of balance for playing the viola.

Balance flows from a stance with knees in and heels out.

* Gordon Liu demonstrates the wire style at time=4:37

Bruce Lee: "One should seek good balance in motion and not in stillness."

Bruce Lee: "Balance is the control of one's center of gravity plus the control and utilization of body slants and unstable equilibrium, hence gravity pull to facilitate movement. So, balance might mean being able to throw one's center of gravity beyond the base of support, chase it, and never let it get away."

* Jet Li and the Drunken Sword. Try this with a viola bow.

Bruce Lee: "The center of gravity kept under delicate and rapid motion are characteristic habbits of athletes in games that require sudden and frequent changes of direction." Bruce Lee: "The short step and the glide, as contrasted with the hop or cross step, are devices to keep the center of gravity. When it is necessary to move rapidly, a good man takes small enough steps so that his center of gravity is rarely out of control."

Bruce Lee: "In general for athletic contests, a preparatory stance a coiled, or semicrouched posture and a lowered, forward center of gravity. with the bending of the forward knee, the center of gravity moves forward a little. For general readiness, the lead heal usually remains just touching even after the knees bend. Slight ground contact of the heel aids in balance and decreases tension."


Hearing

Bruce Lee: Experiments indicate that auditory cues, when occurring close to the athlete, are responded to more quickly than visual ones. Make use of auditory clues together with visual clues, if possible. Remember, however, the focus of attention on general movement produces faster action than focus on hearing or seeing the cue.

Time in milliseconds:

.000003  Time for light to cross a 10 meter orchestra
    .2   Electric synapse. These synapses are 2-way and they do not amplify signals
   2     Chemical synapse. These synapses are 1-way and they can amplify signals
   1     Time for a neural signal to travel 10 cm, the size of a brain
  10     Time for a neural signal to travel from your fingers to your brain
   3     Time for sound to travel 1 meter, the distance to an adjacent musician
   7     Period of a 130 Hertz wave. This is the frequency of the viola C string
  30     Time for sound to travel across a 10 meter orchestra.
  62     Time between notes in "Flight of the Bumblebee"
For an orchestra to have good timing it must use visual cues. Sound isn't fast enough. This is especially true at the rear of the viola section amidst the cacophony of winds and brass.


History of Kung Fu

 -776       First Olympic games
 -648       The sport of "Pankration" is introduced in the Olympic Games. Similar to MMA.
 -536 -520  Milo of Croton dominates Olympic wrestling
 -450       Gautama Buddha develops the art of meditation
  464       Batuo, a monk from India, founds the Shaolin Temple
  500       Bodhidharma, a Buddhist monk, teaches at the Shaolin temple
 1600       Emergence of sumo in Japan
~1700       Shaolin temple destroyed by the Chinese Emperor.
            The monks who escaped spread Shaolin kung fu throughout China. These monks were:
            Ji Sin  - Developed Tiger Crane style
            Ng Mui  - Developed Wing Chun
            Bak Mei - Known as "Pai Mei" in kung fu films. Appears in "Kill Bill"
~1700       Fong Sai Yuk. Portrayed by Jet Li in the "Fong Sai Yuk" film series.
 1847 1924  Wong Fei Hung. Master of Hung Gar style. Portrayed by Jet Li in
            the "Once Upon a Time in China" film series.
 1860 1938  Jigoro Kano. Developed Judo and taught it to Mitsuyo Maeda and Moshe Feldenkrais
 1868 1910  Huo Yuanjia. Portrayed by Jet Li in the film "Fearless"
 1869 1955  F.M. Alexander. Developed "Alexander Technique"
 1893 1972  Yip Man. Practitioner of Wing Chun. Teacher of Bruce Lee
 1904 1984  Moshe Feldenkrais. Developed "Feldenkrais Technique"
 1917       Mitsuyo Maeda teaches Judo to the Gracie family.
            Helio Gracie subsequently develops Brasilian Jiu Jitsu
 1933       Jigoro Kano trains Feldenkrais in Judo
 1940 1973  Bruce Lee
 1940       Chuck Norris
 1951       Masahiko Kimura vs. Helio Gracie
 1952       Sammo Hung
 1954       Jackie Chan
 1955       Gordon Liu
 1963       Jet Li
 1963       Michelle Yeoh
 1963       Donnie Yen
 1970       Shaw Brothers Studios begins mass-producing kung fu films
 1993       Age of Mixed Martial Arts begins when Royce Gracie wins a tournament
              consisting of fighers with diverse styles.
 2000       Kazushi Sakuraba vs. Royce Gracie
 2009-      Ben Askren dominates MMA with wrestling
 2012       Miesha Tate vs. Ronda Rousey
 2013       Ben Askren signs with One FC.  UFC declines in significance

Interviewer:  Other than wrestling what would you say the best base to be a
              successful MMA fighter would be?
Ben Askren:   Wrestling

Aliens from film

Pierson's Puppeteer from the Niven universe


How long would it take an alien spacecraft to reach the Earth?

Hydrogen+oxygen rocket
VASIMR ion drive
Nuclear thermal rocket
Orion fusion rocket


Rocket propulsion system             Exhaust speed
                                        (km/s)
Hydrogen+oxygen rocket                     4.4
Chang-Diaz ion drive                      50          VASIMR design
Nuclear thermal rocket, H2 exhaust         9
Orion fusion rocket                    10000
Antimatter rocket                      1/2 C
All of these rockets are possible with current technology except for the antimatter rocket.


Distance to Alpha Centauri, the nearest star    4.3  light years
Milky Way diameter                              0.1  million light years
Distance to Andromeda                           2.5  million light years
Distance to the Virgo Supercluster             54    million light years
Light travel time during age of universe    13750    million light years

Age of the universe  ~  13.75 billion years
Age of the Earth     ~   4.54 billion years
An alien civilization in the Virgo Supercluster with a 1 billion year head start on us has plenty of time to get here.

The Doomsday Destroyer from Star Trek


Valence sites
   1           2        3          4           3          2          1          0
                                                                  Hydrogen    Helium
Lithium    Beryllium  Boron      Carbon     Nitrogen    Oxygen    Fluorine    Neon
Sodium     Magnesium  Aluminum   Silicon    Phosphorus  Sulfur    Chlorine    Argon
To be a part of a chain, an atom needs at least 2 valence sites and it needs to be able to form strong bonds.


Bond strengths in eV
       Single  Double  Triple   Quadruple
B  B    3.04
B  C    3.69
B  O    5.56
C  C    3.65   6.45    8.68   6.32
C  N    3.19   6.38    9.19
C  O    3.73   7.7    11.11
C  Si   3.30
C  P    2.74
C  S    2.82   5.94
N  N    1.76   4.33    9.79
N  O    2.08   6.29
N  Si   3.70
N  P
N  S
O  O    1.50   5.15
O  Si   4.69
O  P    3.47   5.64
O  S           5.41
Si Si   2.30
Si S    3.04
Si P
P  P    2.08
P  S           3.47
S  S    2.34   4.41
H  H    4.52
H  C    4.25
H  N    4.05
H  O    3.79
H  F    5.89
H  Si   3.30
H  P    3.34
H  S    3.76
H  Cl   4.48

96.47 kJoules/mol = 1 eV

Predictions about the aliens

Oxygen atmosphere
Fats and sugars for fuel
We'll be able to eat each other's food
As large as or larger than us
Flight is likely
Come from a small planet
Star is less hot than the sun
The planet is volcanic
The planet has a magnetic field
The planet has high metallicity


Problems

If a planet is close enough to a star it becomes tidally locked to the star. Mercury is just barely close enough for this and it orbits such that

3 * Orbit period = 2 * Spin period

If it were any closer it would be forced into a lock such that

Orbit period = Spin period

All of the solar system's moons are locked to their planets in this way. None of the planets are locked to their moons except Pluto.

For a low-mass star, the habitable zone is closer to the star than it is for the sun. If the star is sufficiently small, a planet in the habitable zone will be close enough to be locked to the star and will experience extreme weather.

Let L = Luminosity of a star / Luminosity of the sun (Watts). If a star is such that the habitable zone is at Mercury's orbit, what is L? What stellar mass corresponds to this luminosity?


Cellular biology
Dr. Jay Maron
jaymaron.com

Building blocks for life

       Minimum   Used by   Used    Human     Crust     Ocean   Atmosphere
       for life  humans   by life   ppt       ppt       ppt       ppt

Hydrogen    *       *        *    .10        1.5       108            .00055
Helium                                        .000008                 .0052
Lithium                                       .02
Beryllium                                     .0028
Boron               *        *    .0000007    .01
Carbon      *       *        *    .18        1.0          .028        .407
Nitrogen    *       *        *    .03         .02                  780
Oxygen      *       *        *    .65      460         858         210
Fluorine                     *                .5
Neon                                          .0000051                .018
Sodium      *       *        *    .0015     25          10.8
Magnesium   *       *        *    .0005     25           1.3
Aluminum                                    82
Silicon                      *             275
Phosphorus  *       *        *    .011       1.1
Sulfur      *       *        *    .0025       .4          .91
Chlorine    *       *        *    .0015       .2        19
Argon                                         .0035                  9.3
Potassium   *       *        *    .0025     20            .4
Calcium     *       *        *    .014      45            .4
Scandium                                      .022
Titanium                                     5.6
Vanadium                     *                .12
Chromium                                      .10
Manganese           *        *    .00000017   .95
Iron                *        *    .00006    60
Cobalt              *        *    .000000021  .025
Nickel                       *                .084
Copper              *        *    .000001     .06
Krypton                                                                .0011
Zinc                *        *    .000032     .075
Gallium                                       .019
Germanium                                     .0015
Arsenic                      *                .0018
Selenium            *        *    .00000019   .00005
Bromine             *        *    .0000029    .0024       .067
Molybdenum                   *                .0012
Tellurium                    *                .000001
Iodine              *        *    .00000016   .00045
Tungsten                     *                .0012

Among the elements required for life, nitrogen is the scarcest. The nitrogen in the first 250 km of the Earth's crust has the same mass as the nitrogen in the atmosphere.

The elements that are abundant in the crust and never used by life are aluminum and titanium.

All elements necessary for life are abundant in either the crust, the ocean, or the atmosphere.


ATP and ATP Synthase

Enzymes use ATP as an energy source to power chemical reactions. ATP and ATP synthase are common to all Earth life.

* Video of the ATP synthase enzyme in action


Cell walls
Lipids and cell membranes

Cell walls are formed from a double layer of lipids. They are elastic and they self-assemble.

Each lipid has a polar and a non-polar end. The polar end faces the water and the non-polar end faces another lipid.

* Video of the self-assembly of a bilipid layer
* Video of an amoeba

If life were to exist in a non-polar solvent it would have to find another way to make cell walls.


Amino acids

Amino acids have the above form, where R stands for an arbitrary molecule.

The 21 amino acids used by eucaryote life


Protein

Synthesis of two amino acids. Proteins are chains of animo acids with a backbone of the form:

C-C-N-C-C-N-C-C-N-C-C-N-C-C-N

DNA and the genetic code

DNA codes a sequence of amino acids. The 64-element codon system is universal to Earth life.

The codon ATG both codes for methionine and serves as an initiation site: the first ATG in an mRNA's coding region is where translation into protein begins.

21 amino acids are used by eucaryote. More than 500 amino acids are known.


Food

          MJoule/kg  Calories/gram

Sugar           17         5
Protein         17         5
Alcohol         25         7
Fat             38         9

ATP               .057
Phosphocreatine   .137

Hydrogen       143
Natural gas     53.6
Gasoline        47
Coal            24
Wood            16
Li-ion battery    .6

Hydrocarbons have good energy/mass and are good for energy storage. Sugars and fats are convenient hydrocarbons to metabolize, and humans can metabolize most of them.


Hydrocarbons

Methane
Ethane
Propane
Octane

An "Alkane" is a carbon chain with hydrocarbons attached. At standard temperature (300 K), alkanes are solid if they have more than 20 carbons. This is why lipids (long alkanes) are the optimal form of energy storage. Short alkanes are liquids or gases at STP and are hard to store.

In the following table, the first section shows properties of alkanes and the second section shows properties of other energy sources.

Alkane   Carbons  Energy of   Melt  Boil  Solid    Liquid    Gas       Phase at
type              combustion  (K)   (K)   density  density   density   300 K
                  (MJ/kg)                 (g/cm^3) (g/cm^3)  (g/cm^3)
Hydrogen     0     141.8      14.0   20.3           .07      .000090   Gas
Methane      1      55.5      90.7  111.7           .423     .00070    Gas
Ethane       2      51.9      90.4  184.6           .545     .0013     Gas
Propane      3      50.4      85.5  231.1           .60      .0020     Gas
Butane       4      49.5     136    274             .60      .0025     Gas
Pentane      5      48.6     143.5  309             .63                Liquid
Hexane       6      48.2     178    342             .65                Liquid
Heptane      7      48.0     182.6  371.5           .68                Liquid
Octane       8      47.8     216.3  398.7           .70                Liquid
Dodecain    12      46       263.5  489             .75                Liquid
Hexadecane  16      46       291    560             .77                Liquid
Icosane     20      46       310    616     .79                        Solid
Alkane-30   30      46       339    723     .81                        Solid
Alkane-40   40      46       355    798     .82                        Solid
Alkane-50   50      46       364    848     .82                        Solid
Alkane-60   60      46       373    898     .83                        Solid


Gasoline   ~ 8      47                               .76               Liquid     Mostly alkanes with ~ 8 carbons
Natural gas         54        91    112                                Gas        Mostly methane
Coal                32         -      -                                Solid      Mostly carbon
Wood                22         -      -                                Solid      Carbon, oxygen, hydrogen
Pure carbon  1      32.8       -      -                                Solid      Pure carbon, similar to coal
Methanol     1     175.6  337.8           .79                          Liquid
Ethanol      2     159    351.5           .79                          Liquid
Propanol     3     147    370                                          Liquid

An alkane with 7 or more carbons has a heat of combustion of 46 MJoules/kg.

A nitrogen molecule is more tightly bound than an oxygen molecule, making it impossible to extract energy from hydrocarbons with nitrogen. Few things burn in a nitrogen atmosphere, lithium and magnesium being examples.


Sugar

Glucose

A sugar generally has the formula CN H2N ON, where N = 2, 3, etc. The common sugars are hexoses with N=6.

         Number of   Number of
          carbons     sugars
Diose        2          1
Triose       3          2
Tetrose      4          3
Pentose      5          4
Hexose       6         12       At least 6 carbons are required to form a ring
Heptose      7       many       Rarely observed in nature
Octose       8       many       Unstable.  Not observered in nature.
"Number of sugars" refers to the number of different types of sugar molecules for each carbon number.

Each sugar molecule has two mirror-symmetric forms, the "D" and "L" form. Only the D forms are found in nature.

The following figures show all sugars up to 6 carbons. All can be metabolized by humans.

2 carbons:

Glycolaldehyde

3 carbons:

Glyceraldehyde
Dihydroxyacetone

4 carbons:

Erythrose
Threrose
Erythrulose

5 carbons:

Ribose
Arabinose
Lyxose
Xylose

6 carbons:

Glucose
Galactose
Mannose
Allose
Altrose
Gulose
Idose
Talose

Fructose
Sorbose
Psichose
Tagatose

         Energy  Sweetness

Succrose   1.00    1.00      Benchmark
Glucose             .74
Maltose             .32
Galactose           .32
Lactose             .16
Allose
Altrose
Mannose
Fructose           1.73
Psichose            .70
Tagatose    .38     .92
Sorbose            1.0
Honey               .97

Complex sugars
Monosaccharde:   1 sugar molecule
Disaccharide:    2 monosaccharides
Polysaccharide:  More than 2 monosaccharides, such as starch and cellulose
Sucrose
Maltose
Lactose
Lactulose
Trehalose
Sucrose    =  Glucose     + Fructose
Maltose    =  Glucose     + Glucose
Lactose    =  Galactose   + Glucose
Lactulose  =  Galactoce   + Fructose
Trehalose  =  Glucose     + Glucose
Cellobiose =  Glucose     + Glucose
Chitobiose =  Glucosamine + Glucosamine
Starch and cellulose are long chains of glucose molecules.

Starch
Cellulose


Synthesis


Metabolism

Fatty acid with 16 carbons
Sugar (glucose)
Acetyl
Pyruvic acid
H2O
CO2

Fatty acids and sugars are metabolized in the following stages, with each stage yielding energy.

Fatty acid    ->     Acetyl      ->     CO2 and H2O

Sugar         ->     Pyruvate    ->     CO2 and H2O

Blood delivers fatty acids to cells.

The citric acid cycle (Krebs cycle) converts acetyl or pyrovate into H2O and CO2. Coenzyme-A carries the acetyl around.


Fat metabolism

A fat molecule is converted into a fatty acid by lipolysis, and then the fatty acid is converted into acetyl by beta oxydation, and then the acetyl is converted into H2O and CO2 by the citric acid cycle.

Beta oxidation cleaves 2 carbons from a fatty acid, which becomes acetyl. This process is repeated until te entire fatty acid has been converted into acetyls.

The steps of beta oxidation are:


Sugar metabolism (glycolysis)

Glycolysis converts a glucose molecule into 2 pyrovate molecules. A summary of the reaction showing only the starting and ending points is:

The full reaction is:


Citric acid cycle

Citric acid

The citric acid cycle (Krebs cycle) converts acetyl or pyrovate into H2O and CO2.

Fat metabolism oxidizes a carbon chain so that the chain can be split into acetyl. The strategy of the citric acid cycle is to further oxidize the acetyl (now a part of citrate) so that the remaining carbon bonds in the acetyl can be broken.


Alcohol

An alcohol is a carbon chain with one OH attached.

Methanol
Ethanol
Propanol
Isopropanol
Butanol

          Carbons
Methanol     1       Toxic
Ethanol      2       Inebriating
Propanol     3       3 times more inebriating than ethanol
Isopropanol  3       Toxic
Butanol      4       6 times more inebriating than ethanol

Fatty acids (carboxylic acids)

Formic acid
Acetic acid
Palmitic acid

Palmitic acid has 16 carbons and is the most common fatty acid found in food.

Carbons
   1
   2    Vinegar
   3
   4    Found in butter
   8    Found in coconuts
  10    Found in coconuts
  12    Found in coconuts
  16    Most common fatty acid.  Found in palm oil
  18    Found in chocolate
  20    Found in peanut oil

Metabolism molecules

NADH
FAD
Guanosine triphosphate
Glucosamine
Acetic acid
Citric acid
Vitamin C


Toxic molecules

Formaldehyde

             LD50
            (mg/kg)
CO                     Carbon monoxide
HCN             6.4    Hydrogen cyanide
CH2O                   Methanol
CH2O                   Formaldehyde
H2S                    Hydrogen sulfide
NO2                    Nitrite
Cl2                    Chlorine
Fl2                    Fluorine
Ethanol      7060
Salt         3000
Caffeine      192
Aspirin       200
NaNO2         180      Sodium nitrite
Cobalt         80
NaF            52
Capsaicin      47      Chili pepper
Mercury        41
Arsenic        13
Nicotine         .8
Bromine
C2N2
PH3
SiCl4
Almost anything with fluorine or bromine is toxic.

Weakly toxic:

C2H2          Acetylene.  Inebriating
C3H6          Propene.  Inebriating

Spices

Cumin
Fennel
Caraway
Coriander
Cardamom
Fenugreek
Cubeb

Cashew
Pistachio
Walnut
Hazelnut
Peanut
Almond
Pine

Sesame
Poppy
Chia
Flax
Sunflower
Lotus

Black pepper
Mustard

Cumin
Turmermic
Paprika
Chili

Oregano
Basil
Bay
Coriander
Curry
Sage

Chive
Lemongrass
Tarragon
Arugula
Mint
Dill
Marjoram

Rosemary
Parsley
Saffron
Juniper

Bell pepper
Chili
Jalapeno
Cayenne
Habanero

Onion
Garlic
Clove
Galangal
Cinnamon
Vanilla

Portobello
Shiitake
Oyster
Morel
Enoki
Porcini
Truffle

Olea europaea
Kalamata
Arbequina
Belice

Grapefruit
Orange
Tangerine
Lemon
Lime
Kaffir lime
Key lime
Kiwi

Tomato
Avocado
Coconut
Egg
Olive oil

Milk cream
Sour cream
Butter
Cream cheese
Yogurt

Parmesan
Mozzarella
Reggiano
Asiago

Adzuki
Kidney
Red
Black
Pinto

Coffee
Cacao
Kola

Salt
Monosodium glutamate


Spices

Turmeric: curcumin
Cumin: cuminaldehyde
Chili: capsaicin
Mustard: allyl isotyiolcyanate

Bay: myrcene
Garlic and onion: allicin
Clove: eugenol

Raspberry ketone
Tangerine: tangeritin
Lemon: citral
Lemon peel: limonene

Chocolate: theobromine
Smoke: guaiacol
Cardamom: terpineol
Wintergreen: methyl salicylate

Hydrogen   White
Carbon     Black
Nitrogen   Blue
Oxygen     Red
Sulfur     Yellow
        Scoville scale (relative capsaicin content)

Ghost pepper     1000000
Trinidad         1000000      Trinidad moruga scorpion
Naga Morich      1000000
Habanero          250000
Cayenne pepper     40000
Malagueta pepper   40000
Tabasco            40000
Jalapeno            5000
Guajillo pepper     5000
Cubanelle            500
Banana pepper        500
Bell pepper           50
Pimento               50

Molecule        Relative hotness

Rresiniferatoxin   16000
Tinyatoxin          5300
Capsaicin             16         Chili pepper
Nonivamide             9.2       Chili pepper
Shogaol                 .16      Ginger
Piperine                .1       Black pepper
Gingerol                .06      Ginger
Capsiate                .016     Chili pepper
Caraway: carvone
Black tea: theaflavin
Cinnamon: cinnamaldehyde
Citrus: hesperidin
Fruit: quercetin

Mint: menthol
Juniper: pinene
Saffron: picrocrocin
Saffron: safranal
Wine: tannic acid

Black pepper: piperine
Oregano: carvacrol
Sesame: sesamol
Curry leaf: girinimbine
Aloe emodin
Whiskey lactone


Signalling molecules

Alcohol
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Materials science and elasticity
Dr. Jay Maron


Tensile stress

For a rod under tension,

Rod cross-sectional area = A         meter2
Tensile force            = F         Meter
Tensile stress           = P = F/A   Pascal

Strain

Tensile strain is stretching, and is measured as a fractional change in length. For a rod under strain,

Rod length            =  X         Meter
Rod change in length  =  x         Meter
Strain                =  s  = x/X  Dimensionless

Tensile modulus

The tensile modulus is resistance to strain, and can be thought of as stiffness. This is a form of Hooke's law. For a rod under stress,

Stress on the rod     = P        Pascals
Rod tensile modulus   = T        Pascals
Rod strain            = s = P/T  Dimensionless


Tensile strength

A material's "tensile strength" is the maximum tensile stress it can take before breaking.

Tensile strength      =  tbreak              Newton/meter2   (Pascals)
Cross-sectional area  =  A                  meter2
Breaking force        =  Fbreak = tbreak A    Newton

Yield strength

A material's "tensile yield strength" is the maximum stress it can take before deforming irreversibly. For metals, the yield strength is usually 3/4 of the tensile strength, and for wood, the yield strength is only slightly less than the tensile strength.

For engineering, we focus on yield strength rather than tensile strength.


Elasticity data


Yield strain

A material's "tensile yield strain" is the maximum strain it can take before yielding. For metals, the value varies widely.

Alloying a metal doesn't change the tensile modulus, but it improves yield strain.

Yield strength    =  t          Pascals
Tensile modulus   =  T          Pascals
Yield strain      =  S  =  t/T  Dimensionless


Variables

Density                =  ρ          kg/meter2

Cross-sectional area   =  A          meter2
Force                  =  F          Newton
Tensile stress         =  P  =  F/A  Pascals

Tensile modulus        =  T          Pascals
Tensile yield stress   =  t          Pascals
Tensile breaking stress=  tbreak      Pascals

Strain                 =  s  =  P/T  Dimensionless
Tensile yield strain   =  S  =  t/T  Dimensionless

Tensile energy/volume  =  evol =  ½ T s2     Joule/meter3
Tensile energy/mass    =  e   =  ½ T s2/ρ    Joule/kg

Textbook on elasticity


Strong metals

The table shows the "strong metals", the metals with good strength/density.


Modulus/Density

For bridges, what counts is strength/density.

For wood and for the strong metals,

Tensile modulus / Density  ~  25 MJoules/kg

Beryllium is an exception, with a value of 137 MJoules/kg.

The plot shows the tensile modulus divided by density.


Energy/mass

For many applications, the measure of the quality of a material is the elastic energy/mass it can take before yielding. For this, a material should have a large tensile modulus and a large yield strain.

Tensile modulus        =  T
Tensile yield strength =  t
Tensile yield strain   =  S
Density                =  ρ
Tensile energy/volume  =  evol =  ½ T S2       Joule/meter3
Tensile energy/mass    =  e    =  ½ T S2/ρ     Joule/kg

The best materials are polymers such as Kevlar.

Alloys outperform pure metals. The best alloy is titanium alloy.


Deformation

The types of deformation are tension, shear, and bulk compression.

Tensile
Shear
Bulk compression


Poisson ratio

A wire shortens when stretched and widens when compressed.

dX            =  Fractional increase in length of the wire
dY            =  Fractional decrease in diameter of the wire
PoissonRatio  =  dY / dX

For an isotropic material, the tensile, shear, and bulk moduli are related through the dimensionless Poisson ratio.

Tensile modulus        =  T          Pascals
Shear modulus          =  Tshear     Pascals
Bulk modulus           =  Tbulk      Pascals
Poisson ratio          =  U          dimensionless

T  =  2 (1 + U) Tshear  =  3 (1 - 2U) Tbulk

Beams

For beams, the types of stresses are:

Tension
Bending
Compression


Tension

Tensile strength relates to the strength of wires.

Two vices pull on a wire

Tensile yield strength =  t          Newton/meter2   (Pascals)
Cross-sectional area   =  A          meter2
Yield force            =  F  = tA    Newton

Bending

For bending, the yield force of a beam is determined by the shear yield strength.

Beam length            =  X   meter
Beam width             =  Y   meter
Beam height            =  Z   meter          The force is in the Z direction
Beam yield force       =  f   Newton
Tensile yield strength =  t   Pascal
Poisson ratio          =  U   dimensionless
Shear yield strength   =  tshear = ½ t / (1+U)   Pascal
Bending yield force    =  f  =  ⅔ tshear Y Z2 / X

Z matters more than Y. If you have a beam with a 2x4 cross section, it's best to align the beam so that Z=4 and Y=2, rather than with Z=2 and Y=4.


Column crushing

Short columns fail by crushing and long columns fail by buckling.

Crushing strength is determined by bulk yield strength.

Bulk yield strength  =  tbulk        Newton/meter2   (Pascals)
Cross-sectional area =  A            meter2
Crushing force       =  F  = bbulkA  Newton

Column buckling

Long columns fail by buckling, and strength is determined by tensile yield strength.

For a column that is cylindrical and hollow,

Column length          =  L
Column outer radius    =  R
Column inner radius    =  r
Column boundary factor =  K        dimensionless
                       =   .5      if both ends are fixed
                       =  2        if one end is fixed and the other end is free to move laterally
                       =  1        if both ends are pinned  (hinged and free to rotate)
                       =   .699    if one end is fixed and the other is pinned
Tensile yield strength =  t
Buckling force         =  f  =  ½ π3 t (R4-r4) / (K L)2

Buckling threshold

If a column's buckling limit is equal to its squashing limit, and if r=0,

R/L  =  (K/π) (tbulk/t)1/2

Beam scalings

Beam length            = L
Beam radius            = R
Beam tension strength  ~  R2
Beam bending strength  ~  R3/L
Beam buckling strength ~  R4/L2

Beams and density

For beams and columns, the lower the density, the better.

For a square beam with Y=Z,

Density           =  ρ
Mass              =  M  =  X Y Z ρ
Beam yield force  =  F  =  ⅔ s Y Z2 / X  =  ⅔ S M3/2 ρ-3/2 / X5/2

At fixed length and mass, the measure of quality is t/ρ3/2.


Columns and density

For a cylindrical column,

Density                =  ρ
Mass                   =  M  =  π R2 L ρ
Column effective length=  K                 = 1/2   dimensionless        For a column that's fixed at both ends
Column buckling force  =  F  =  ½ π3 t R4 / (K L)2  =  ½ π3 t M2 ρ-2 / (K2 L4)

At fixed length and mass, the measure of quality is t ρ-2.


Quality

The measure of merit depends on the application. If force/mass is what counts, then the measure of merit is

Tensile yield strength / Density         Beam under tension
Tensile yield strength / Density3/2      Beam under shear
Tensile yield strength / Density2        Beam under compression

Energy/Mass

For many applications, the measure of merit for a material is energy/mass, where "energy" is the maximum elastic energy the material can take before breaking. This applies to things like racquets, aircraft, and swords. The cases are:

Case            Measure of merit

Tension         Energy / Mass
Shear           Energy / Mass / Density1/2
Compression     Energy / Mass / Density

Strong woods

The strongest woods are:

              Density   Tensile   Tensile  Hardness
                        strength  modulus
              gram/cm3  GPascal   GPascal  kNewton

 Balsa            .12    .020     3.7      .31
 Cedar, white     .32    .046     5.7
 Cedar, red       .34    .054     8.2
 Pine, white      .37    .063     9.0     1.9
 Spruce, red      .41    .072    11.7
 Redwood          .44    .076     9.6
 Ash, black       .53    .090    11.3
 Walnut, black    .56    .104    11.8     4.5
 Ash, white       .64    .110    12.5     5.9
 Mahogany         .67    .124    10.8
 Locust, black    .71    .136    14.5     7.6
 Hickory          .81    .144    15.2
 Bamboo           .85    .15     20.0     7.2
 Oak, live        .98    .13     13.8
 Ironwood        1.1     .181    21.0    14.5
 Verawood        1.19    .178    15.7    16.5
 Quebracho       1.24    .14     16.6    20.3
 Lignum vitae    1.26    .127    14.1    19.5
 Ironwood, black 1.36    .125    20.5    16.3

Wood Strength/Density

Tensile yield strength  =  t   Pascal
Density                 =  ρ   kg/meter3

For most woods, t/ρ has a similar value. For t/ρ2, balsa wins. We plot t/ρ, t/ρ3/2, and t/ρ2.


Wood Energy/Density


Materials

To compare wood to other materials,


Wood grain

For a vertical tree trunk, "longitudinal" is the vertical direction. "Radial" is the direction from the tree center axis, going outward in the horizonal plane. "Tangential" is the direction along a tree ring, in the horizontal plane.

Poisson numbers:

                 Longitudinal  Radial  Tangential

Wood, low density    .4         .25       .2
Wood, high density   .43        .35       .18

The strongest direction is the longitudinal direction and the weakest direction is the radial direction. For a beam under bending stress, you should align the longitudinal grain with the long axis of the beam, and you should align the tangential grain with the direction of the force.


Bridge design

Truss

Brown truss
Pratt truss
Pratt truss
Howe truss
Bowstring truss

A hollow beam is weaker than a solid beam, but it has a better stength/mass ratio. This is the point of a truss. A truss consists of a set of upper and lower beams connected by struts. The struts deliver forces between the beams and they resist warp. Struts are arranged as triangles because triangles resist warp better than squares.

In a Pratt truss, diagonal beams are under tension and vertical beams are under compression.

A Howe truss is like a Pratt truss except that the diagonals slant the opposite way. In a Howe truss, diagonal beams are under compression and vertical beams are under tension.

Beams under compression should be wider than beams under tension. Compression is harder than tension.

Bridges from centuries ago tended to use wood for compression elements and steel rods for tension elements.


Triangles

Triangles are stronger than squares. A structure needs triangles to resist warping.


3D truss

Diamond lattice
Diamond lattice


Suspension bridge

Tension is easy. If you can use pure tension, do it.


Catenary

Roman bridge

A cable hangs as a catenary, and the ideal form for an arch is a catenary.

A hanging catenary transforms the load into pure tension.

An arch transforms the load into pure compression.

For a suspension bridge supporting a road, if the cable is heavier than the road, then the cable hangs as a catenary. If the road is heavier than the cable, the cable hangs as a parabola.


Tower

If you want height, use a concave catenary. If you want volume, use a convex catenary.


Arch bridge

The arch can go above or below.


Arch and truss

You can combine an arch and a truss.


Cantor design


Compressive strength

Tension
Compression

Concrete and ceramics typically have much higher compressive strengths than tensile strengths. Concrete is typically mixed with steel bars to improve tensile strength.


Hardness

Brinell hardness test
Vickers hardness test

Diamond indenter for a Vickers hardness test
Indentation left in steel by a diamond indenter

Brinell  =  A measure of a material's resistance to dents, measured in Pascals
Mohs     =  A dimensionless measure of a material's resistance to dents
The Mohs scale of mineral hardness reflect's a material's ability to resist scratching. If two materials are scraped together then the material with the lower Mohs value will be scratched more. Diamond has the largest Mohs value of any material.
                Mohs

Diamond          10
RhB2              9.5
Silicon carbide   9.5
Corundum          9
Tungsten carbide  9
Chromium          8.5
Emerald           8
Topaz             8
Tungsten          8
Hardened steel    8
Quartz            7
Osmium            7
Rhenium           7
Vanadium          7

If a material has a large Brinell hardness then it has a large Mohs hardness. The reverse is not necessarily true. Materials exist with a large Mohs hardness and a small Brinell hardness.



The Brinell hardness is related to the tensile modulus and tensile strength.





Elasticity

For tension, what usually matters is tensile strength divided by density. Materials with a high value include:

              Young's  Yield   Tensile  Tensile  Strength/   Tough/   Density
              modulus  stress  strengh  strain    density    density
                GPa     Gpa      GPa             MNewton/kg  kJ/kg    g/cm^3

Graphene          1050         160       .152     160      12190      1.0
Nanotube          1000          63       .063      48       1480      1.34   Carbon nanotube
Colossal tube     1000           7                                     .116  Carbon nanotube with large radius

Zylon              270           5.8     .010       3.7               1.56
Kevlar             155           3.76    .023       2.6               1.44
Vectran UM         103           3.0     .029                         1.4
Vectran HT          75           3.2     .043                         1.4
Vectran NT          52           1.1     .021                         1.4


Diamond           1220    1.6    2.8     .0023       .80        .92   3.5
Sapphire           345     .4    1.9     .0055       .48       1.315  3.98

Carbon fiber       181           1.6     .0088       .91       4.04   1.75
Rubber, butyl         .007        .020  2.86                           .92

Balsa                3.7   .020                                        .12
Pine, white          9     .063                                        .37
Bamboo              20     .15                                         .85
Ironwood            21     .181   .181   .0086                  .65   1.1

Beryllium          287     .345   .448   .0016                  .189  1.85
Magnesium + Li      45     .14                                        1.43
Magnesium + Y2O3    45     .31                                        1.76
Magnesium alloy     45     .100   .232   .0052                  .344  1.74
Aluminum  + Be      70     .41                                        2.27
Aluminum alloy      70     .414   .483   .0069                  .595  2.8
Titanium           120     .225   .37    .0031                  .054  4.51
Steel + Co, Ni     220    2.07           .0094                        8.6
Moly + W, Hf              1.8                                          14.3

Aluminum amorphous  70    1.97                                        2.67   LiMgAlScTi
Titanium amorphous 120    1.20                                        4.6    Titanium + AlVCrMo
Chromium amorphous        2.26                                        6.5    AlCrFeCoNiTi
Molybden amorphous        1.22                                       12.3    VNbMoTaW
Molybdenum + W, Hf        1.8                                        14.3

Polymers

Zylon
Vectran
Aramid (Kevlar)
Polyethylene

Aramid
Nylon
Hydrogen bonds in Nylon

Spider silk
Lignin

Lignin comprises 30 percent of wood and it is the principal structural element.


Rope

               Year   Young  Tensile  Strain  Density   Common
                      (GPa)  strength         (g/cm3)   name
                              (GPa)
Gut           Ancient           .2
Cotton        Ancient                   .1       1.5
Hemp          Ancient   10      .3      .023
Duct tape                       .015
Gorilla tape                    .030
Polyamide      1939      5     1.0      .2       1.14    Nylon, Perlon
Polyethylene   1939    117                       1.4     Dacron
Polyester      1941     15     1.0      .067     1.38
Polypropylene  1957                               .91
Carbon fiber   1968            3.0               1.75
Aramid         1973    135     3.0      .022     1.43    Kevlar
HMPE           1975    100     2.4      .024      .97    Dyneema, Spectra
PBO            1985    280     5.8      .021     1.52    Zylon
LCAP           1990     65     3.8      .058     1.4     Vectran
Vectran HT              75     3.2      .043     1.41    Vectran
Vectran NT              52     1.1      .021     1.41    Vectran
Vectran UM             103     3.0      .029     1.41    Vectran
Nanorope             ~1000     3.6      .0036    1.3
Nanotube              1000    63        .063     1.34
Graphene              1050   160        .152     1.0


Strain  =  Strength / Young
Carbon fiber is not useful as a rope.

A string ideally has both large strength and large strain, which favors Vectran.

Suppose Batman has a rope made out of Zylon, the strongest known polymer.

Batman mass            =  M         =    100 kg               (includes suit and gear)
Gravity constant       =  g         =     10 meters/second2
Batman weight          =  F         =   1000 Newtons
Zylon density          =  D         =   1520 kg/meter3
Zylon tensile strength =  Pz        = 5.8⋅109 Newtons/meter2
Rope load              =  P         = 1.0⋅109 Newtons/meter2   (safety margin)
Rope length            =  L              100 meters
Rope cross section     =  A  = F/P  =1.0⋅10-6 meters2
Rope radius            =  R  =(A/π)½=     .56 mm
Rope mass              =  Mr = DAL  =     .15 kg

Wood

         Density   Tensile   Young
                   strength
         (g/cm^3)  (Gpa)     (Gpa)

Balsa         .12    .020      3.7
Corkwood      .21
Cedar         .32    .046      5.7     Northern white
Poplar        .33    .048      7.2     Balsam
Cedar         .34    .054      8.2     Western red
Pine          .37    .063      9.0     Eastern white
Buckeye       .38    .054      8.3     Yellow
Butternut     .40    .057      8.3
Basswood      .40    .061     10.3
Spruce, red   .41    .072     10.7
Aspen         .41    .064     10.0
Fir, silver   .42    .067     10.8
Hemlock       .43    .061      8.5     Eastern
Redwood       .44    .076      9.6
Ash, black    .53    .090     11.3
Birch, gray   .55    .069      8.0
Walnut, black .56    .104     11.8
Ash, green    .61    .100     11.7
Ash, white    .64    .110     12.5
Oak, red      .66    .100     12.7
Elm, rock     .66    .106     10.9
Beech         .66    .102     11.8
Birch, yellow .67    .119
Mahogany      .67    .124     10.8     West Africa
Locust        .71    .136     14.5     Black or Yellow
Persimmon     .78    .127     14.4
Oak, swamp    .79    .124     14.5     Swamp white
Gum, blue     .80    .118     16.8
Hickory       .81    .144     15.2     Shagbark
Eucalyptus    .83    .122     18.8
Bamboo        .85    .169     20.0
Oak, live     .98    .130     13.8
Ironwood     1.1     .181     21.0
Lignum Vitae 1.26    .127     14.1
Data #1     Data #2
Plastic

           Density   Tensile   Young
                     strength
           (g/cm^3)  (Gpa)     (Gpa)


Polyamide            .11       4.5
Polyimide            .085      2.5
Acrylic              .07       3.2
Polycarbonate        .07       2.6
Acetyl copoly        .06       2.7
ABS                  .04       2.3
Polypropylene  .91   .04       1.9
Polystyrene          .04       3.0
Polyethylene   .95   .015       .8

Alloys

Copper
Orichalcum (gold + copper)
Gold

Alloy of gold, silver, and copper


Superstrong amorphous alloys

Crystal, polycrystal, amorphous

New alloys have been discovered that are stronger and ligher than diamond. These alloys have an amorphous structure rather than the crystalline structure of conventional alloys. A crystaline alloy tends to be weak at the boundaries between crystals and this limits its strength. Amorphous alloys don't have these weaknesses and can be stronger.

Pure metals and alloys consisting of 2 or 3 different metals tend to be crystaline while alloys with 5 or more metals tend to be amorphous. The new superalloys are mixes of at least 5 different metals.

A material's strength is characterized by the "yield strength" and the quality is the ratio of the yield strength to the density. This is often referred to as the "strength to weight ratio".

Yield strength  =  Y            (Pascals)
Density         =  D            (kg/meter3)
Quality         =  Q  =  Y/D    (Joules/kg)
The strongest allyos are:
       Yield strength   Density   Quality
       (GPa)        (g/cm3)    (MJoule/kg)

Magnesium + Lithium             .14        1.43        98
Magnesium + Y2O3                .31        1.76       177
Aluminum  + Beryllium           .41        2.27       181
Amorphous LiMgAlScTi           1.97        2.67       738
Diamond                        1.6         3.5        457
Titanium  + AlVCrMo            1.3         4.6        261
Amorphous AlCrFeCoNiTi         2.26        6.5        377
Steel     + Cobalt, Nickel     2.07        8.6        241
Amorphous VNbMoTaW             1.22       12.3         99
Molybdenum+ Tungsten, Hafnium  1.8        14.3        126
The strongest pure metals are weaker than the strongest alloys.
       Yield strength   Density   Quality
       (GPa)        (g/cm3)    (MJoule/kg)

Magnesium                        .10       1.74        57
Beryllium                        .34       1.85       184
Aluminum                         .02       2.70         7
Titanium                         .22       4.51        49
Chromium                         .14       7.15        20
Iron                             .10       7.87        13
Cobalt                           .48       8.90        54
Molybdenum                       .25      10.28        24
Tungsten                         .95      19.25        49

Alloy types
Beryllium + Li           →  Doesn't exist. The atoms don't mix
Beryllium + Al           →  Improves strength
Magnesium + Li           →  Weaker and lighter than pure Mg. Lightest existing alloy
Magnesium + Be           →  Only tiny amounts of beryllium can be added to magnesium
Magnesium + Carbon tubes →  Improves strength, with an optimal tube fraction of 1%
Aluminum  + Li,Mg,Be,Sc  →  Stronger and lighter than aluminum
Titanium  + Li,Mg,Sc     →  Stronger and lighter than titanium
Steel     + Cr,Mo        →  Stronger and more uncorrodable than steel. "Chromoly"
Copper    + Be           →  Stronger than beryllium and is unsparkable

High-temperature metals (refractory metals)
          Melting point (Celsius)

Tungsten    3422
Rhenium     3186
Osmium      3033
Tantalum    3017
Molybdenum  2623
Niobium     2477
Iridium     2446
Ruthenium   2334
Hafnium     2233
Technetium  2157
Rhodium     1964
Vanadium    1910
Chromium    1907

High-temperature superalloys

Most alloys weaken with increasing temperature except for a small subset called "superalloys" that strengthen with temperature, such as Ni3Al and Co3Al. This is called the "yield strength anomaly".

Nickel alloys in jet engines have a surface temperature of 1150 Celsius and a bulk temperature of 980 Celsius. This is the limiting element for jet engine performance. Half the mass of a jet engine is superalloy.

Current engines use Nickel superalloys and Cobalt superalloys are under development that will perform even better.

Yield strength in GPa as a function of Celsius temperature.

                   20   600   800  900  1000  1100 1200  1400  1600 1800  1900  Celsius

VNbMoTaW          1.22         .84        .82       .75  .66   .48   .4
AlMohNbTahTiZr    2.0   1.87  1.60  1.2   .74  .7   .25
Nickel superalloy 1.05        1.20   .90  .60  .38  .15
Tungsten           .95   .42   .39        .34  .31  .28  .25   .10   .08  .04
Below 1100 Celsius AlMohNbTahTiZr has the best strength-to-mass ratio and above this VNbMoTaW has the best ratio. Both alloys supersede nickel superalloy and both outperform tungsten, the metal with the highest melting point. Data:   
Entropy, nickel superalloy
Copper alloys
                  Yield strength (GPa)

Copper                  .27
Brass                   .41     30% zinc
Bronze                  .30     5% tin
Phosphor bronze         .69     10% tin, .25% phosphorus
Copper + beryllium     1.2      2% beryllium, .3% cobalt
Copper + nickel + zinc  .48     18% nickel, 17% zinc
Copper + nickel         .40     10% nickel, 1.25% iron, .4% manganese
Copper + aluminum       .17     8% aluminum

Bells and cymbals

Bells and cymbals are made from bell bronze, 4 parts copper and 1 part tin.


Fullerines

Buckyball with 540 atoms
Buckyball with 60 atoms
Buckyballs in the liquid phase

Nanotube

Buckyballs in a nanotube
Graphene


3D printer materials

                   Young's  Tensile   Hardness  Max temp  Density  Toughness  Price/kg
                   modulus  strength                               /density   
                     GPa      MPa     Shore D   Celsius    g/cm3   kJoule/kg    $/kg


PVA                  1.5      78        72        64       1.23      1650      75
PC Polycarbonate     2.2      65        82       112       1.23                58
PLA                  3.2      65        84        56       1.32
PLA Tough            2.8      46        84        56       1.32
PAHT CF15            5.2      66        72       127       1.10
Nylon                1.8      60        81        88       1.15                45
ASA                  2        55       110        95       1.07                39
PETG                 2.0      50        71        70       1.27                40
TPU                   .2      40        48       110       1.45
Carbon fiber filled  4        46                  52       1.3
Flexible              .2      37        10        67       1.21                50
ABS                  1.9      40        76        95       1.07
HIPS                 4        32        77       100       1.04                28
PP Polypropylene     1        30        42        90        .9                 90
PP GF30              2.6      42        42       126        .9
Metal filled         4        25                  52       3                   85
PA                    .4      35        73       100       1.00

Diamond           1220       1600                          3.5        300
Graphene          1050     160000                          1.0
Kevlar             112       3620                170       1.44     40600           Aramid
Zylon              270       5800                          1.56                     PBO, Polyoxazole
Vectran             11.5      140                          1.40
Rubber, butyl         .004     17                          1.25     28900
Carbon fiber       228       3500       88                 1.8      16000

Balsa                3.7       20        4.9                .2
Bamboo              20        150       70                  .85
Ironwood            21        181       90                 1.1

Beryllium alloy    287        500                          2.1
Magnesium alloy     45        260                          1.74
Aluminum alloy      70        590                          2.7
Titanium alloy     116       1100                          4.51      1160
Iron alloy         211       1500                          7.9
Tungsten alloy     441       2100                         19.25

Zylon
Kevlar
Vectran
Nylon
Neoprene rubber

PVA
PC Polycarbonate
PLA


Ancient metallurgy

Stone
Copper
Bronze
Iron
Carbon

Gold and silver were known since antiquity because they occur naturally in pure form. Gold mining started in 6000 BCE and silver smelting started in 4000 BCE.

Iron can occasionally be found as iron meteorites.

Gold nugget
Silver nugget
Iron meteorite

Copper was discovered around 7500 BCE by smelting copper minerals in a wood fire. Around 3200 BCE it was found that copper is strenghened by tin, and this is bronze. Around 2000 BCE it was found that copper is also strengthed by zinc, and this is brass.

The earliest metals were smeltable with a wood fire and they consist of copper, lead, silver, tin, zinc, and mercury. They come from the following minerals:

Lead. Galena. PbS
Copper. Chalcocite. Cu2S
Silver. Acanthite. Ag2S
Tin. Cassiterite. SnO2
Zinc. Sphalerite. ZnS
Mercury. Cinnabar. HgS

The next metal to be discovered was iron (c. 1200 BC), which requires a bellows-fed coal fire to smelt.

Iron. Hematite. Fe2O3
Iron. Pyrite. FeS2

No new metals were discovered until cobalt in 1735. Once cobalt was discovered, it was realized that new minerals may have new metals, and the race was on to find new minerals. This gave nickel, chromium, manganese, molybdenum, and tungsten.

Cobalt. Cobaltite. CoAsS
Nickel. Millerite. NiS
Chromium. Chromite. FeCr2O4
Manganese. Pyrolusite. MnO2
Molybdenum. Molybdenite. MoS2
Tungsten. Wolframite. FeWO4

Chromium is lighter and stronger than steel and was discovered in 1797. It satisfies the properties of mithril from "Lord of the Rings" and Valyrian steel from "Game of Thrones". There's no reason chromium couldn't have been discovered earlier.

Coal smelting can't produce the metals lighter than chromium. These need electrolysis. The battery was invented in 1799, enabling electrolysis, and the lighter metals were discovered shortly after. These include aluminum, magnesium, titanium, and beryllium. Once you have

Aluminum. Bauxite. Al(OH)3 and AlO(OH)
Mangesium. Magnesite. MgCO3
Titanium. Rutile. TiO2
Beryllium. Beryl. Be3Al2(SiO3)6

Carbon fiber eclipses metals. The present age could be called the carbon age. The carbon age became mature in 1987 when Jimmy Connors switched from a wood to a carbon racket.

The plot shows the strength of materials.

Alloys can be much stronger than pure metals.

Wood rivals alloys for strength.


Currency

Gold was the densest element known until the discovery of platinun in 1735. It was useful as an uncounterfeitable currency until the discovery of tungsten in 1783, which has the same density as gold. Today, we could use iridium, platinum, or rhenium as an uncounterfeitable currency.


Modern chemistry and the discovery of elements

Prior to 1800, metals were obtained by smelting minerals, and the known metals were gold, silver, copper, iron, tin, zinc, mercury, cobalt, manganese, chromium, molybdenum, and tungsten. Elements to the left of chromium titanium and scandium cant's be obtained by smelting, and neither can aluminum, magnesium, and beryllium. They require electrolysis, which was enabled by Volta's invention of the battery in 1799.

Prior to 1800, few elements were known in pure form. Electrolyis enabled the isolation of most of the rest of the elements. The periodic table then became obvious and was discovered by Mendeleev 1871. The battery launched modern chemistry, and the battery could potentially have been invented much earlier.

Electrolysis enabled the isolation of sodium and potassium in 1807, and these were used to smelt metals that can't be smelted with carbon.

         Discovery   Method of             Source
          (year)     discovery

Carbon     Ancient   Naturally occuring
Gold       Ancient   Naturally occuring
Silver     Ancient   Naturally occuring
Sulfur     Ancient   Naturally occuring
Lead         -6500   Smelt with carbon     Galena       PbS
Copper       -5000   Smelt with carbon     Chalcocite   Cu2S
Bronze (As)  -4200   Copper + Arsenic      Realgar      As4S4
Tin          -3200   Smelt with carbon     Calamine     ZnCO3
Bronze (Sn)  -3200   Copper + Tin
Brass        -2000   Copper + Zinc         Sphalerite   ZnS
Mercury      -2000   Heat the sulfide      Cinnabar     HgS
Iron         -1200   Smelt with carbon     Hematite     Fe2O3
Arsenic       1250   Heat the sulfide      Orpiment     As2S3
Zinc          1300   Smelt with wool       Calamine     ZnCO3 (smithsonite) & Zn4Si2O7(OH)2·H2O (hemimorphite)
Antimony      1540   Smelt with iron       Stibnite     Sb2S3
Phosphorus    1669   Heat NaPO3 Excrement
Cobalt        1735   Smelt with carbon     Cobaltite    CoAsS
Platinum      1735   Naturally occuring
Nickel        1751   Smelt with carbon     Nickeline    NiAs
Bismuth       1753   Isolated from lead
Hydrogen      1766   Hot iron + steam      Water
Oxygen        1771   Heat HgO
Nitrogen      1772   Isolated from air
Manganese     1774   Smelt with carbon     Pyrolusite   MnO2
Molybdenum    1781   Smelt with carbon     Molybdenite  MoS2
Tungsten      1783   Smelt with carbon     Wolframite   (Fe,Mn)WO4
Chromium      1797   Smelt with carbon     Crocoite     PbCrO4
Palladium     1802   Isolated from Pt
Osmium        1803   Isolated from Pt
Iridium       1803   Isolated from Pt
Rhodium       1804   Isolated from Pt
Sodium        1807   Electrolysis
Potassium     1807   Electrolysis
Magnesium     1808   Electrolysis          Magnesia     MgCO3
Cadmium       1817   Isolated from zinc
Lithium       1821   Electrolysis of LiO2  Petalite     LiAlSi4O10
Zirconium     1824   Smelt with potassium  Zircon       ZrSiO4
Aluminum      1827   Smelt with potassium
Silicon       1823   Smelt with potassium
Beryllium     1828   Smelt with potassium  Beryl        Be3Al2Si6O18
Thorium       1929   Smelt with potassium  Gadolinite   (Ce,La,Nd,Y)2FeBe2Si2O10
Vanadium      1831   Smelt VCl2 with H2    Vanadinite   Pb5(VO4)3Cl
Uranium       1841   Smelt with potassium  Uranite      UO2
Ruthenium     1844   Isolated from Pt
Tantalum      1864   Smelt with hydrogen   Tantalite    [(Fe,Mn)Ta2O6]
Niobium       1864   Smelt with hydrogen   Tantalite    [(Fe,Mn)Ta2O6]
Fluorine      1886   Electrolysis
Helium        1895   From uranium ore
Titanium      1910   Smelt with sodium     Ilmenite     FeTiO3
Hafnium       1924   Isolated from zirconium
Rhenium       1928   Isolated from Pt
Scandium      1937   Electrolysis          Gadolinite   FeTiO3

History of mineralogy

 -384  -322   Aristotle. Wrote "Meteorology"
 -370  -285   Theophrastus. Wrote "De Mineralibus"
         77   Pliny the Elder publishes "Natural History"
  973  1050   Al Biruni. Published "Gems"
       1546   Georgius Agricola publishes "On the Nature of Rocks"
       1556   Georgius Agricola publishes "On Metals"
       1609   de Boodt publishes a catalog of minerals
       1669   Brand: Discovery of phosphorus
       1714   John Woodward publishes "Naturalis historia telluris illustrata & aucta", a mineral catalog
       1735   Brandt: Discovery of cobalt
       1777   Lavoisier: Discovery of sulfur
       1778   Lavoisier: Discovery of oxygen and prediction of silicon
       1783   Lavoisier: Discovery of hydrogen
       1784   T. Olof Bergman publishes "Manuel du mineralogiste, ou sciagraphie du regne mineral",
              and founds analytical chemistry
       1778   Lavoisier: Discovery of oxygen
       1801   Rene Just Huay publishes "Traite de Mineralogie", founding crystallography
       1811   Avogadro publishes "Avogadro's law"
       1860   The Karlsruhe Congress publishes a table of atomic weights
       1869   Mendeleev publishes the periodic table

Metals known since antiquity

For a metal, the stiffness is characterized by the "shear strength" and the sword worthiness is characterized by the shear strength over the density (the "strength to weight ratio"). For example for iron,

Shear modulus    =  S         =   82 GJoules/meter3
Density          =  D         = 7900 kg/meter3
Sword worthiness =  Q  = S/D  = 10.4 MJoules/kg

Metals

This plot includes all metals with a strength/density at least as large as lead, plus mercury. Beryllium is beyond the top of the plot.


Wootz steel

-600  Wootz steel developed in India and is renowned as the finest steel in the world.
1700  The technique for making Wootz steel is lost.
1790  Wootz steel begins to be studied by the British Royal Society.
1838  Anosov replicates Wootz steel.
Wootz steel is a mix of two phases: martensite (crystalline iron with .5% carbon), and cementite (iron carbide, Fe, 6.7% carbon).

Iron meteorites

In prehistoric times iron meteorites were the only source of metallic iron. They consist of 90% iron and 10% nickel.


Metal smelting

Prehistoric-style smelter

Most metals are in oxidized form. The only metals that can be found in pure form are gold, silver, copper, platinum, palladium, osmium, and iridium.

Smelting is a process for removing the oxygen to produce pure metal. The ore is heated in a coal furnace and the carbon seizes the oxygen from the metal. For copper,

Cu2O + C  →  2 Cu + CO
At low temperature copper stays in the form of Cu2O and at high temperature it gives the oxygen to carbon and becomes pure copper.

For iron, the oxidation state is reduced in 3 stages until the pure iron is left behind.

3 Fe2O3 + C  →  2 Fe3O4 + CO
Fe3O4   + C  →  3 FeO   + CO
FeO     + C  →    Fe   + CO
Oxidation state  =  Number of electrons each iron atom gives to oxygen

       Oxidation state
CuO          2
Cu2O         1
Cu           0
Fe2O3        3
Fe3O4       8/3
FeO          2
Fe           0

Smelting temperature

The following table gives the temperature required to smelt each element with carbon.

        Smelt  Method  Year  Abundance
         (C)                   (ppm)

Gold        <0   *   Ancient      .0031
Silver      <0   *   Ancient      .08
Platinum    <0   *    1735        .0037
Mercury     <0  heat -2000        .067
Palladium   <0  chem  1802        .0063
Copper      80   C   -5000      68
Sulfur     200   *   Ancient   420
Lead       350   C   -6500      10
Nickel     500   C    1751      90
Cadmium    500   C    1817        .15
Cobalt     525   ?    1735      30
Tin        725   C   -3200       2.2
Iron       750   C   -1000   63000
Phosphorus 750  heat  1669   10000
Tungsten   850   C    1783    1100
Potassium  850   e-   1807   15000
Zinc       975   C    1746      79
Sodium    1000   e-   1807   23000
Chromium  1250   C    1797     140
Niobium   1300   H    1864      17
Manganese 1450   C    1774    1120
Vanadium  1550   ?    1831     190
Silicon   1575   K    1823  270000
Titanium  1650   Na   1910   66000
Magnesium 1875   e-   1808   29000
Lithium   1900   e-   1821      17
Aluminum  2000   K    1827   82000
Uranium   2000   K    1841       1.8
Beryllium 2350   K    1828       1.9

Smelt:      Temperature required to smelt with carbon
Method:     Method used to purify the metal when it was first discovered
            *:  The element occurs in its pure form naturally
            C:  Smelt with carbon
            K:  Smelt with potassium
            Na: Smelt with sodium
            H:  Smelt with hydrogen
            e-: Electrolysis
            heat:  Heat causes the oxide to decompose into pure metal. No carbon required.
            chem:  Chemical separation
Discovery:  Year the element was first obtained in pure form
Abundance:  Abundance in the Earth's crust in parts per million
Elements with a low carbon smelting temperature were discovered in ancient times unless the element was rare. Cobalt was discovered in 1735, the first new metal since antiquity, and this inspired scientists to smelt every known mineral in the hope that it would yield a new metal. By 1800 all the rare elements that were carbon smeltable were discovered.

The farther to the right on the periodic table, the lower the smelting temperature, a consequence of "electronegativity".

The battery was invented in 1800, launching the field of electrochemistry and enabling the the isolation of non-carbon-smeltable elements. Davy used electrolysis in 1807 to isolate sodium and potassium and then he used these metals to smelt other metals. To smelt beryllium with potassium, BeO + 2 K ↔ Be + K2O.

Titanium can't be carbon smelted because it forms the carbide Ti3C.

Data

For an expanded discussion of smelting physics, see jaymaron.com/metallurgy.html.


Thermite

Thermite is smelting with aluminum. For example, to smelt iron with aluminum,

Fe2O3 + 2 Al  →  2 Fe + Al2O3

Smelting reactions

The following table shows reactions that change the oxidation state of a metal. "M" stands for an arbitrary metal and the magnitudes are scaled to one mole of O2. The last two columns give the oxidation state of the metal on the left and right side of the reaction. An oxidation state of "0" is the pure metal and "M2O" has an oxidation state of "1".

                            Oxidation state   Oxidation state
                                at left          at right
 2  M2O   ↔  4  M     + O2        1                0
 4  MO    ↔  2  M2O   + O2        2                1
 2  M3O4  ↔  6  MO    + O2       8/3               2
 6  M2O3  ↔  4  M3O4  + O2        3               8/3
 2  M2O3  ↔  4  MO    + O2        3                2
 2  MO    ↔  2  M     + O2        2                0
2/3 M2O3  ↔ 4/3 M     + O2        3                0
 1  MO2   ↔  1  M     + O2        4                0
 2  MO2   ↔  2  MO    + O2        4                2

Minerals

These elements are not necessarily on the Science Olympiad list.

We list minerals by element, with the most abundant mineral for each element listed first.

Lithium

Spodumene: LiAl(SiO3)2
Stilbite: LiAlSi2O6
Tourmaline: (Ca,Na,K,)(Li,Mg,Fe+2,Fe+3,Mn+2,Al,Cr+3,V+3)3(Mg,Al,Fe+3,V+3,Cr+3)6((Si,Al,B)6O18)(BO3)3(OH,O)3(OH,F,O)

Beryllium

Beryl: Be3Al2(SiO3)6
Morganite: Be3Al2(SiO3)6
Emerald

Carbon

Diamond: C

Sodium

Halite: NaCl

Magnesium

Periclase: MgO
Magnesite: MgCO3
Dolomite: CaMg(CO3)2
Peridot: (Mg,Fe)2SiO4
Spinel: MgAl2O4
Spinel: MgAl2O4

Aluminum

Bauxite: Al(OH)3 and AlO(OH)
Alumstone: KAl3(SO4)2(OH)6
Muscovite mica: KAl2(AlSi3O10)(F,OH)2 or KF2(Al2O3)3(SiO2)6(H2O)
Corundum: Al2O3
Topaz: Al2SiO4(F,OH)2

Epidote: Ca2(Al2,Fe)(SiO4)(Si2O7)O(OH)
Jadeite: NaAlSi2O6
Albite: NaAlSi3O8
Amazonite: KAlSi3O8
Labradorite: (Na,Ca)(Al,Si)4O8

Silicon

Amethyst: SiO2
Quartz: SiO2
Citrine: SiO2
Opal: SiO2·nH2O
Agate: SiO2

Sulfur

Volcanic sulfur

Calcium

Fluorite: CaF2
Calcite: CaCO3
Satin Spar: CaSO4 · 2H2O
Selenite: CaSO4 · 2H2O
Aragonite: CaCO3
Pearl: CaCO3
Calcite: CaCO3

Titanium, vanadium, chomium, and manganese

Rutile: TiO2
Vanadinite: Pb5(VO4)3Cl
Chromite: FeCr2O4
Pyrolusite: MnO2
Rhodonite: MnSiO3
Rhodochrosite: MnCO3

Iron

Hematite: Fe2O3
Hematite: Fe2O3
Pyrite: FeS2
Iron meteorite
Goethite: FeO(OH)

Cobalt and nickel

Cobaltite: CoAsS
Millerite: NiS

Copper

Chalcocite: Cu2S
Chalcopyrite: CuFeS2
Malachite: Cu2CO3(OH)l2
Azurite: Cu3(CO3)2(OH)2
Bornite: Cu5FeS4
Turquoise: CuAl6(PO4)4(OH)8•4(H2O)

Zinc and germanium

Sphalerite: ZnS
Germanite: Cu26Fe4Ge4S32

Strontium, zirconium, molybdenum

Celestine: SrSO4
Strontianite: SrCO3
Zircon: ZrSiO4
Molybdenite: MoS2

Silver

Argentite: Ag2S
Acanthite: Ag2S
Silver nugget

Tin

Cassiterite: SnO2

Caesium, barium, rare-earths

Pollucite: (Cs,Na)2Al2Si4O12·2H2O
Barite: BaSO4
Monazite: (Ce,La,Nd,Th)PO4

Tungsten

Wolframite: FeWO4
Scheelite: WCaO4
Hubnerite: WMnO4

Platinum, gold, mercury, lead

Sperrylite: PtAs2
Platinum nugget
Gold nugget
Cinnabar: HgS
Galena: PbS
Anglesite: PbSO4
Thorite: (Th,U)SiO4


Gems

Ruby
Diamond
Topaz
Zircon: ZrSiO4
Spinel: MgAl2O4

Sapphire
Sapphire
Sapphire

Emerald
Beryl: Be3Al2(SiO3)6
Morganite

Quartz
Amethyst: SiO2
Amethyst: SiO2
Citrine: SiO2

Garnet: [Mg,Fe,Mn]3Al2(SiO4)3 & Ca3[Cr,Al,Fe]2(SiO4)3
Peridot: (Mg,Fe)2SiO4
Opal: SiO2·nH2O
Jadeite: NaAlSi2O6
Pearl: CaCO3
Amber: Resin

Corundum is a crystalline form of aluminium oxide (Al2O3). It is transparent in its pure form and can have different colors when metal impurities are present.

             Color    Colorant  carat ($)

Painite                          55000  CaZrAl9O15(BO3)
Diamond      Clear                1400  C
Ruby         Red      Chromium   15000  Al2O3
Sapphire     Blue     Iron         650  Al2O3
Sapphire     yellow   Titanium          Al2O3
Sapphire     Orange   Copper            Al2O3
Sapphire     Green    Magnesium         Al2O3
Emerald      Green    Chromium          Be3Al2(SiO3)6
Beryl        Aqua     Iron              Be3Al2(SiO3)6   AKA "aquamarine"
Morganite    Orange   Manganese    300  Be3Al2(SiO3)6
Topaz        Topaz                      Al2SiO4(F,OH)2
Spinel       Red      Red               MgAl2O4
Quartz       Clear                      SiO2
Amethyst     Purple   Iron              SiO2
Citrine      Yellow                     SiO2
Zircon       Red                        ZrSiO4
Garnet       Orange                     [Mg,Fe,Mn]3Al2(SiO4)3 & Ca3[Cr,Al,Fe]2(SiO4)3
Garnet       Blue                 1500  [Mg,Fe,Mn]3Al2(SiO4)3 & Ca3[Cr,Al,Fe]2(SiO4)3
Opal                                    SiO2·nH2O
Opal         Black               11000  SiO2·nH2O
Jet          Black                      Lignite
Peridot      Green                      (Mg,Fe)2SiO4
Pearl        White                      CaCO3
Jade         Green                      NaAlSi2O6
Amber        Orange                     Resin

Crystals
Crystal, polycrystal, and amorphous

Diamond
Carbon phase diagram

Corundum (Al2O3)
Corundum unit cell
Corundum

Metal lattice
Salt (NaCl)
Tungsten Carbide

Alpha quartz (SiO2)
Beta quartz
Glass (SiO2)
Ice


Conductivity

White: High conductivity
Red:   Low conductivity

Electric and thermal conductivity
         Electric  Thermal  Density   Electric   C/Ct     Heat   Heat      Melt   $/kg  Young  Tensile Poisson  Brinell
         conduct   conduct            conduct/            cap    cap                                   number   hardness
        (e7 A/V/m) (W/K/m)  (g/cm^3)  Density   (AK/VW)  (J/g/K) (J/cm^3K)  (K)         (GPa)  (GPa)             (GPa)

Silver      6.30   429      10.49       .60      147       .235   2.47     1235    590    83   .17      .37      .024
Copper      5.96   401       8.96       .67      147       .385   3.21     1358      6   130   .21      .34      .87
Gold        4.52   318      19.30       .234     142       .129   2.49     1337  24000    78   .124     .44      .24
Aluminum    3.50   237       2.70      1.30      148       .897   2.42      933      2    70   .05      .35      .245
Beryllium   2.5    200       1.85      1.35      125      1.825   3.38     1560    850   287   .448     .032     .6
Magnesium   2.3    156       1.74      1.32      147      1.023   1.78      923      3    45   .22      .29      .26
Iridium     2.12   147      22.56       .094     144       .131   2.96     2917  13000   528  1.32      .26     1.67
Rhodium     2.0    150      12.41       .161     133       .243   3.02     2237  13000   275   .95      .26     1.1
Tungsten    1.89   173      19.25       .098     137       .132   2.54     3695     50   441  1.51      .28     2.57
Molybdenum  1.87   138      10.28       .182     136       .251            2896     24   330   .55      .31     1.5
Cobalt      1.7    100       8.90       .170               .421            1768     30   209   .76      .31      .7
Zinc        1.69   116       7.14                          .388             693      2   108   .2       .25      .41
Nickel      1.4     90.9     8.91                          .444            1728     15
Ruthenium   1.25   117      12.45                                          2607   5600
Cadmium     1.25    96.6     8.65                                           594      2    50   .078     .30      .20
Osmium      1.23    87.6    22.59                          .130            3306  12000
Indium      1.19    81.8     7.31                                           430    750    11   .004     .45      .009
Iron        1.0     80.4     7.87                          .449            1811          211   .35      .29      .49
Palladium    .95    71.8                                                   1828
Tin          .83    66.8                                                    505     22    47   .20      .36      .005
Chromium     .79    93.9                                   .449            2180
Platinum     .95                                           .133            2041
Tantalum     .76                                           .140            3290
Gallium      .74                                                            303
Thorium      .68
Niobium      .55    53.7                                                   2750
Rhenium      .52                                           .137            3459
Vanadium     .5     30.7                                                   2183
Uranium      .35
Titanium     .25    21.9                                   .523            1941
Scandium     .18    15.8                                                   1814
Neodymium    .156                                                          1297
Mercury      .10     8.30                                  .140             234
Manganese    .062    7.81                                                  1519
Germanium    .00019                                                        1211

Diamondiso 10     3320
Diamond     e-16  2200                                     .509
Nanotube   10     3500                                                Carbon nanotube. Electric conductivity = e-16 laterally
Tube bulk          200                                                Carbon nanotubes in bulk
Graphene   10     5000
Graphite    2      400                                     .709       Natural graphite
Al Nitride  e-11   180
Brass       1.5    120
Steel               45                                                Carbon steel
Bronze       .65    40
Steel Cr     .15    20                                                Stainless steel (usually 10% chromium)
Quartz (C)          12                                                Crystalline quartz.  Thermal conductivity is anisotropic
Quartz (F)  e-16     2                                                Fused quartz
Granite              2.5
Marble               2.2
Ice                  2
Concrete             1.5
Limestone            1.3
Soil                 1
Glass       e-12      .85
Water       e-4       .6
Seawater    1         .6
Brick                 .5
Plastic               .5
Wood                  .2
Wood (dry)            .1
Plexiglass  e-14      .18
Rubber      e-13      .16
Snow                  .15
Paper                 .05
Plastic foam          .03
Air        5e-15      .025
Nitrogen              .025                                1.04
Oxygen                .025                                 .92
Silica aerogel        .01

Siemens:    Amperes^2 Seconds^3 / kg / meters^2     =   1 Ohm^-1
For most metals,
Electric conductivity / Thermal conductivity  ~  140  J/g/K

Magnetic field magnitudes
                                     Teslas

Field generated by brain             10-12
Wire carrying 1 Amp                  .00002     1 cm from the wire
Earth magnetic field                 .0000305   at the equator
Neodymium magnet                    1.4
Magnetic resonance imaging machine  8
Large Hadron Collider magnets       8.3
Field for frog levitation          16
Strongest electromagnet            32.2         without using superconductors
Strongest electromagnet            45           using superconductors
Neutron star                       1010
Magnetar neutron star              1014

Dielectric strength

The critical electric field for electric breakdown for the following materials is:


              MVolt/meter
Air                3
Glass             12
Polystyrene       20
Rubber            20
Distilled water   68
Vacuum            30        Depends on electrode shape
Diamond         2000

Relative permittivity

Relative permittivity is the factor by which the electric field between charges is decreased relative to vacuum. Relative permittivity is dimensionless. Large permittivity is desirable for capacitors.

             Relative permittivity
Vacuum            1                   (Exact)
Air               1.00059
Polyethylene      2.5
Sapphire         10
Concrete         4.5
Glass          ~ 6
Rubber           7
Diamond        ~ 8
Graphite       ~12
Silicon         11.7
Water (0 C)     88
Water (20 C)    80
Water (100 C)   55
TiO2         ~ 150
SrTiO3         310
BaSrTiO3       500
Ba TiO3     ~ 5000
CaCuTiO3    250000

Magnetic permeability

A ferromagnetic material amplifies a magnetic field by a factor called the "relative permeability".

                Relative    Magnetic   Maximum    Critical
              permeability  moment     frequency  temperature
                                       (kHz)      (K)
Metglas 2714A    1000000                100               Rapidly-cooled metal
Iron              200000      2.2                 1043
Iron + nickel     100000                                  Mu-metal or permalloy
Cobalt + iron      18000
Nickel               600       .606                627
Cobalt               250      1.72                1388
Carbon steel         100
Neodymium magnet       1.05
Manganese              1.001
Air                    1.000
Superconductor         0
Dysprosium                   10.2                   88
Gadolinium                    7.63                 292
EuO                           6.8                   69
Y3Fe5O12                      5.0                  560
MnBi                          3.52                 630
MnAs                          3.4                  318
NiO + Fe                      2.4                  858
CrO2                          2.03                 386

Effect of temperature on conductivity

Resistivity in 10^-9 Ohm Meters

              293 K   300 K   500 K

Beryllium     35.6    37.6     99
Magnesium     43.9    45.1     78.6
Aluminum      26.5    27.33    49.9
Copper        16.78   17.25    30.9
Silver        15.87   16.29    28.7

Current density

Current density
Resistor

                  Electric quantities             |                Thermal quantities
                                                  |
Q  =  Charge                 Coulomb              |   Etherm=  Thermal energy          Joule
I  =  Current                Amperes              |   Itherm=  Thermal current         Watts
E  =  Electric field         Volts/meter          |   Etherm=  Thermal field           Kelvins/meter
C  =  Electric conductivity  Amperes/Volt/meter   |   Ctherm=  Thermal conductivity    Watts/meter/Kelvin
A  =  Area                   meter^2              |   A     =  Area                    meter^2
Z  =  Distance               meter                |   Z     =  Distance                meter^2
J  =  Current flux           Amperes/meter^2      |   Jtherm=  Thermal flux            Watts/meter^2
   =  I / A                                       |         =  Ittherm / A
   =  C * E                                       |         =  Ctherm * Etherm
V  =  Voltage                Volts                |   Temp  =  Temperature difference  Kelvin
   =  E Z                                         |         =  Etherm Z
   =  I R                                         |         =  Itherm Rtherm
R  =  Resistance             Volts/Ampere = Ohms  |   Rtherm=  Thermal resistance      Kelvins/Watt
   =  Z / (A C)                                   |         =  Z / (A Ct)
H  =  Current heating        Watts/meter^3        |
   =  E J                                         |
P  =  Current heating power  Watts                |
   =  E J Z A                                     |
   =  V I                                         |

Continuum
Continuum quantity       Macroscopic quantity

     E             <->      V
     C             <->      R = L / (A C)
     J = C E       <->      I = V / R
     H = E J       <->      P = V I

Superconductors

                 Critical    Critical  Type
                temperature  field
                 (Kelvin)    (Teslas)

Magnesium-Boron2     39        55       2   MRI machines
Niobium3-Germanium   23.2      37       2   Field for thin films.  Not widely used
Magnesium-Boron2-C   34        36           Doped with 5% carbon
Niobium3-Tin         18.3      30       2   High-performance magnets.  Brittle
Vanadium3-Gallium    14.2      19       2
Niobium-Titanium     10        15       2   Cheaper than Niobium3-Tin.  Ductile
Niobium3-Aluminum

Technetium           11.2               2
Niobium               9.26       .82    2
Vanadium              5.03      1       2
Tantalum              4.48       .09    1
Lead                  7.19       .08    1
Lanthanum             6.3               1
Mercury               4.15       .04    1
Tungsten              4                 1    Not BCS
Tin                   3.72       .03    1
Indium                3.4        .028
Rhenium               2.4        .03    1
Thallium              2.4        .018
Thallium              2.39       .02    1
Aluminum              1.2        .01    1
Gallium               1.1
Gadolinium            1.1
Protactinium          1.4
Thorium               1.4
Thallium              2.4
Molybdenum             .92
Zinc                   .85       .0054
Osmium                 .7
Zirconium              .55
Cadmium                .52       .0028
Ruthenium              .5
Titanium               .4        .0056
Iridium                .1
Lutetium               .1
Hafnium                .1
Uranium                .2
Beryllium              .026
Tungsten               .015

HgBa2Ca2Cu3O8       134                 2
HgBa2Ca Cu2O6       128                 2
YBa2Cu3O7            92                 2
C60Cs2Rb             33                 2
C60Rb                28         2       2
C60K3                19.8        .013   2
C6Ca                 11.5        .95    2    Not BCS
Diamond:B            11.4       4       2    Diamond doped with boron
In2O3                 3.3       3       2
The critical fields for Niobium-Titanium, Niobium3-Tin, and Vanadium3-Gallium are for 4.2 Kelvin.

All superconductors are described by the BCS theory unless stated otherwise.

         Boiling point (Kelvin)

Water      273
Ammonia    248
Freon R12  243
Freon R22  231
Propane    230
Acetylene  189
Ethane     185
Xenon      165.1
Krypton    119.7
Oxygen      90.2
Argon       87.3
Nitrogen    77.4     Threshold for cheap superconductivity
Neon        27.1
Hydrogen    20.3     Cheap MRI machines
Helium-4     4.23    High-performance magnets
Helium-3     3.19
The record for Niobium3-Tin is 2643 Amps/mm^2 at 12 T and 4.2 K.

Titan has a temperature of 94 Kelvin, allowing for superconducting equipment. The temperature of Mars is too high at 210 Kelvin.


Gases

Ideal gas law

Molecules in a gas
Brownian motion

Pressure                          =  P             (Pascals or Newtons/meter2 or Joules/meter3)
Temperature                       =  T             (Kelvin)
Volume                            =  Vol           (meters3)
Total gas kinetic energy          =  E             (Joules)
Kinetic energy per volume         =  e  =  E/Vol   (Joules/meter3)
Number of gas molecules           =  N
Mass of a gas molecule            =  M
Gas molecules per volume          =  n  =   N / Vol
Gas density                       =  D  = N M / Vol
Avogadro number                   =  Avo=  6.022⋅1023  moles-1
Moles of gas molecules            =  Mol=  N / Avo
Boltzmann constant                =  k  =  1.38⋅10-23 Joules/Kelvin
Gas constant                      =  R  =  k Avo  =  8.31 Joules/Kelvin/mole
Gas molecule thermal speed        =  Vth
Mean kinetic energy / gas molecule=  ε  =  E / n  =  ½ M Vth2     (Definition of the mean thermal speed)
Gas pressure arises from the kinetic energy of gas molecules and has units of energy/volume.
The ideal gas law can be written in the following forms:
P  =  23 e                    Form used in physics
   =  R Mol T / Vol            Form used in chemistry
   =  k N   T / Vol
   =  13 N M Vth2/ Vol
   =  13 D Vth2
   =  k T D / M
Gas simulation at phet.colorado.edu
Derivation of the ideal gas law
History

Boyle's law
Charles' law

1660  Boyle law          P Vol     = Constant          at fixed T
1802  Charles law        T Vol     = Constant          at fixed P
1802  Gay-Lussac law     T P       = Constant          at fixed Vol
1811  Avogadro law       Vol / N   = Constant          at fixed T and P
1834  Clapeyron law      P Vol / T = Constant          combined ideal gas law

Boltzmann constant

For a system in thermodynamic equilibrium each degree of freedom has a mean energy of ½ k T. This is the definition of temperature.

Molecule mass                =  M
Thermal speed                =  Vth
Boltzmann constant           =  k  =  1.38⋅10-23 Joules/Kelvin
Molecule mean kinetic energy =  ε
A gas molecule moving in N dimensions has N degrees of freedom. In 3D the mean energy of a gas molecule is
ε  =  32 k T  =  ½ M V2th

Speed of sound

The sound speed is proportional to the thermal speed of gas molecules. The thermal speed of a gas molecule is defined in terms of the mean energy per molecule.

Adiabatic constant  =  γ
                    =  5/3 for monatomic molecules such as helium, neon, krypton, argon, and xenon
                    =  7/5 for diatomic molecules such as H2, O2, and N2
                    =  7/5 for air, which is 21% O2, 78% N2, and 1% Ar
                    ≈  1.31 for a triatomic gas such as CO2
Pressure            =  P
Density             =  D
Sound speed         =  Vsound
Mean thermal speed  =  Vth
K.E. per molecule   =  ε  =  ½ M Vth2

V2sound  =  γ  P / D  =  13  γ  V2th
The sound speed depends on temperature and not on density or pressure.

For air, γ = 7/5 and

Vsound  =  .68  Vth
These laws are derived in the appendix.

We can change the sound speed by using a gas with a different value of M.

                   M in atomic mass units

Helium atom                4
Neon atom                 20
Nitrogen molecule         28
Oxygen molecule           32
Argon atom                40
Krypton atom              84
Xenon atom               131
A helium atom has a smaller mass than a nitrogen molecule and hence has a higher sound speed. This is why the pitch of your voice increases if you inhale helium. Inhaling xenon makes you sound like Darth Vader. Then you pass out because Xenon is an anaesthetic.

In a gas, some of the energy is in motion of the molecule and some is in rotations and vibrations. This determines the adiabatic constant.

Ethane
Molecule with thermal vibrations


History of the speed of sound
1635  Gassendi measures the speed of sound to be 478 m/s with 25% error.
1660  Viviani and Borelli produce the first accurate measurement of the speed of
      sound, giving a value of 350 m/s.
1660  Hooke's law published.  The force on a spring is proportional to the change
      in length.
1662  Boyle discovers that for air at fixed temperature,
      Pressure * Volume = Constant
1687  Newton publishes the Principia Mathematica, which contains the first analytic
      calculation of the speed of sound.  The calculated value was 290 m/s.
Newton's calculation was correct if one assumes that a gas behaves like Boyle's law and Hooke's law.

The fact that Newton's calculation differed from the measured speed is due to the fact that air consists of diatomic molecules (nitrogen and oxygen). This was the first solid clue for the existence of atoms, and it also contained a clue for quantum mechanics.

In Newton's time it was not known that changing the volume of a gas changes its temperature, which modifies the relationship between density and pressure. This was discovered by Charles in 1802 (Charles' law).


Gas data
       Melt   Boil  Solid    Liquid   Gas      Mass   Sound speed
       (K)    (K)   density  density  density  (AMU)  at 20 C
                    g/cm3    g/cm3    g/cm3            (m/s)

He        .95   4.2            .125   .000179    4.00  1007
Ne      24.6   27.1           1.21    .000900   20.18
Ar      83.8   87.3           1.40    .00178    39.95   319
Kr     115.8  119.9           2.41    .00375    83.80   221
Xe     161.4  165.1           2.94    .00589   131.29   178
H2      14     20              .070   .000090    2.02  1270
N2      63     77              .81    .00125    28.01   349
O2      54     90             1.14    .00143    32.00   326
Air                                   .0013     29.2    344     79% N2, 21% O2, 1% Ar
H2O    273    373     .917    1.00    .00080    18.02
CO2    n/a    195    1.56      n/a    .00198    44.00   267
CH4     91    112              .42    .00070    16.04   446
CH5OH  159    352              .79    .00152    34.07           Alcohol
Gas density is for 0 Celsius and 1 Bar. Liquid density is for the boiling point, except for water, which is for 4 Celsius.

Carbon dioxide doesn't have a liquid state at standard temperature and pressure. It sublimes directly from a solid to a vapor.


Height of an atmosphere

M  =  Mass of a gas molecule
V  =  Thermal speed
E  =  Mean energy of a gas molecule
   =  1/2 M V^2
H  =  Characteristic height of an atmosphere
g  =  Gravitational acceleration
Suppose a molecule at the surface of the Earth is moving upward with speed V and suppose it doesn't collide with other air molecules. It will reach a height of
M H g  =  1/2  M  V^2
This height H is the characteristic height of an atmosphere.
Pressure of air at sea level      =  1   Bar
Pressure of air in Denver         = .85  Bar      One mile high
Pressure of air at Mount Everest  = 1/4  Bar      10 km high
The density of the atmosphere scales as
Density ~ (Density At Sea Level) * exp(-E/E0)
where E is the gravitational potential energy of a gas molecule and E0 is the characteristic thermal energy given by
E0 = M H g = 1/2 M V^2
Expressed in terms of altitude h,
Density ~ Density At Sea Level * exp(-h/H)
For oxygen,
E0  =  3/2 * Boltzmann_Constant * Temperature
E0 is the same for all molecules regardless of mass, and H depends on the molecule's mass. H scales as
H  ~  Mass^-1

Atmospheric escape
S = Escape speed
T = Temperature
B = Boltzmann constant
  = 1.38e-23 Joules/Kelvin
g = Planet gravity at the surface

M = Mass of heavy molecule                    m = Mass of light molecule
V = Thermal speed of heavy molecule           v = Thermal speed of light molecule
E = Mean energy of heavy molecule             e = Mean energy of light molecule
H = Characteristic height of heavy molecule   h = Characteristic height of light molecule
  = E / (M g)                                   = e / (m g)
Z = Energy of heavy molecule / escape energy  z = Energy of light molecule / escape energy
  = .5 M V^2 / .5 M S^2                         = .5 m v^2 / .5 m S^2
  = V^2 / S^2                                   = v^2 / S^2


For an ideal gas, all molecules have the same mean kinetic energy.

    E     =     e      =  1.5 B T

.5 M V^2  =  .5 m v^2  =  1.5 B T
The light molecules tend to move faster than the heavy ones. This is why your voice increases in pitch when you breathe helium. Breathing a heavy gas such as Xenon makes you sound like Darth Vader.

For an object to have an atmosphere, the thermal energy must be much less than the escape energy.

V^2 << S^2        <->        Z << 1


          Escape  Atmos    Temp    H2     N2      Z        Z
          speed   density  (K)    km/s   km/s    (H2)     (N2)
          km/s    (kg/m^3)
Jupiter   59.5             112   1.18    .45   .00039   .000056
Saturn    35.5              84   1.02    .39   .00083   .00012
Neptune   23.5              55    .83    .31   .0012    .00018
Uranus    21.3              53    .81    .31   .0014    .00021
Earth     11.2     1.2     287   1.89    .71   .028     .0041
Venus     10.4    67       735   3.02   1.14   .084     .012
Mars       5.03     .020   210   1.61    .61   .103     .015
Titan      2.64    5.3      94   1.08    .41   .167     .024
Europa     2.02    0       102   1.12    .42   .31      .044
Moon       2.38    0       390   2.20    .83   .85      .12
Ceres       .51    0       168   1.44    .55  8.0      1.14
Even if an object has enough gravity to capture an atmosphere, it can still lose it to the solar wind. Also, the upper atmosphere tends to be hotter than at the surface, increasing the loss rate.

The threshold for capturing an atmosphere appears to be around Z = 1/25, or

Thermal Speed  <  1/5 Escape speed

Heating by gravitational collapse

When an object collapses by gravity, its temperature increases such that

Thermal speed of molecules  ~  Escape speed
In the gas simulation at phet.colorado.edu, you can move the wall and watch the gas change temperature.

For an ideal gas,

3 * Boltzmann_Constant * Temperature  ~  MassOfMolecules * Escape_Speed^2
For the sun, what is the temperature of a proton moving at the escape speed? This sets the scale of the temperature of the core of the sun. The minimum temperature for hydrogen fusion is 4 million Kelvin.

The Earth's core is composed chiefly of iron. What is the temperature of an iron atom moving at the Earth's escape speed?

      Escape speed (km/s)   Core composition
Sun        618.             Protons, electrons, helium
Earth       11.2            Iron
Mars         5.03           Iron
Moon         2.38           Iron
Ceres         .51           Iron

Derivation of the ideal gas law

We first derive the law for a 1D gas and then extend it to 3D.

Suppose a gas molecule bounces back and forth between two walls separated by a distance L.

M  = Mass of molecule
V  = Speed of the molecule
L  = Space between the walls
With each collision, the momentum change = 2 M V

Time between collisions = 2 L / V

The average force on a wall is

Force  =  Change in momentum  /  Time between collisions  =  M  V^2  /  L
Suppose a gas molecule is in a cube of volume L^3 and a molecule bounces back and forth between two opposite walls (never touching the other four walls). The pressure on these walls is
Pressure  =  Force  /  Area
          =  M  V^2  /  L^3
          =  M  V^2  /  Volume

Pressure * Volume  =  M  V^2
This is the ideal gas law in one dimension. For a molecule moving in 3D,
Velocity^2  = (Velocity in X direction)^2
            + (Velocity in Y direction)^2
            + (Velocity in Z direction)^2

Characteristic thermal speed in 3D  =  3  *  Characteristic thermal speed in 1D.
To produce the 3D ideal gas law, replace V^2 with 1/3 V^2 in the 1D equation.
Pressure * Volume  =  1/3  M  V^2        Where V is the characteristic thermal speed of the gas
This is the pressure for a gas with one molecule. If there are n molecules,
Pressure  Volume  =  n  1/3  M  V^2            Ideal gas law in 3D
If a gas consists of molecules with a mix of speeds, the thermal speed is defined as
Kinetic dnergy density of gas molecules  =  E  =  (n / Volume) 1/2 M V^2
Using this, the ideal gas law can be written as
Pressure  =  2/3  E
          =  1/3  Density  V^2
          =  8.3  Moles  Temperature  /  Volume
The last form comes from the law of thermodynamics:
M V^2 = 3 B T

Virial theorem

A typical globular cluster consists of millions of stars. If you measure the total gravitational and kinetic energy of the stars, you will find that

Total gravitational energy  =  -2 * Total kinetic energy
just like for a single satellite on a circular orbit.

Suppose a system consists of a set of objects interacting by a potential. If the system has reached a long-term equilibrium then the above statement about energies is true, no matter how chaotic the orbits of the objects. This is the "Virial theorem". It also applies if additional forces are involved. For example, the protons in the sun interact by both gravity and collisions and the virial theorem holds.

Gravitational energy of the sun  =  -2 * Kinetic energy of protons in the sun

Newton's calculation for the speed of sound

Hooke's law for a spring
Wave in a continuum
Gas molecules


Because of Hooke's law, springs oscillate with a constant frequency.

X = Displacement of a spring
V = Velocity of the spring
A = Acceleration of the spring
F = Force on the spring
M = Spring mass
Q = Spring constant
q = (K/M)^(1/2)
t = time
T = Spring oscillation period
Hooke's law and Newton's law:
F  =  - Q X  =  M A

A  =  - (Q/M) X  =  - q^2 X
This equation is solved with
X  =      sin(q t)
V  =  q   cos(q t)
A  = -q^2 sin(q t)  =  - q^2 X
The oscillation period of the spring is
T  =  2 Pi / q
   =  2 Pi (M/Q)^(1/2)

According to Boyle's law, a gas functions like a spring and hence a gas oscillates like a spring. An oscillation in a gas is a sound wave.

For a gas,

P   =  Pressure
dP  =  Change in pressure
Vol =  Volume
dVol=  Change in volume
If you change the volume of a gas according to Boyle's law,
P Vol            =  Constant
P dVol + Vol dP  =  0

dP = - (P/Vol) dVol
The change in pressure is proportional to the change in volume. This is equivalent to Hooke's law, where pressure takes the role of force and the change in volume takes the role of displacement of the spring. This is the mechanism behind sound waves.


In Boyle's law, the change in volume is assumed to be slow so the gas has time to equilibrate temperature with its surroundings. In this case the temperature is constant as the volume changes and the change is "isothermal".

P Vol = Constant
If the change in volume is fast then the walls do work on the molecules, changing their temperature. If there isn't enough time to equilibrate temperature with the surroundings then the change is "adiabatic". You can see this in action with the "Gas" simulation at phet.colorado.edu. Moving the wall changes the thermal speed of molecules and hence the temperature.


If a gas consists of pointlike particles then

Vol =  Volume of the gas
Ek  =  Total kinetic energy of gas molecules within the volume
E   =  Total energy of gas molecules within the volume
    =  Kinetic energy plus the energy from molecular rotation and vibration
dE  =  Change in energy as the volume changes
P   =  Pressure
dP  =  Change in pressure as the volume changes
D   =  Density
C   =  Speed of sound in the gas
d   =  Number of degrees of freedom of a gas molecule
    =  3 for a monotomic gas such as Helium
    =  5 for a diatomic gas such as nitrogen
G   =  Adiabatic constant
    =  1 + 2/d
    =  5/3 for a monatomic gas
    =  7/5 for a diatomic gas
k   =  Boltzmann constant
T   =  Temperature
The ideal gas law is
P Vol =  (2/3) Ek                    (Derived in www.jaymaron.com/gas/gas.html)
This law is equivalent to the formula that appears in chemistry.
P Vol = Moles R T
For a gas in thermal equilibrium each degree of freedom has a mean energy of .5 k T. For a gas of pointlike particles (monotomic) there are three degrees of freedom, one each for motion in the X, Y, and Z direction. In this case d=3. The mean kinetic energy of each gas molecule is 3 * (.5 k T). The total mean energy of each gas molecule is also 3 * (.5 k T).

For a diatomic gas there are also two rotational degrees of freedom. In this case d=5.

In general,

Ek  =  3 * (.5 k T)
E   =  d * (.5 k T)

Ek  =  (3/d) E
If you change the volume of a gas adiabatically, the walls change the kinetic and rotational energy of the gas molecules.
dE  =  -P dVol
The ideal gas law in terms of E instead of Ek is
P Vol =  (2/d) E

dP  =  (2/d) (dE/Vol - E dVol/Vol^2)
    =  (2/d) [-P dVol/Vol - (d/2) P dVol/Vol]
    = -(1+2/d) P dVol/Vol
    = - G P dVol/Vol
This equation determines the speed of sound in a gas.
C^2  =  G P / D
For air,
P = 1.01e5 Newtons/meter^2
D = 1.2    kg/meter^3
Newton assumed G=1 from Boyle's law, yielding a sound speed of
C  =  290 m/s
The correct value for air is G=7/5, which gives a sound speed of
C = 343 m/s
which is in accord with the measurement.


For a gas, G can be measured by measuring the sound speed. The results are

Helium     5/3    Monatomic molecule
Argon      5/3    Monatonic molecule
Air        7/5    4/5 Nitrogen and 1/5 Oxygen
Oxygen     7/5    Diatomic molecule
Nitrogen   7/5    Diatomic molecule
The fact that G is not equal to 1 was the first solid evidence for the existence of atoms and it also contained a clue for quantum mechanics. If a gas is a continuum (like Hooke's law) it has G=1 and if it consists of pointlike particles (monatonic) it has G=5/3. This explains helium and argon but not nitrogen and oxygen. Nitrogen and oxygen are diatomic molecules and their rotational degrees of freedom change Gamma.
                             Kinetic degrees   Rotational degrees    Gamma
                                of freedom         of freedom
Monatonic gas                      3                  0               5/3
Diatomic gas  T < 1000 K           3                  2               7/5
Diatomic gas, T > 1000 K           3                  3               4/3
Quantum mechanics freezes out one of the rotation modes at low temperature. Without quantum mechanics, diatomic molecules would have Gamma=4/3 at room temperature.

The fact that Gamma=7/5 for air was a clue for the existence of both atoms, molecules, and quantum mechanics.


Dark energy

For dark energy,

E  =  Energy
dE =  Change in energy
e  =  Energy density
Vol=  Volume
P  =  Pressure
The volume expands as the universe expands.

As a substance expands it does work on its surroundings according to its pressure.

dE = - P dVol
For dark energy, the energy density "e" is constant in space and so
dE = e dVol
Hence,
P = - e
Dark energy has a negative pressure, which means that it behaves differently from a continuum and from particles.

Dark matter consists of pointlike particles but they rarely interact with other particles and so they exert no pressure.


Valyrian steel

"Ice" is the sword with the red handle

Valyrian steel is a fictional substance from "Game of Thrones" that is stronger, lighter, and harder than steel. The only elements that qualify are beryllium, titanium, and vanadium, none of which were known in Earth history until the 18th century. Valyrian steel could be of these elements, an alloy, or a magical substance. According to George Martin, magic is involved.

The fact that it is less dense than steel means that it can't be a fancy form of steel such as Damascus steel or Wootz steel. Also, fancy steel loses its special properties if melted and hence cannot be reforged, whereas Valyrian steel swords can be reforged.

In Earth history, the first metal discovered since iron was cobalt in 1735. This launched a frenzy to smelt all known minerals and most of the smeltable metals were discovered by 1800. Then the battery and electrochemstry were discovered in 1800 and these were used to obtain the unsmeltable metals, which are lithium, beryllium, magnesium, aluminum, titanium, vanadium, niobium, and Uranium. Almost all of the strong alloys use these metals, and so the Valyrians must have used either electrochemistry or magic to make Valyrian steel.


Candidates for Valyrian steel

The following metals and alloys are both stronger and lighter than steel and could hypothetically be Valyrian steel.

                Yield     Density  Strength/Density
                strength  (g/cm3)   (GJoule/kg)
                (GPascal)
Beryllium            .34     1.85     .186
Aluminum + Be        .41     2.27     .181
LiMgAlScTi          1.97     2.67     .738
Titanium             .22     4.51     .050
Titanium + AlVCrMo  1.20     4.6      .261
Vanadium             .53     6.0      .076
AlCrFeCoNiTi        2.26     6.5      .377
AlCrFeCoNiMo        2.76     7.1      .394
Steel                .25     7.9      .032     Iron plus carbon
Copper               .12     9.0      .013
"Yield strength" is the maximum pressure a material can sustain before deforming. "Strength/Density" is the strength-to-weight ratio. Steel is stronger and lighter than copper.
Lore

Petyr Baelish: Nothing holds an edge like Valyrian steel.

Tyrion Lannister: Valyrian steel blades were scarce and costly, yet thousands remained in the world, perhaps two hundred in the Seven Kingdoms alone.

George Martin: Valyrian steel is a fantasy metal. Which means it has magical characteristics, and magic plays a role in its forging.

George Martin: Valyrian steel was always costly, but it became considerably more so when there was no more Valyria, and the secret of its making were lost.

Ned Stark's stord "Ice" is melted down and reforged into two smaller swords, "Oathkeeper" and "Widow's Wail". This rules out Valyrian steel being Wootz steel because Wootz steel loses its special properties when reforged.

Appearances of Valyrian steel in Game of Thrones:

        Name          Owner

Sword   Longclaw      Jon Snow
Sword   Heartsbane    Samwell Tarly
Dagger                Arya
Sword   Ice           Eddard Stark         Reforged into Oathkeeper and Widow's Wail
Sword   Oathkeeper    Brienne of Tarth
Sword   Widow's Wail  The Crown
Sword   Lady Forlorn  Ser Lyn Corbray
Sword   Nightfall     Ser Harras Harlow
Sword   Red Rain      Lord Dunstan Drumm
Arakh                 Caggo
Armor                 Euron Greyjoy
Horn    Dragonbinder  The Citadel of The Maesters
Some Maesters carry links of Valyrian steel, a symbol of mastery of the highest arts.
Black materials

Vantablack is the blackest known substance, composed of carbon nanotubes and invented in 2014. "Vanta" stands for Vertically Aligned Nano tube Arrays.

               Reflectivity
Black paint       .025
Super black       .004        Nickel-phosphorus alloy
Vantablack        .00035      Carbon nanotubes

Viscosity

Viscosity is analogous to electrical conductivity and thermal conductivity.

Quantity                    Electricity            Thermal               Viscosity

Stuff                       Coulomb                Joule                 Momentum
Stuff/volume                Coulomb/m^3            Joule/m^3             Momentum/m^3
Flow = Stuff/time           Coulomb/second         Joule/s               Momentum/s
Potential                   Volts                  Kelvin                Momentum/m^3
Field                       Volts/meter            Kelvins/meter         Momentum/m^3/m
Flow density = Flow/m^2     Amperes/meter^2        Watts/meter^2         Momentum/s/m^2
Conductivity                Amperes/Volt/meter     Watts/meter/Kelvin    m^2/s
Resistance                  Volts/Ampere           Kelvins/Watt          s/m^3


Flow density  =  Conductivity  *  Field

Flow          =  Potential  /  Resistance

Field         =  -Gradient(Potential)

Kinematic and dynamic viscosity
Fluid density          =  ρ              (kg/meter3)
Fluid velocity         =  V
Fluid momentum density =  U  =  D V
Kinematic viscosity    =  νk             (meters2 / second)
Dynamic viscosity      =  νd  =  ρ νk    (Pascal seconds)
Lagrangian time deriv. =  Dt

Dt U =  ∇⋅(νd∇U)
Dt V =  ∇⋅(νk∇V)

Viscosity
               Dynamic       Kinematic  Density
               viscosity     viscosity  (kg/m3)
                 (Pa s)      (m2/s)
Hydrogen            .00000876
Nitrogen            .0000178
Air                 .0000183  .0000150     1.22
Helium              .000019
Oxygen              .0000202
Xenon               .0000212
Acetone             .00031
Benzine             .00061
Water at   2 C      .00167
Water at  10 C      .00131    .0000010  1000
Water at  20 C      .00100              1000
Water at  30 C      .000798             1000
Water at 100 C      .000282             1000
Mercury             .00153    .00000012
Blood               .0035
Motor oil           .065
Olive oil           .081
Honey              6
Peanut butter    250
Asthenosphere   7e19         Weak layer between the curst and mantle
Upper mantle   .8e21
Lower mantle  1.5e21
1 Stokes = 1 cm2/s = 10-4 m2/s
Fluid mechanics
Schmidt number           = Momentum diffusivity / Mass diffusivity
Prandtl number           = Momentum diffusivity / Thermal diffusivity
Magnetic Prandtl number  = Momentum diffusivity / Magnetic diffusivity

                Prandtl   Schmidt
Air                .7       .7
Water             7
Liquid metals  << 1
Oils           >> 1

Plasma physics
n       =  Electron density
M       =  Electron mass
V       =  Electron thermal velocity
Q       =  Proton charge
k       =  Boltzmann constant
Temp    =  Temperature
Xdebye  =  Debye length                   (k*Temp/n/Q^2/(4 Pi Ke))^.5
Xgyro   =  Electron gyro radius           M V / Q B
Fgyro   =  Electron gyrofrequency


               Electron  Temp  Debye   Magnetic
               density   (K)    (m)    field (T)
               (m^-3)
Solar core       e32     e7    e-11    -
ITER          1.0e20     e8    e-4     5.3
Laser fusion  6.0e32     e8            -    National Ignition Facility.  density=1000 g/cm^3
Gas discharge    e16     e4    e-4     -
Ionosphere       e12     e3    e-3    e-5
Magnetosphere    e7      e7    e2     e-8
Solar wind       e6      e5    e1     e-9
Interstellar     e5      e4    e1     e-10
Intergalactic    e0      e6    e5      -


ITER ion temperature      = 8.0 keV
ITER electron temperature = 8.8 keV
ITER confinement time     = 400 seconds

Inertial confinement fusion
                                 Compression  Heating     Fusion   Heating  Density    Year
                                 laser (MJ)   laser (MJ)  energy   time     (kg/m^3)
                                                          (MJ)     (s)
NOVA                                                                          .3    1984.  LLNL
National Ignition Facility (NIF)   330           -          20                .9       2010
HiPER                                 .2        .07         30      e-11      .3       Future

Strings


Characteristic string tension

For a given instrument there is a characteristic ideal tension for the strings. If the tension is too low or high the string becomes unplayable. The tension can be varied to suit the performer's taste but it can't be changed by an extreme degree.


           String                      Height of   Height of        String  String
           length   Tension (Newtons)  top string  bottom string    length  length
             mm     E   A   D   G   C     mm         mm              inch  violin=1

Violin      320    80  50  45  45         3.2        5.2             12.6    1
Viola       388        65  55  55  55     4.8        6.2             15.3    1.21
Cello       690       160 130 130 130     5.2        8.2             27.2    2.2
Bass       1060       160 160 160 160                                41.3    3.3
Guitar      650       120 120 120 120                                25.6    2.0
Bass guitar 860       160 160 160 160                                33.6    2.7

The height of the string is the distance from the fingerboard, at the end of the fingerboard.


Waves on a string

The frequency of a string and the speed of a wave on the string are related by:

                                              Values for a violin A-string

L  =  Length of a string                   =  .32 meters
F  =  Vibration frequency of the string    =  440 Hertz
V  =  Speed of a wave on the string        =  281.6 meters/second
   =  2 F L
For a given instrument and string frequency, the wavespeed is fixed.

The speed of a wave on a string is

WaveSpeed^2  =  Tension / (Density * Pi * Radius^2)
The variables you can vary for a string are {Tension, Density, Radius}. Once you have chosen the frequency and length of the string then these variables are related by
Tension = Constant * Density * Radius^2

The larger the radius the more difficult the string is to play and the more impure the overtones. The radius can be minimized by using a material with a high density. This is why cello, bass, and bass guitar strings are often made of tungsten.

High-density strings are only appropriate for low-frequency strings because they have a low wavespeed. High-frequency strings require a material with low density.

String manufacturers almost never state the density and radius of the string. You can infer the density from the type of metal used, with numbers given the table below.

The speed of sound in air has an analogous form as the speed of a wave on a string.

SoundSpeed^2  =  (7/5) Pressure / Density

String tensile strength

If the tension force on a string exceeds the "Tensile strength" then the string breaks.

Force  =  Force on the string
A      =  Area of the string
S      =  Stress on the string
       =  Force / A
Smax   =  Tensile strength
       =  Maximum string stress before breaking
Z      =  Strength to weight ratio
Z      =  Smax / Density


                 Tensile   Density   Z/10^6   Young's
                 strength                     modulus
                   (GPa)   (g/cm^3)  (J/kg)   (GPa)

Carbon nanotube    7          .116   60.3              Technology not yet developed
Nylon               .045     1.15      .04      5
Kevlar             3.6       1.44     2.5
Zylon              5.8       1.5      3.9
Gut                 .2       1.5       .13      6
Magnesium alloy     .4       1.8       .22
Aluminum            .05      2.7
Titanium alloy      .94      4.5       .21
Nickel              .20      8.9
Chromium            .28      7.2
Steel alloy        2.0       7.9       .25    220
Brass               .55      8.7
Silver              .17     10.5
Tungsten            .55     19.2       .029
Gold                .13     19.3
Osmium             1.0      22.6
Iridium

Maximum frequency of a string

F    =  String frequency
R    =  String radius
A    =  String cross-sectional area
     =  Pi R^2
D    =  String density
L    =  String length
Force=  String tension force (Newtons)
S    =  Tensile stress (Pascals)
     =  Force / A
Smax =  Maximum string tensile stress before breaking
     =  Tensile strength
V    =  Speed of a wave on the string
     =  SquareRoot(P/D)
Z    =  String strength-to-weight ratio
     =  S/D
Fmax =  Maximum frequency of a string
The maximum frequency of a string happens when S=Smax.
Fmax  =  V / (2L)
      =  SquareRoot(Smax/D) / (2L)
      =  SquareRoot(Z) / (2L)
The maximum frequency of a string depends on the strength-to-weight ratio Z. Values for Z for various string materials are given in the table above. Steel alloy is often used for the highest-frequency strings on a violin or piano.

A space elevator requires a material with Z > 100.


Maximum frequency of a string for various materials
            Gut   Steel   Zylon   Carbon    Tungsten
                                 nanotube

Violin      563    781    2960    12100       266
Viola       465    644    2440     3160       220
Cello       261    362    1370     5620       123
Bass        170    236     895     3660        80
Guitar      277    385    1519     5973       131
Bass guitar 209    291    1148     4514        99
Frequencies are in Hertz.

Gut was usually used in the Baroque age because steel alloys hadn't been perfected. A-strings were tuned to a frequency of around 420 Hertz. Modern steel made possible the 660 Hertz E-string and the high-frequency strings on a piano.

You can use zylon to make a bass sound like a violin.


Low-frequency strings

Tungsten is a high-density metal that can be used to make low-frequency strings ("Darth Vader" strings). You can make a violin sound like a bass.

The larger the diameter of a string the more difficult it is to play. Diameter sets the lower limit of the frequency of a string.

Frequency = Constant * SquareRoot(Smax/D) / R
String frequency is inversely proportional to radius. A string can be made an octave lower by doubling the radius.

If a string is made of tungsten with a density of 19.25 g/cm^3 then the diameter of the lowest string on each instrument is

-
              Freq   Length  Diameter
              (Hz)    (mm)    (mm)

Violin G      196     320     .46
Viola C       130     388     .62
Cello C        65     690    1.07
Bass E         41    1060    1.18
Guitar E       82     650     .90
Bass guitar E  41     860    1.7

String diameter

The "Tungsten" lines are string diameters for tungsten and the "Zylon" lines are string diameters for zylon. Tungsten diameters assume a density of 19.3 g/cm^3 and zylon diameters assume a density of 1.5 g/cm^3. The zylon lines cut off at the right at the frequency where the string breaks.


String price

The price is for strings made of gold with a density 19.3 g/cm^3, the same as for tungsten. If the strings are made from iridium or osmium then the metal price is half this. For tungsten strings the price of the tungsten is negligible.

Even though iridium is half the price of gold, gold wire may be cheaper because gold is easier to forge.


              Density   Price
              (g/cm^3)  ($/g)

Zylon           1.5     Cheap
Tungsten       19.2       .05
Gold           19.3     40
Rhenium        21.0     10
Platinum       21.4     80
Iridium        22.4     20
Osmium         22.6     20

String stiffness

When a beam is bent it exerts a restoring force. If a string is too stiff it acts like a beam and becomes impossible to play. The stiffness is inversely proportional to the Young's modulus. This is why metal strings are usually wound around a flexible core.

Examples of beam vibrations.


String winding

Strings typically have a flexible core with a low Young's modulus and a high-density metallic winding.


String inharmonicity

The overtones of an ideal string are exact integer ratios. If the string is non-ideal then the overtones can change. The principal source of non-ideality is the finite thickness of the string. String stiffness also contributes non-ideality.

R    =  String radius
L    =  String length
D    =  String density
Y    =  Young's modulus for the string
Force=  Tension force on the string
N    =  An integer greater than or equal to 1
Fn   =  Frequency of overtone N
     =  N F (1 + C N^2)
C    =  Constant of inharmonicity
     =  Pi^3 R^4 Y / (8 L^2 Force)
If C=0 then there is no inharmonicity and the overtones are exact integer multiples of the fundamental mode. If the string has finite thickness then the frequencies of the overtones shift.

Plucked strings exhibit inharmonicity. Bowed strings are "mode-locked" so that the harmonics are exact integer ratios. Reed instruments and the human voice are also mode locked.

The coefficient of inharmonicity can be expressed in terms of density as

C  =  Pi Force Y / (128 D^2 F^4 L^6)
Increasing the density decreases the inharmonicity.

Low strings are more inharmonic than high strings.

The higher the note you play on a string, the smaller the effective string length and the more inharmonic the note. This is what prevents you from playing notes of arbitrarily high frequency.

The following is a table of inharmonicity coefficients for various instruments. We have assumed standard values for the string tension and we assume the string has the density of steel.


               String   Tension  Frequency  Density  Radius  Young's   C
               length  (Newtons)  (Hertz)   (g/cm^3)  (mm)   modulus
                (mm)                                         (GPa)
            
Violin E gut     320      80        660      1.5     .31       6     .000026
Violin E steel   320      80        660      7.9     .13     220     .000033
Violin G steel   320      45        196      7.9     .34     220     .00012
Viola C steel    388      55        130      7.9     .47     220     .00019
Cello C steel    690     130         65      7.9     .81     220     .000098
Bass E steel    1060     160         41      7.9     .92     220     .000047
Guitar E steel   650     140         82      7.9     .70     220     .000058
Bass guitar E    860     220         41      7.9    1.34     220     .00017

If we set the frequency shift from inharmonicity equal to the frequency resolution for human hearing,
N^2 C = 1/170

If C=.0001 then N=7.7       (The inharmonicity appears at the 8th overtone)

Instrument size and inharmonicity

The lower the frequency of a string, the more inharmonic it is. Low-frequency strings typically consist of a synthetic core (for elasticity) and an outer metallic winding (for density). You can't use metal for the entire string because metal is too stiff (the Young's modulus is too high.

An ideal core material has a high tensile strengh, so that you can use a small core diameter, and a low Young's modulus, to minimize inharmonicity. The synthetic material that is best suited for this is Vectran (see the table above).

L    =  Length of the string
R    =  Outer radius of the string
r    =  Radius of the inner core
     =  K R               where K is a dimensionless constant
Y    =  Young's modulus of the core material
D    =  Density of the outer winding
Force=  Force on the string
     =  k L               where k is a constant
Y    =  Young's modulus of the core
S    =  Stress on the inner core
     =  Force / (Pi r^2)
s    =  Strain on the inner core
     =  S/Y
C    =  Constant of inharmonicity
     =  Pi^3 R^4 Y / (8 L^2 Force)
     =  Pi Force Y / (128 D^2 F^4 L^6)
The strain should be as large as possible to minimize the Young's modulus, but if it is too large then the string loses functionality. We assume that the strain is a constant value.

For constant string length the ideal force doesn't depend on frequency.

Force / (Pi r^2) = Y s
The larger the value of "r" the lower the value of "Y" and the lower the inharmonicity.

If "r" is too large compared to "R" then the string loses density. We assume that r is is a fixed fraction of R and that r/R ~ 2/5.

Using

Force  =  Pi R^2 4 D F^2 L^2
       =  Pi r^2 Y s
We have
4 D F^2 L^2  =  K^2 Y s
The inharmonicity is
C  =  Pi Force Y / (128 D^2 F^4 L^6)
   =  Pi Force 4 D F^2 L^2 / (128 K^2 s D^2 F^4 L^6)
   =  Pi Force / (32 K^2 D F^2 s L^4)
   =  Constant * Force / (F^2 L^4)
If we assume that
Force = Constant * L
then
C  =  Constant / (F^2 L^3)
The lowest practical frequency of an instrument scales as L^(-3/2).

Let

Relative inharmonicity  =  1/(Freq^2 Length^3)
The relative inharmonicity of the lowest string for various instruments is given by the following table. The value is similar for all instruments.
              Freq   Length    Relative inharmonicity
              (Hz)    (mm)     = 1/(Freq^2 Length^3)

Violin G      196     320      .00079
Viola C       130     388      .00101
Cello C        65     690      .00072
Bass E         41    1060      .00050
Guitar E       82     650      .00054
Bass guitar E  41     860      .00094

Parameters for low-frequency strings

The following table shows a set of example parameters for low-frequency strings. We assume a core of Vectran (density=1400 kg/m^3) and a winding of osmium (density=22600 kg/m^3).

          Note   Freq   Tension  Core    Core    Outer   Core  Core
                (Hertz)          stress  radius  radius  Young strain
                          (N)    (GPa)   (mm)            (GPa)

Viola       C   130.4     50      .2      .28     .70     70    .0155
Viola       C    65.2     50      .2      .28    1.30     70    .0155
Viola       C    65.2     50     1.0      .126   1.25     70    .0155

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Data from Wikipedia unless otherwise specified.
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Spices

Cumin
Fennel
Caraway
Coriander
Cardamom
Fenugreek
Cubeb

Cashew
Pistachio
Walnut
Hazelnut
Peanut
Almond
Pine

Sesame
Poppy
Chia
Flax
Sunflower
Lotus

Black pepper
Mustard

Cumin
Turmermic
Paprika
Chili

Oregano
Basil
Bay
Coriander
Curry
Sage

Chive
Lemongrass
Tarragon
Arugula
Mint
Dill
Marjoram

Rosemary
Parsley
Saffron
Juniper

Bell pepper
Chili
Jalapeno
Cayenne
Habanero

Onion
Garlic
Clove
Galangal
Cinnamon
Vanilla

Portobello
Shiitake
Oyster
Morel
Enoki
Porcini
Truffle

Olea europaea
Kalamata
Arbequina
Belice

Grapefruit
Orange
Tangerine
Lemon
Lime
Kaffir lime
Key lime
Kiwi

Tomato
Avocado
Coconut
Egg
Olive oil

Milk cream
Sour cream
Butter
Cream cheese
Yogurt

Parmesan
Mozzarella
Reggiano
Asiago

Adzuki
Kidney
Red
Black
Pinto

Coffee
Cacao
Kola

Salt
Monosodium glutamate


Spices

Turmeric: curcumin
Cumin: cuminaldehyde
Chili: capsaicin
Mustard: allyl isotyiolcyanate

Bay: myrcene
Garlic and onion: allicin
Clove: eugenol

Raspberry ketone
Tangerine: tangeritin
Lemon: citral
Lemon peel: limonene

Chocolate: theobromine
Smoke: guaiacol
Cardamom: terpineol
Wintergreen: methyl salicylate

Hydrogen   White
Carbon     Black
Nitrogen   Blue
Oxygen     Red
Sulfur     Yellow
        Scoville scale (relative capsaicin content)

Ghost pepper     1000000
Trinidad         1000000      Trinidad moruga scorpion
Naga Morich      1000000
Habanero          250000
Cayenne pepper     40000
Malagueta pepper   40000
Tabasco            40000
Jalapeno            5000
Guajillo pepper     5000
Cubanelle            500
Banana pepper        500
Bell pepper           50
Pimento               50

Molecule        Relative hotness

Rresiniferatoxin   16000
Tinyatoxin          5300
Capsaicin             16         Chili pepper
Nonivamide             9.2       Chili pepper
Shogaol                 .16      Ginger
Piperine                .1       Black pepper
Gingerol                .06      Ginger
Capsiate                .016     Chili pepper
Caraway: carvone
Black tea: theaflavin
Cinnamon: cinnamaldehyde
Citrus: hesperidin
Fruit: quercetin

Mint: menthol
Juniper: pinene
Saffron: picrocrocin
Saffron: safranal
Wine: tannic acid

Black pepper: piperine
Oregano: carvacrol
Sesame: sesamol
Curry leaf: girinimbine
Aloe emodin
Whiskey lactone


Signalling molecules

Alcohol
Caffeine
Tetrahydrocannabinol
Nicotine

Adrenaline
Noadrenaline
Dopamine
Seratonin

Aspirin
Ibuprofen
Hydrocodone
Morphone

Vitamin A (beta carotene)
Vitamin A (retinol)
Vitamin C (ascorbic acid)
Vitamin D (cholecalciferol)


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© Jason Maron, all rights reserved.

Data from Wikipedia unless otherwise specified.
Atoms

Hydrogen
Helium
Lithium

Elements are built from protons, neutrons, and electrons. The identity of an element is determined by the proton number. The heaviest naturally-occuring element is uranium with 92 protons.

Particle     Charge   Mass (kg)       Mass / Proton mass

Proton         +1     1.673⋅10-27       1
Neutron         0     1.675⋅10-27       1.0012
Electron       -1     9.109⋅10-31        .000544
Proton number

Diatomic molecules

If two atoms of hydrogen encounter each other they combine into a diatomic molecule, releasing energy. All elements that are gases at room temperature are diatomic.
Oxygen O2
Water H2O
Methane CH4
Nitrous oxide N2O
Metal


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© Jason Maron, all rights reserved.

Data from Wikipedia unless otherwise specified.