Jump to content

Hydrogen: Difference between revisions

Edit links
Page semi-protected
Listen to this article
From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
m r2.7.2+) (Robot: Adding ps:هايډروجن
Hodeken (talk | contribs)
144 edits
mNo edit summary
Line 13: Line 13:
}} Note that most of the universe's mass is not in the form of chemical elements, however. See [[dark matter]] and [[dark energy]].</ref> Non-[[stellar remnant|remnant]] [[star]]s are mainly composed of hydrogen in its [[plasma (physics)|plasma]] state. Naturally occurring elemental hydrogen is relatively rare on Earth.
}} Note that most of the universe's mass is not in the form of chemical elements, however. See [[dark matter]] and [[dark energy]].</ref> Non-[[stellar remnant|remnant]] [[star]]s are mainly composed of hydrogen in its [[plasma (physics)|plasma]] state. Naturally occurring elemental hydrogen is relatively rare on Earth.


The most common [[isotope]] of hydrogen is [[hydrogen-1|protium]] (name rarely used, symbol <sup>1</sup>H) with a single [[proton]] and no [[neutron]]s. In [[ionic compound]]s it can take a negative charge (an [[anion]] known as a [[hydride]] and written as H<sup>−</sup>), or as a positively charged [[chemical species|species]] H<sup>+</sup>. The latter [[cation]] is written as though composed of a bare proton, but in reality, hydrogen cations in [[ionic compound]]s always occur as more complex species. Hydrogen forms compounds with most elements and is present in water and most [[organic compound]]s. It plays a particularly important role in [[acid-base reaction theories|acid-base chemistry]] with many reactions exchanging protons between soluble molecules. As the simplest atom known, the [[hydrogen atom]] has been of theoretical use. For example, as the only neutral atom with an analytic solution to the [[Schrödinger equation]], the study of the energetics and bonding of the hydrogen atom played a key role in the development of [[quantum mechanics]].
The most common [[isotope]] of hydrogen is [[hydrogen-1|protium]] (name rarely used, symbol <sup>1</sup>H) with a single [[proton]] and no [[neutron]]s. In [[ionic compound]]s it can take a negative charge (an [[anion]] known as a [[hydride]] and written as H<sup>−</sup>), or as a positively charged [[chemical species|species]] H<sup>+</sup>. The latter [[cation]] is written as though composed of a bare proton, but in reality, hydrogen cations in [[ionic compound]]s always occur as more complex species. Hydrogen forms compounds with most elements and is present in the water molecule and most [[organic compound]]s. It plays a particularly important role in [[acid-base reaction theories|acid-base chemistry]] with many reactions exchanging protons between soluble molecules. As the simplest atom known, the [[hydrogen atom]] has been of theoretical use. For example, as the only neutral atom with an analytic solution to the [[Schrödinger equation]], the study of the energetics and bonding of the hydrogen atom played a key role in the development of [[quantum mechanics]].


Hydrogen gas (now known to be H<sub>2</sub>) was first artificially produced in the early 16th century, via the mixing of metals with strong acids. In 1766–81, [[Henry Cavendish]] was the first to recognize that hydrogen gas was a discrete substance,<ref>
Hydrogen gas (now known to be H<sub>2</sub>) was first artificially produced in the early 16th century, via the mixing of metals with strong acids. In 1766–81, [[Henry Cavendish]] was the first to recognize that hydrogen gas was a discrete substance,<ref>

Revision as of 18:19, 24 April 2012

Template:Two other uses

Hydrogen, 1H
Purple glow in its plasma state
Hydrogen
AppearanceColorless gas
Standard atomic weight Ar°(H)
Hydrogen in the periodic table
Hydrogen Helium
Lithium Beryllium Boron Carbon Nitrogen Oxygen Fluorine Neon
Sodium Magnesium Aluminium Silicon Phosphorus Sulfur Chlorine Argon
Potassium Calcium Scandium Titanium Vanadium Chromium Manganese Iron Cobalt Nickel Copper Zinc Gallium Germanium Arsenic Selenium Bromine Krypton
Rubidium Strontium Yttrium Zirconium Niobium Molybdenum Technetium Ruthenium Rhodium Palladium Silver Cadmium Indium Tin Antimony Tellurium Iodine Xenon
Caesium Barium Lanthanum Cerium Praseodymium Neodymium Promethium Samarium Europium Gadolinium Terbium Dysprosium Holmium Erbium Thulium Ytterbium Lutetium Hafnium Tantalum Tungsten Rhenium Osmium Iridium Platinum Gold Mercury (element) Thallium Lead Bismuth Polonium Astatine Radon
Francium Radium Actinium Thorium Protactinium Uranium Neptunium Plutonium Americium Curium Berkelium Californium Einsteinium Fermium Mendelevium Nobelium Lawrencium Rutherfordium Dubnium Seaborgium Bohrium Hassium Meitnerium Darmstadtium Roentgenium Copernicium Nihonium Flerovium Moscovium Livermorium Tennessine Oganesson
–
↑
H
↓
Li
(none) ← hydrogen → helium
Atomic number (Z)1
Groupgroup 1: hydrogen and alkali metals
Periodperiod 1
Block  s-block
Electron configuration1s1
Electrons per shell1
Physical properties
Phase at STPgas
Melting point(H2) 13.99 K ​(−259.16 °C, ​−434.49 °F)
Boiling point(H2) 20.271 K ​(−252.879 °C, ​−423.182 °F)
Density (at STP)0.08988 g/L
when liquid (at m.p.)0.07 g/cm3 (solid: 0.0763 g/cm3)[3]
when liquid (at b.p.)0.07099 g/cm3
Triple point13.8033 K, ​7.041 kPa
Critical point32.938 K, 1.2858 MPa
Heat of fusion(H2) 0.117 kJ/mol
Heat of vaporization(H2) 0.904 kJ/mol
Molar heat capacity(H2) 28.836 J/(mol·K)
Vapor pressure
P (Pa) 1 10 100 1 k 10 k 100 k
at T (K) 15 20
Atomic properties
Oxidation statescommon: −1, +1
ElectronegativityPauling scale: 2.20
Ionization energies
  • 1st: 1312.0 kJ/mol
Covalent radius31±5 pm
Van der Waals radius120 pm
Color lines in a spectral range
Spectral lines of hydrogen
Other properties
Natural occurrenceprimordial
Crystal structure ​hexagonal (hP4)
Lattice constants
Hexagonal crystal structure for hydrogen
a = 378.97 pm
c = 618.31 pm (at triple point)[4]
Thermal conductivity0.1805 W/(m⋅K)
Magnetic orderingdiamagnetic[5]
Molar magnetic susceptibility−3.98×10−6 cm3/mol (298 K)[6]
Speed of sound1310 m/s (gas, 27 °C)
CAS Number12385-13-6
1333-74-0 (H2)
History
DiscoveryHenry Cavendish[7][8] (1766)
Named byLouis-Bernard Guyton de Morveau
Antoine Lavoisier[9][10] (1787)
Isotopes of hydrogen
Main isotopes Decay
abun­dance half-life (t1/2) mode pro­duct
1H 99.9855% stable
2H 0.0145% stable
3H trace 12.32 y β− 3He
 Category: Hydrogen
| references

Hydrogen (/[invalid input: 'icon']ˈhaɪdr[invalid input: 'ɵ']dʒ[invalid input: 'ɨ']n/ HY-drə-jin)[11] is the chemical element with atomic number 1. It is represented by the symbol H. With an average atomic weight of 1.00794 u (1.007825 u for hydrogen-1), hydrogen is the lightest and most abundant chemical element, constituting roughly 75% of the Universe's chemical elemental mass.[12] Non-remnant stars are mainly composed of hydrogen in its plasma state. Naturally occurring elemental hydrogen is relatively rare on Earth.

The most common isotope of hydrogen is protium (name rarely used, symbol 1H) with a single proton and no neutrons. In ionic compounds it can take a negative charge (an anion known as a hydride and written as H−), or as a positively charged species H+. The latter cation is written as though composed of a bare proton, but in reality, hydrogen cations in ionic compounds always occur as more complex species. Hydrogen forms compounds with most elements and is present in the water molecule and most organic compounds. It plays a particularly important role in acid-base chemistry with many reactions exchanging protons between soluble molecules. As the simplest atom known, the hydrogen atom has been of theoretical use. For example, as the only neutral atom with an analytic solution to the Schrödinger equation, the study of the energetics and bonding of the hydrogen atom played a key role in the development of quantum mechanics.

Hydrogen gas (now known to be H2) was first artificially produced in the early 16th century, via the mixing of metals with strong acids. In 1766–81, Henry Cavendish was the first to recognize that hydrogen gas was a discrete substance,[13] and that it produces water when burned, a property which later gave it its name, which in Greek means "water-former." At standard temperature and pressure, hydrogen is a colorless, odorless, nonmetallic, tasteless, non-toxic, highly combustible diatomic gas with the molecular formula H2.

Industrial production is mainly from the steam reforming of natural gas, and less often from more energy-intensive hydrogen production methods like the electrolysis of water.[14] Most hydrogen is employed near its production site, with the two largest uses being fossil fuel processing (e.g., hydrocracking) and ammonia production, mostly for the fertilizer market.

Hydrogen is a concern in metallurgy as it can embrittle many metals,[15] complicating the design of pipelines and storage tanks.[16]

Properties

Combustion

A black cup-like object hanging by its bottom with blue glow coming out of its opening.
The Space Shuttle Main Engine burnt hydrogen with oxygen, producing a nearly invisible flame at full thrust.

Hydrogen gas (dihydrogen or molecular hydrogen)[17] is highly flammable and will burn in air at a very wide range of concentrations between 4% and 75% by volume.[18] The enthalpy of combustion for hydrogen is −286 kJ/mol:[19]

2 H2(g) + O2(g) → 2 H2O(l) + 572 kJ (286 kJ/mol)[note 1]

Hydrogen gas forms explosive mixtures with air if it is 4–74% concentrated and with chlorine if it is 5–95% concentrated. The mixtures spontaneously explode by spark, heat or sunlight. The hydrogen autoignition temperature, the temperature of spontaneous ignition in air, is 500 °C (932 °F).[20] Pure hydrogen-oxygen flames emit ultraviolet light and are nearly invisible to the naked eye, as illustrated by the faint plume of the Space Shuttle Main Engine compared to the highly visible plume of a Space Shuttle Solid Rocket Booster. The detection of a burning hydrogen leak may require a flame detector; such leaks can be very dangerous. The destruction of the Hindenburg airship was an infamous example of hydrogen combustion; the cause is debated, but the visible flames were the result of combustible materials in the ship's skin.[21] Because hydrogen is buoyant in air, hydrogen flames tend to ascend rapidly and cause less damage than hydrocarbon fires. Two-thirds of the Hindenburg passengers survived the fire, and many deaths were instead the result of falls or burning diesel fuel.[22]

H2 reacts with every oxidizing element. Hydrogen can react spontaneously and violently at room temperature with chlorine and fluorine to form the corresponding hydrogen halides, hydrogen chloride and hydrogen fluoride, which are also potentially dangerous acids.[23]

Electron energy levels

Main article: Hydrogen atom
Drawing of a light-gray large sphere with a cut off quarter and a black small sphere and numbers 1.7x10−5 illustrating their relative diameters.
Depiction of a hydrogen atom with size of central proton shown, and the atomic diameter shown as about twice the Bohr model radius (image not to scale).

The ground state energy level of the electron in a hydrogen atom is −13.6 eV, which is equivalent to an ultraviolet photon of roughly 92 nm wavelength.[24]

The energy levels of hydrogen can be calculated fairly accurately using the Bohr model of the atom, which conceptualizes the electron as "orbiting" the proton in analogy to the Earth's orbit of the Sun. However, the electromagnetic force attracts electrons and protons to one another, while planets and celestial objects are attracted to each other by gravity. Because of the discretization of angular momentum postulated in early quantum mechanics by Bohr, the electron in the Bohr model can only occupy certain allowed distances from the proton, and therefore only certain allowed energies.[25]

A more accurate description of the hydrogen atom comes from a purely quantum mechanical treatment that uses the Schrödinger equation or the Feynman path integral formulation to calculate the probability density of the electron around the proton.[26] The most complicated treatments allow for the small effects of special relativity and vacuum polarization. In the quantum mechanical treatment, the electron in a ground state hydrogen atom has no angular momentum at all— an illustration of how different the "planetary orbit" conception of electron motion differs from reality.

Elemental molecular forms

See also: Spin isomers of hydrogen
Two bright circles on dark background, both contain numerous thin black lines inside.
First tracks observed in liquid hydrogen bubble chamber at the Bevatron

There exist two different spin isomers of hydrogen diatomic molecules that differ by the relative spin of their nuclei.[27] In the orthohydrogen form, the spins of the two protons are parallel and form a triplet state with a molecular spin quantum number of 1 (½+½); in the parahydrogen form the spins are antiparallel and form a singlet with a molecular spin quantum number of 0 (½–½). At standard temperature and pressure, hydrogen gas contains about 25% of the para form and 75% of the ortho form, also known as the "normal form".[28] The equilibrium ratio of orthohydrogen to parahydrogen depends on temperature, but because the ortho form is an excited state and has a higher energy than the para form, it is unstable and cannot be purified. At very low temperatures, the equilibrium state is composed almost exclusively of the para form. The liquid and gas phase thermal properties of pure parahydrogen differ significantly from those of the normal form because of differences in rotational heat capacities, as discussed more fully in Spin isomers of hydrogen.[29] The ortho/para distinction also occurs in other hydrogen-containing molecules or functional groups, such as water and methylene, but is of little significance for their thermal properties.[30]

The uncatalyzed interconversion between para and ortho H2 increases with increasing temperature; thus rapidly condensed H2 contains large quantities of the high-energy ortho form that converts to the para form very slowly.[31] The ortho/para ratio in condensed H2 is an important consideration in the preparation and storage of liquid hydrogen: the conversion from ortho to para is exothermic and produces enough heat to evaporate some of the hydrogen liquid, leading to loss of liquefied material. Catalysts for the ortho-para interconversion, such as ferric oxide, activated carbon, platinized asbestos, rare earth metals, uranium compounds, chromic oxide, or some nickel[32] compounds, are used during hydrogen cooling.[33]

Phases

Compounds

Further information: Hydrogen compounds

Covalent and organic compounds

While H2 is not very reactive under standard conditions, it does form compounds with most elements. Hydrogen can form compounds with elements that are more electronegative, such as halogens (e.g., F, Cl, Br, I), or oxygen; in these compounds hydrogen takes on a partial positive charge.[34] When bonded to fluorine, oxygen, or nitrogen, hydrogen can participate in a form of medium-strength noncovalent bonding called hydrogen bonding, which is critical to the stability of many biological molecules.[35][36] Hydrogen also forms compounds with less electronegative elements, such as the metals and metalloids, in which it takes on a partial negative charge. These compounds are often known as hydrides.[37]

Hydrogen forms a vast array of compounds with carbon called the hydrocarbons, and an even vaster array with heteroatoms that, because of their general association with living things, are called organic compounds.[38] The study of their properties is known as organic chemistry[39] and their study in the context of living organisms is known as biochemistry.[40] By some definitions, "organic" compounds are only required to contain carbon. However, most of them also contain hydrogen, and because it is the carbon-hydrogen bond which gives this class of compounds most of its particular chemical characteristics, carbon-hydrogen bonds are required in some definitions of the word "organic" in chemistry.[38] Millions of hydrocarbons are known, and they are usually formed by complicated synthetic pathways, which seldom involve elementary hydrogen.

Hydrides

Compounds of hydrogen are often called hydrides, a term that is used fairly loosely. The term "hydride" suggests that the H atom has acquired a negative or anionic character, denoted H−, and is used when hydrogen forms a compound with a more electropositive element. The existence of the hydride anion, suggested by Gilbert N. Lewis in 1916 for group I and II salt-like hydrides, was demonstrated by Moers in 1920 with the electrolysis of molten lithium hydride (LiH), that produced a stoichiometry quantity of hydrogen at the anode.[41] For hydrides other than group I and II metals, the term is quite misleading, considering the low electronegativity of hydrogen. An exception in group II hydrides is BeH
2, which is polymeric. In lithium aluminium hydride, the AlH−
4 anion carries hydridic centers firmly attached to the Al(III).

Although hydrides can be formed with almost all main-group elements, the number and combination of possible compounds varies widely; for example, there are over 100 binary borane hydrides known, but only one binary aluminium hydride.[42] Binary indium hydride has not yet been identified, although larger complexes exist.[43]

In inorganic chemistry, hydrides can also serve as bridging ligands that link two metal centers in a coordination complex. This function is particularly common in group 13 elements, especially in boranes (boron hydrides) and aluminium complexes, as well as in clustered carboranes.[44]

Protons and acids

Further information: Acid–base reaction

Oxidation of hydrogen removes its electron and gives H+, which contains no electrons and a nucleus which is usually composed of one proton. That is why H+
 is often called a proton. This species is central to discussion of acids. Under the Bronsted-Lowry theory, acids are proton donors, while bases are proton acceptors.

A bare proton, H+
, cannot exist in solution or in ionic crystals, because of its unstoppable attraction to other atoms or molecules with electrons. Except at the high temperatures associated with plasmas, such protons cannot be removed from the electron clouds of atoms and molecules, and will remain attached to them. However, the term 'proton' is sometimes used loosely and metaphorically to refer to positively charged or cationic hydrogen attached to other species in this fashion, and as such is denoted "H+
" without any implication that any single protons exist freely as a species.

To avoid the implication of the naked "solvated proton" in solution, acidic aqueous solutions are sometimes considered to contain a less unlikely fictitious species, termed the "hydronium ion" (H
3O+
). However, even in this case, such solvated hydrogen cations are thought more realistically physically to be organized into clusters that form species closer to H
9O+
4.[45] Other oxonium ions are found when water is in solution with other solvents.[46]

Although exotic on earth, one of the most common ions in the universe is the H+
3 ion, known as protonated molecular hydrogen or the trihydrogen cation.[47]

Isotopes

Main article: Isotopes of hydrogen
Hydrogen discharge (spectrum) tube
Deuterium discharge (spectrum) tube
Schematic drawing of a positive atom in the center orbited by a negative particle.
Protium, the most common isotope of hydrogen, has one proton and one electron. Unique among all stable isotopes, it has no neutrons (see diproton for a discussion of why others do not exist).

Hydrogen has three naturally occurring isotopes, denoted 1
H, 2
H and 3
H. Other, highly unstable nuclei (4
H to 7
H) have been synthesized in the laboratory but not observed in nature.[48][49]

  • 1
    H     is the most common hydrogen isotope with an abundance of more than 99.98%. Because the nucleus of this isotope consists of only a single proton, it is given the descriptive but rarely used formal name protium.[50]
  • 2
    H    , the other stable hydrogen isotope, is known as deuterium and contains one proton and one neutron in its nucleus. Essentially all deuterium in the universe is thought to have been produced at the time of the Big Bang, and has endured since that time. Deuterium is not radioactive, and does not represent a significant toxicity hazard. Water enriched in molecules that include deuterium instead of normal hydrogen is called heavy water. Deuterium and its compounds are used as a non-radioactive label in chemical experiments and in solvents for 1
    H    -NMR spectroscopy.[51] Heavy water is used as a neutron moderator and coolant for nuclear reactors. Deuterium is also a potential fuel for commercial nuclear fusion.[52]
  • 3
    H     is known as tritium and contains one proton and two neutrons in its nucleus. It is radioactive, decaying into helium-3 through beta decay with a half-life of 12.32 years.[44] It is so radioactive that it can be used in luminous paint, making it useful in such things as watches. The glass prevents the small amount of radiation from getting out.[53] Small amounts of tritium occur naturally because of the interaction of cosmic rays with atmospheric gases; tritium has also been released during nuclear weapons tests.[54] It is used in nuclear fusion reactions,[55] as a tracer in isotope geochemistry,[56] and specialized in self-powered lighting devices.[57] Tritium has also been used in chemical and biological labeling experiments as a radiolabel.[58]

Hydrogen is the only element that has different names for its isotopes in common use today. During the early study of radioactivity, various heavy radioactive isotopes were given their own names, but such names are no longer used, except for deuterium and tritium. The symbols D and T (instead of 2
H and 3
H) are sometimes used for deuterium and tritium, but the corresponding symbol for protium, P, is already in use for phosphorus and thus is not available for protium.[59] In its nomenclatural guidelines, the International Union of Pure and Applied Chemistry allows any of D, T, 2
H, and 3
H to be used, although 2
H and 3
H are preferred.[60]

History

Discovery and use

Main article: Timeline of hydrogen technologies

In 1671, Robert Boyle discovered and described the reaction between iron filings and dilute acids, which results in the production of hydrogen gas.[61][62] In 1766, Henry Cavendish was the first to recognize hydrogen gas as a discrete substance, by naming the gas from a metal-acid reaction "flammable air". He speculated that "flammable air" was in fact identical to the hypothetical substance called "phlogiston"[63][64] and further finding in 1781 that the gas produces water when burned. He is usually given credit for its discovery as an element.[7][8] In 1783, Antoine Lavoisier gave the element the name hydrogen (from the Greek ὕδρω hydro meaning water and γενῆς genes meaning creator)[10] when he and Laplace reproduced Cavendish's finding that water is produced when hydrogen is burned.[8]

Antoine-Laurent de Lavoisier

Lavoisier produced hydrogen for his famous experiments on mass conservation by reacting a flux of steam with metallic iron through an incandescent iron tube heated in a fire. Anaerobic oxidation of iron by the protons of water at high temperature can be schematically represented by the set of following reactions:

   Fe +    H2O → FeO + H2
2 Fe + 3 H2O → Fe2O3 + 3 H2
3 Fe + 4 H2O → Fe3O4 + 4 H2

Many metals such as zirconium undergo a similar reaction with water leading to the production of hydrogen.

Hydrogen was liquefied for the first time by James Dewar in 1898 by using regenerative cooling and his invention, the vacuum flask.[8] He produced solid hydrogen the next year.[8] Deuterium was discovered in December 1931 by Harold Urey, and tritium was prepared in 1934 by Ernest Rutherford, Mark Oliphant, and Paul Harteck.[7] Heavy water, which consists of deuterium in the place of regular hydrogen, was discovered by Urey's group in 1932.[8] François Isaac de Rivaz built the first internal combustion engine powered by a mixture of hydrogen and oxygen in 1806. Edward Daniel Clarke invented the hydrogen gas blowpipe in 1819. The Döbereiner's lamp and limelight were invented in 1823.[8]

The first hydrogen-filled balloon was invented by Jacques Charles in 1783.[8] Hydrogen provided the lift for the first reliable form of air-travel following the 1852 invention of the first hydrogen-lifted airship by Henri Giffard.[8] German count Ferdinand von Zeppelin promoted the idea of rigid airships lifted by hydrogen that later were called Zeppelins; the first of which had its maiden flight in 1900.[8] Regularly scheduled flights started in 1910 and by the outbreak of World War I in August 1914, they had carried 35,000 passengers without a serious incident. Hydrogen-lifted airships were used as observation platforms and bombers during the war.

The first non-stop transatlantic crossing was made by the British airship R34 in 1919. Regular passenger service resumed in the 1920s and the discovery of helium reserves in the United States promised increased safety, but the U.S. government refused to sell the gas for this purpose. Therefore, H2 was used in the Hindenburg airship, which was destroyed in a midair fire over New Jersey on May 6, 1937.[8] The incident was broadcast live on radio and filmed. Ignition of leaking hydrogen is widely assumed to be the cause, but later investigations pointed to the ignition of the aluminized fabric coating by static electricity. But the damage to hydrogen's reputation as a lifting gas was already done.

In the same year the first hydrogen-cooled turbogenerator went into service with gaseous hydrogen as a coolant in the rotor and the stator in 1937 at Dayton, Ohio, by the Dayton Power & Light Co,[65] because of the thermal conductivity of hydrogen gas this is the most common type in its field today.

The nickel hydrogen battery was used for the first time in 1977 aboard the U.S. Navy's Navigation technology satellite-2 (NTS-2).[66] For example, the ISS,[67] Mars Odyssey[68] and the Mars Global Surveyor[69] are equipped with nickel-hydrogen batteries. In the dark part of its orbit, the Hubble Space Telescope is also powered by nickel-hydrogen batteries, which were finally replaced in May 2009, more than 19 years after launch, and 13 years over their design life.

Role in quantum theory

A line spectrum showing black background with narrow lines superimposed on it: two violet, one blue and one red.
Hydrogen emission spectrum lines in the visible range. These are the four visible lines of the Balmer series

Because of its relatively simple atomic structure, consisting only of a proton and an electron, the hydrogen atom, together with the spectrum of light produced from it or absorbed by it, has been central to the development of the theory of atomic structure.[70] Furthermore, the corresponding simplicity of the hydrogen molecule and the corresponding cation H2+ allowed fuller understanding of the nature of the chemical bond, which followed shortly after the quantum mechanical treatment of the hydrogen atom had been developed in the mid-1920s.

One of the first quantum effects to be explicitly noticed (but not understood at the time) was a Maxwell observation involving hydrogen, half a century before full quantum mechanical theory arrived. Maxwell observed that the specific heat capacity of H2 unaccountably departs from that of a diatomic gas below room temperature and begins to increasingly resemble that of a monatomic gas at cryogenic temperatures. According to quantum theory, this behavior arises from the spacing of the (quantized) rotational energy levels, which are particularly wide-spaced in H2 because of its low mass. These widely spaced levels inhibit equal partition of heat energy into rotational motion in hydrogen at low temperatures. Diatomic gases composed of heavier atoms do not have such widely spaced levels and do not exhibit the same effect.[71]

Natural occurrence

A white-green cotton-like clog on black background.
NGC 604, a giant region of ionized hydrogen in the Triangulum Galaxy

Hydrogen, as atomic H, is the most abundant chemical element in the universe, making up 75% of normal matter by mass and over 90% by number of atoms (most of the mass of the universe, however, is not in the form of chemical-element type matter, but rather is postulated to occur as yet-undetected forms of mass such as dark matter and dark energy).[72] This element is found in great abundance in stars and gas giant planets. Molecular clouds of H2 are associated with star formation. Hydrogen plays a vital role in powering stars through proton-proton reaction and CNO cycle nuclear fusion.[73]

Throughout the universe, hydrogen is mostly found in the atomic and plasma states whose properties are quite different from molecular hydrogen. As a plasma, hydrogen's electron and proton are not bound together, resulting in very high electrical conductivity and high emissivity (producing the light from the Sun and other stars). The charged particles are highly influenced by magnetic and electric fields. For example, in the solar wind they interact with the Earth's magnetosphere giving rise to Birkeland currents and the aurora. Hydrogen is found in the neutral atomic state in the Interstellar medium. The large amount of neutral hydrogen found in the damped Lyman-alpha systems is thought to dominate the cosmological baryonic density of the Universe up to redshift z=4.[74]

Under ordinary conditions on Earth, elemental hydrogen exists as the diatomic gas, H2 (for data see table). However, hydrogen gas is very rare in the Earth's atmosphere (1 ppm by volume) because of its light weight, which enables it to escape from Earth's gravity more easily than heavier gases. However, hydrogen is the third most abundant element on the Earth's surface,[75] mostly in the form of chemical compounds such as hydrocarbons and water.[44] Hydrogen gas is produced by some bacteria and algae and is a natural component of flatus, as is methane, itself a hydrogen source of increasing importance.[76]

A molecular form called protonated molecular hydrogen (H
3+) is found in the interstellar medium (ISM), where it is generated by ionization of molecular hydrogen from cosmic rays. It has also been observed in the upper atmosphere of the planet Jupiter. This ion is relatively stable in the environment of outer space due to the low temperature and density. H
3+ is one of the most abundant ions in the Universe, and it plays a notable role in the chemistry of the interstellar medium.[77] Neutral triatomic hydrogen H3 can only exist in an excited form and is unstable.[78] The hydrogen molecular ion (H
2+) is a rare molecular system in the universe.

Production

Further information: Hydrogen production

H2 is produced in chemistry and biology laboratories, often as a by-product of other reactions; in industry for the hydrogenation of unsaturated substrates; and in nature as a means of expelling reducing equivalents in biochemical reactions.

Laboratory

In the laboratory, H2 is usually prepared by the reaction of acids on metals such as zinc with Kipp's apparatus.

Zn + 2 H+
 → Zn2+
 + H
2

Aluminium can also produce H
2 upon treatment with bases:

2 Al + 6 H
2O + 2 OH−
 → 2 Al(OH)−
4 + 3 H
2

The electrolysis of water is a simple method of producing hydrogen. A low voltage current is run through the water, and gaseous oxygen forms at the anode while gaseous hydrogen forms at the cathode. Typically the cathode is made from platinum or another inert metal when producing hydrogen for storage. If, however, the gas is to be burnt on site, oxygen is desirable to assist the combustion, and so both electrodes would be made from inert metals. (Iron, for instance, would oxidize, and thus decrease the amount of oxygen given off.) The theoretical maximum efficiency (electricity used vs. energetic value of hydrogen produced) is in the range 80–94%.[79]

2 H
2O(l) → 2 H
2(g) + O
2(g)

In 2007, it was discovered that an alloy of aluminium and gallium in pellet form added to water could be used to generate hydrogen. The process also creates alumina, but the expensive gallium, which prevents the formation of an oxide skin on the pellets, can be re-used. This has important potential implications for a hydrogen economy, as hydrogen can be produced on-site and does not need to be transported.[80]

Industrial

Main article: Hydrogen production

Hydrogen can be prepared in several different ways, but economically the most important processes involve removal of hydrogen from hydrocarbons. Commercial bulk hydrogen is usually produced by the steam reforming of natural gas.[81] At high temperatures (1000–1400 K, 700–1100 °C or 1300–2000 °F), steam (water vapor) reacts with methane to yield carbon monoxide and H
2.

CH
4 + H
2O → CO + 3 H
2

This reaction is favored at low pressures but is nonetheless conducted at high pressures (2.0  MPa, 20 atm or 600 inHg). This is because high-pressure H
2 is the most marketable product and Pressure Swing Adsorption (PSA) purification systems work better at higher pressures. The product mixture is known as "synthesis gas" because it is often used directly for the production of methanol and related compounds. Hydrocarbons other than methane can be used to produce synthesis gas with varying product ratios. One of the many complications to this highly optimized technology is the formation of coke or carbon:

CH
4 → C + 2 H2

Consequently, steam reforming typically employs an excess of H
2O. Additional hydrogen can be recovered from the steam by use of carbon monoxide through the water gas shift reaction, especially with an iron oxide catalyst. This reaction is also a common industrial source of carbon dioxide:[81]

CO + H
2O → CO
2 + H
2

Other important methods for H
2 production include partial oxidation of hydrocarbons:[82]

2 CH
4 + O
2 → 2 CO + 4 H
2

and the coal reaction, which can serve as a prelude to the shift reaction above:[81]

C + H
2O → CO + H
2

Hydrogen is sometimes produced and consumed in the same industrial process, without being separated. In the Haber process for the production of ammonia, hydrogen is generated from natural gas.[83] Electrolysis of brine to yield chlorine also produces hydrogen as a co-product.[84]

Thermochemical

There are more than 200 thermochemical cycles which can be used for water splitting, around a dozen of these cycles such as the iron oxide cycle, cerium(IV) oxide-cerium(III) oxide cycle, zinc zinc-oxide cycle, sulfur-iodine cycle, copper-chlorine cycle and hybrid sulfur cycle are under research and in testing phase to produce hydrogen and oxygen from water and heat without using electricity.[85] A number of laboratories (including in France, Germany, Greece, Japan, and the USA) are developing thermochemical methods to produce hydrogen from solar energy and water.[86]

Anaerobic corrosion

Under anaerobic conditions, iron and steel alloys are slowly oxidized by the protons of water concomitantly reduced in molecular hydrogen (H2). The anaerobic corrosion of iron leads first to the formation of ferrous hydroxide (green rust) and can be described by the following reaction:

Fe + 2 H2O → Fe(OH)2 + H2

In its turn, under anaerobic conditions, the ferrous hydroxide (Fe(OH)2 ) can be oxidized by the protons of water to form magnetite and molecular hydrogen. This process is described by the Schikorr reaction:

3 Fe(OH)2 → Fe3O4 + 2 H2O + H2
ferrous hydroxide → magnetite + water + hydrogen

The well crystallized magnetite (Fe3O4) is thermodynamically more stable than the ferrous hydroxide (Fe(OH)2 ).

This process occurs during the anaerobic corrosion of iron and steel in oxygen-free groundwater and in reducing soils below the water table.

Geological occurrence: the serpentinization reaction

In the absence of atmospheric oxygen (O2), in deep geological conditions prevailing far away from Earth atmosphere, hydrogen (H2) is produced during the process of serpentinization by the anaerobic oxidation by the water protons (H+) of the ferrous (Fe2+) silicate present in the crystal lattice of the fayalite (Fe2SiO4, the olivine iron-endmember). The corresponding reaction leading to the formation of magnetite (Fe3O4), quartz (SiO2) and hydrogen (H2) is the following:

3 Fe2SiO4 + 2 H2O → 2 Fe3O4 + 3 SiO2 + 3 H2
fayalite + water → magnetite + quartz + hydrogen

This reaction closely resembles the Schikorr reaction observed in the anaerobic oxidation of the ferrous hydroxide in contact with water.

Applications

Consumption in processes

Large quantities of H
2 are needed in the petroleum and chemical industries. The largest application of H
2 is for the processing ("upgrading") of fossil fuels, and in the production of ammonia. The key consumers of H
2 in the petrochemical plant include hydrodealkylation, hydrodesulfurization, and hydrocracking. H
2 has several other important uses. H
2 is used as a hydrogenating agent, particularly in increasing the level of saturation of unsaturated fats and oils (found in items such as margarine), and in the production of methanol. It is similarly the source of hydrogen in the manufacture of hydrochloric acid. H
2 is also used as a reducing agent of metallic ores.[87]

Hydrogen is highly soluble in many rare earth and transition metals[88] and is soluble in both nanocrystalline and amorphous metals.[89] Hydrogen solubility in metals is influenced by local distortions or impurities in the crystal lattice.[90] These properties may be useful when hydrogen is purified by passage through hot palladium disks, but the gas's high solubility is a metallurgical problem, contributing to the embrittlement of many metals,[15] complicating the design of pipelines and storage tanks.[16]

Apart from its use as a reactant, H
2 has wide applications in physics and engineering. It is used as a shielding gas in welding methods such as atomic hydrogen welding.[91][92] H2 is used as the rotor coolant in electrical generators at power stations, because it has the highest thermal conductivity of any gas. Liquid H2 is used in cryogenic research, including superconductivity studies.[93] Because H
2 is lighter than air, having a little more than 1⁄15 of the density of air, it was once widely used as a lifting gas in balloons and airships.[94]

In more recent applications, hydrogen is used pure or mixed with nitrogen (sometimes called forming gas) as a tracer gas for minute leak detection. Applications can be found in the automotive, chemical, power generation, aerospace, and telecommunications industries.[95] Hydrogen is an authorized food additive (E 949) that allows food package leak testing among other anti-oxidizing properties.[96]

Hydrogen's rarer isotopes also each have specific applications. Deuterium (hydrogen-2) is used in nuclear fission applications as a moderator to slow neutrons, and in nuclear fusion reactions.[8] Deuterium compounds have applications in chemistry and biology in studies of reaction isotope effects.[97] Tritium (hydrogen-3), produced in nuclear reactors, is used in the production of hydrogen bombs,[98] as an isotopic label in the biosciences,[58] and as a radiation source in luminous paints.[99]

The triple point temperature of equilibrium hydrogen is a defining fixed point on the ITS-90 temperature scale at 13.8033 kelvins.[100]

Coolant

Hydrogen is commonly used in power stations, as a coolant in generators, due to its specific heat capacity being considerably higher than any other gas.

Energy carrier

See also: Hydrogen economy and Hydrogen infrastructure

Hydrogen is not an energy resource,[101] except in the hypothetical context of commercial nuclear fusion power plants using deuterium or tritium, a technology presently far from development.[102] The Sun's energy comes from nuclear fusion of hydrogen, but this process is difficult to achieve controllably on Earth.[103] Elemental hydrogen from solar, biological, or electrical sources require more energy to make it than is obtained by burning it, so in these cases hydrogen functions as an energy carrier, like a battery. Hydrogen may be obtained from fossil sources (such as methane), but these sources are unsustainable.[101]

The energy density per unit volume of both liquid hydrogen and compressed hydrogen gas at any practicable pressure is significantly less than that of traditional fuel sources, although the energy density per unit fuel mass is higher.[101] Nevertheless, elemental hydrogen has been widely discussed in the context of energy, as a possible future carrier of energy on an economy-wide scale.[104] For example, CO
2 sequestration followed by carbon capture and storage could be conducted at the point of H
2 production from fossil fuels.[105] Hydrogen used in transportation would burn relatively cleanly, with some NOx emissions,[106] but without carbon emissions.[105] However, the infrastructure costs associated with full conversion to a hydrogen economy would be substantial.[107]

Semiconductor industry

Hydrogen is employed to saturate broken ("dangling") bonds of amorphous silicon and amorphous carbon that helps stabilizing material properties.[108] It is also a potential electron donor in various oxide materials, including ZnO,[109][110] SnO2, CdO, MgO,[111] ZrO2, HfO2, La2O3, Y2O3, TiO2, SrTiO3, LaAlO3, SiO2, Al2O3, ZrSiO4, HfSiO4, and SrZrO3.[112]

Biological reactions

Further information: Biohydrogen and Biological hydrogen production

H2 is a product of some types of anaerobic metabolism and is produced by several microorganisms, usually via reactions catalyzed by iron- or nickel-containing enzymes called hydrogenases. These enzymes catalyze the reversible redox reaction between H2 and its component two protons and two electrons. Creation of hydrogen gas occurs in the transfer of reducing equivalents produced during pyruvate fermentation to water.[113]

Water splitting, in which water is decomposed into its component protons, electrons, and oxygen, occurs in the light reactions in all photosynthetic organisms. Some such organisms, including the alga Chlamydomonas reinhardtii and cyanobacteria, have evolved a second step in the dark reactions in which protons and electrons are reduced to form H2 gas by specialized hydrogenases in the chloroplast.[114] Efforts have been undertaken to genetically modify cyanobacterial hydrogenases to efficiently synthesize H2 gas even in the presence of oxygen.[115] Efforts have also been undertaken with genetically modified alga in a bioreactor.[116]

Safety and precautions

Main article: Hydrogen safety

Hydrogen poses a number of hazards to human safety, from potential detonations and fires when mixed with air to being an asphyxiant in its pure, oxygen-free form.[117] In addition, liquid hydrogen is a cryogen and presents dangers (such as frostbite) associated with very cold liquids.[118] Hydrogen dissolves in many metals, and, in addition to leaking out, may have adverse effects on them, such as hydrogen embrittlement,[119] leading to cracks and explosions.[120] Hydrogen gas leaking into external air may spontaneously ignite. Moreover, hydrogen fire, while being extremely hot, is almost invisible, and thus can lead to accidental burns.[121]

Even interpreting the hydrogen data (including safety data) is confounded by a number of phenomena. Many physical and chemical properties of hydrogen depend on the parahydrogen/orthohydrogen ratio (it often takes days or weeks at a given temperature to reach the equilibrium ratio, for which the data is usually given). Hydrogen detonation parameters, such as critical detonation pressure and temperature, strongly depend on the container geometry.[117]

See also

Template:Multicol

Template:Multicol-break

Template:Multicol-end

Notes

  1. ^ 286 kJ/mol: energy per mole of the combustible material (hydrogen)

References

  1. ^ "Standard Atomic Weights: Hydrogen". CIAAW. 2009.
  2. ^ Prohaska, Thomas; Irrgeher, Johanna; Benefield, Jacqueline; Böhlke, John K.; Chesson, Lesley A.; Coplen, Tyler B.; Ding, Tiping; Dunn, Philip J. H.; Gröning, Manfred; Holden, Norman E.; Meijer, Harro A. J. (2022-05-04). "Standard atomic weights of the elements 2021 (IUPAC Technical Report)". Pure and Applied Chemistry. doi:10.1515/pac-2019-0603. ISSN 1365-3075.
  3. ^ Wiberg, Egon; Wiberg, Nils; Holleman, Arnold Frederick (2001). Inorganic chemistry. Academic Press. p. 240. ISBN 978-0123526519.
  4. ^ Arblaster, John W. (2018). Selected Values of the Crystallographic Properties of Elements. Materials Park, Ohio: ASM International. ISBN 978-1-62708-155-9.
  5. ^ Lide, D. R., ed. (2005). "Magnetic susceptibility of the elements and inorganic compounds". CRC Handbook of Chemistry and Physics (PDF) (86th ed.). Boca Raton (FL): CRC Press. ISBN 978-0-8493-0486-6.
  6. ^ Weast, Robert (1984). CRC, Handbook of Chemistry and Physics. Boca Raton, Florida: Chemical Rubber Company Publishing. pp. E110. ISBN 978-0-8493-0464-4.
  7. ^ a b c "Hydrogen". Van Nostrand's Encyclopedia of Chemistry. Wylie-Interscience. 2005. pp. 797–799. ISBN 978-0-471-61525-5. Cite error: The named reference "Nostrand" was defined multiple times with different content (see the help page).
  8. ^ a b c d e f g h i j k l Emsley, John (2001). Nature's Building Blocks. Oxford: Oxford University Press. pp. 183–191. ISBN 978-0-19-850341-5. Cite error: The named reference "nbb" was defined multiple times with different content (see the help page).
  9. ^ Miśkowiec, Paweł (April 2023). "Name game: The naming history of the chemical elements—part 1—from antiquity till the end of 18th century". Foundations of Chemistry. 25 (1): 29–51. doi:10.1007/s10698-022-09448-5.
  10. ^ a b Stwertka, Albert (1996). A Guide to the Elements. Oxford University Press. pp. 16–21. ISBN 978-0-19-508083-4. Cite error: The named reference "Stwertka" was defined multiple times with different content (see the help page).
  11. ^ Simpson, J.A.; Weiner, E.S.C. (1989). "Hydrogen". Oxford English Dictionary. Vol. 7 (2nd ed.). Clarendon Press. ISBN 0-19-861219-2.
  12. ^ Palmer, D. (13 September 1997). "Hydrogen in the Universe". NASA. Retrieved 2008-02-05. Note that most of the universe's mass is not in the form of chemical elements, however. See dark matter and dark energy.
  13. ^ Presenter: Professor Jim Al-Khalili (2010-01-21). "Discovering the Elements". Chemistry: A Volatile History. 25:40 minutes in. BBC. BBC Four.
  14. ^ "Hydrogen Basics — Production". Florida Solar Energy Center. 2007. Retrieved 2008-02-05.
  15. ^ a b Rogers, H.C. (1999). "Hydrogen Embrittlement of Metals". Science. 159 (3819): 1057–1064. Bibcode:1968Sci...159.1057R. doi:10.1126/science.159.3819.1057. PMID 17775040.
  16. ^ a b Christensen, C.H. (9 July 2005). "Making society independent of fossil fuels — Danish researchers reveal new technology". Technical University of Denmark. Retrieved 2008-03-28. {{cite news}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  17. ^ "Dihydrogen". O=CHem Directory. University of Southern Maine. Retrieved 2009-04-06.
  18. ^ Carcassi, M.N.; Fineschi, F. (2005). "Deflagrations of H2–air and CH4–air lean mixtures in a vented multi-compartment environment". Energy. 30 (8): 1439–1451. doi:10.1016/j.energy.2004.02.012.
  19. ^ Committee on Alternatives and Strategies for Future Hydrogen Production and Use, US National Research Council, US National Academy of Engineering (2004). The Hydrogen Economy: Opportunities, Costs, Barriers, and R&D Needs. National Academies Press. p. 240. ISBN 0-309-09163-2.{{cite book}}: CS1 maint: multiple names: authors list (link)
  20. ^ Patnaik, P (2007). A comprehensive guide to the hazardous properties of chemical substances. Wiley-Interscience. p. 402. ISBN 0-471-71458-5.
  21. ^ Dziadecki, J. (2005). "Hindenburg Hydrogen Fire". Retrieved 2007-01-16.
  22. ^ Kelly, M. "The Hindenburg Disaster". About.com:American history. Retrieved 2009-08-08.
  23. ^ Clayton, D.D. (2003). Handbook of Isotopes in the Cosmos: Hydrogen to Gallium. Cambridge University Press. ISBN 0-521-82381-1.
  24. ^ Millar, Tom (December 10, 2003). "Lecture 7, Emission Lines — Examples". PH-3009 (P507/P706/M324) Interstellar Physics. University of Manchester. Retrieved 2008-02-05.
  25. ^ Stern, David P. (2005-05-16). "The Atomic Nucleus and Bohr's Early Model of the Atom". NASA Goddard Space Flight Center (mirror). Retrieved 2007-12-20.
  26. ^ Stern, David P. (2005-02-13). "Wave Mechanics". NASA Goddard Space Flight Center. Retrieved 2008-04-16.
  27. ^ Staff (2003). "Hydrogen (H2) Properties, Uses, Applications: Hydrogen Gas and Liquid Hydrogen". Universal Industrial Gases, Inc. Retrieved 2008-02-05.
  28. ^ Tikhonov, Vladimir I. (2002). "Separation of Water into Its Ortho and Para Isomers". Science. 296 (5577): 2363. doi:10.1126/science.1069513. PMID 12089435. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  29. ^ Hritz, James (2006). "CH. 6 – Hydrogen" (PDF). NASA Glenn Research Center Glenn Safety Manual, Document GRC-MQSA.001. NASA. Retrieved 2008-02-05. {{cite web}}: Unknown parameter |month= ignored (help)
  30. ^ Shinitzky, Meir; Elitzur, Avshalom C. (2006). "Ortho-para spin isomers of the protons in the methylene group". Chirality. 18 (9): 754–756. doi:10.1002/chir.20319. PMID 16856167. {{cite journal}}: More than one of |first1= and |first= specified (help); More than one of |last1= and |last= specified (help)
  31. ^ Milenko, Yu. Ya. (1997). "Natural ortho-para conversion rate in liquid and gaseous hydrogen". Journal of Low Temperature Physics. 107 (1–2): 77–92. Bibcode:1997JLTP..107...77M. doi:10.1007/BF02396837. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  32. ^ "Ortho-Para conversion. Pag. 13" (PDF).
  33. ^ Svadlenak, R. Eldo (1957). "The Conversion of Ortho- to Parahydrogen on Iron Oxide-Zinc Oxide Catalysts". Journal of the American Chemical Society. 79 (20): 5385–5388. doi:10.1021/ja01577a013. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  34. ^ Clark, Jim (2002). "The Acidity of the Hydrogen Halides". Chemguide. Retrieved 2008-03-09.
  35. ^ Kimball, John W. (2003-08-07). "Hydrogen". Kimball's Biology Pages. Retrieved 2008-03-04.
  36. ^ IUPAC Compendium of Chemical Terminology, Electronic version, Hydrogen Bond
  37. ^ Sandrock, Gary (2002-05-02). "Metal-Hydrogen Systems". Sandia National Laboratories. Retrieved 2008-03-23.
  38. ^ a b "Structure and Nomenclature of Hydrocarbons". Purdue University. Retrieved 2008-03-23.
  39. ^ "Organic Chemistry". Dictionary.com. Lexico Publishing Group. 2008. Retrieved 2008-03-23.
  40. ^ "Biochemistry". Dictionary.com. Lexico Publishing Group. 2008. Retrieved 2008-03-23.
  41. ^ Moers, Kurt (1920). "Investigations on the Salt Character of Lithium Hydride". Zeitschrift für Anorganische und Allgemeine Chemie. 113 (191): 179–228. doi:10.1002/zaac.19201130116.
  42. ^ Downs, Anthony J. (1994). "The hydrides of aluminium, gallium, indium, and thallium: a re-evaluation". Chemical Society Reviews. 23 (3): 175–184. doi:10.1039/CS9942300175. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  43. ^ Hibbs, David E. (1999). "A remarkably stable indium trihydride complex: synthesis and characterisation of [InH3P(C6H11)3]". Chemical Communications (2): 185–186. doi:10.1039/a809279f. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  44. ^ a b c Miessler, Gary L. (2003). Inorganic Chemistry (3rd ed.). Prentice Hall. ISBN 0-13-035471-6. {{cite book}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  45. ^ Okumura, Anthony M. (1990). "Infrared spectra of the solvated hydronium ion: vibrational predissociation spectroscopy of mass-selected H3O+•(H2O)n•(H2)m". Journal of Physical Chemistry. 94 (9): 3416–3427. doi:10.1021/j100372a014. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  46. ^ Perdoncin, Giulio (1977). "Protonation Equilibria in Water at Several Temperatures of Alcohols, Ethers, Acetone, Dimethyl Sulfide, and Dimethyl Sulfoxide". Journal of the American Chemical Society. 99 (21): 6983–6986. doi:10.1021/ja00463a035. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  47. ^ Carrington, Alan (1989). "The infrared predissociation spectrum of triatomic hydrogen cation (H3+)". Accounts of Chemical Research. 22 (6): 218–222. doi:10.1021/ar00162a004. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  48. ^ Gurov, Yu. B.; Aleshkin, D. V.; Behr, M. N.; Lapushkin, S. V.; Morokhov, P. V.; Pechkurov, V. A.; Poroshin, N. O.; Sandukovsky, V. G.; Tel'kushev, M. V.; Chernyshev, B. A.; Tschurenkova, T. D (2004). "Spectroscopy of superheavy hydrogen isotopes in stopped-pion absorption by nuclei". Physics of Atomic Nuclei. 68 (3): 491–97. Bibcode:2005PAN....68..491G. doi:10.1134/1.1891200.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  49. ^ Korsheninnikov, A.; Nikolskii, E.; Kuzmin, E.; Ozawa, A.; Morimoto, K.; Tokanai, F.; Kanungo, R.; Tanihata, I.; Timofeyuk, N. (2003). "Experimental Evidence for the Existence of 7H and for a Specific Structure of 8He". Physical Review Letters. 90 (8): 082501. Bibcode:2003PhRvL..90h2501K. doi:10.1103/PhysRevLett.90.082501.
  50. ^ Urey, Harold C. (1933). "Names for the Hydrogen Isotopes". Science. 78 (2035): 602–603. Bibcode:1933Sci....78..602U. doi:10.1126/science.78.2035.602. PMID 17797765. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  51. ^ Oda, Y; Nakamura, H.; Yamazaki, T.; Nagayama, K.; Yoshida, M.; Kanaya, S.; Ikehara, M. (1992). "1H NMR studies of deuterated ribonuclease HI selectively labeled with protonated amino acids". Journal of Biomolecular NMR. 2 (2): 137–47. doi:10.1007/BF01875525. PMID 1330130.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  52. ^ Broad, William J. (November 11, 1991). "Breakthrough in Nuclear Fusion Offers Hope for Power of Future". The New York Times. Retrieved 2008-02-12.
  53. ^ The Elements, Theodore Gray, Black Dog & Leventhal Publishers Inc., 2009
  54. ^ Staff (November 15, 2007). "Tritium". U.S. Environmental Protection Agency. Retrieved 2008-02-12.
  55. ^ Nave, C. R. (2006). "Deuterium-Tritium Fusion". HyperPhysics. Georgia State University. Retrieved 2008-03-08.
  56. ^ Kendall, Carol; Caldwell, Eric (1998). "Fundamentals of Isotope Geochemistry". US Geological Survey. Retrieved 2008-03-08. {{cite journal}}: Cite journal requires |journal= (help)
  57. ^ "The Tritium Laboratory". University of Miami. 2008. Retrieved 2008-03-08.
  58. ^ a b Holte, Aurali E.; Houck, Marilyn A.; Collie, Nathan L. (2004). "Potential Role of Parasitism in the Evolution of Mutualism in Astigmatid Mites". Experimental and Applied Acarology. 25 (2). Lubbock: Texas Tech University: 97–107. doi:10.1023/A:1010655610575.
  59. ^ van der Krogt, Peter (May 5, 2005). "Hydrogen". Elementymology & Elements Multidict. Retrieved 2010-12-20.
  60. ^ § IR-3.3.2, Provisional Recommendations, Nomenclature of Inorganic Chemistry, Chemical Nomenclature and Structure Representation Division, IUPAC. Accessed on line October 3, 2007.
  61. ^ Boyle, Robert "Tracts written by the Honourable Robert Boyle containing new experiments, touching the relation betwixt flame and air..." (London, England: 1672).
  62. ^ Winter, Mark (2007). "Hydrogen: historical information". WebElements Ltd. Retrieved 2008-02-05.
  63. ^ "Why did oxygen supplant phlogiston? Research programmes in the Chemical Revolution – Cambridge Books Online – Cambridge University Press". Retrieved 2011-10-22.
  64. ^ Just the Facts—Inventions & Discoveries, School Specialty Publishing, 2005
  65. ^ "A chronological history of electrical development from 600 B.C". Archive.org. Retrieved 2009-04-06.
  66. ^ "NTS-2 Nickel-Hydrogen Battery Performance 31". Aiaa.org. Retrieved 2009-04-06.
  67. ^ Jannette, A.G.; Hojnicki, J.S.; McKissock, D.B.; Fincannon, J.; Kerslake, T.W.; Rodriguez, C.D. (2004 (2002)). "IECEC '02. 2002 37th Intersociety Energy Conversion Engineering Conference, 2002" (PDF): 45–50. doi:10.1109/IECEC.2002.1391972. ISBN 0-7803-7296-4. Retrieved 2011-11-11. {{cite journal}}: |chapter= ignored (help); Check date values in: |year= (help); Cite journal requires |journal= (help)CS1 maint: year (link)
  68. ^ Anderson, P.M.; Coyne, J.W. (2002). "A lightweight high reliability single battery power system for interplanetary spacecraft". 5: 5–2433. doi:10.1109/AERO.2002.1035418. ISBN 0-7803-7231-X. {{cite journal}}: |chapter= ignored (help); Cite journal requires |journal= (help)
  69. ^ "Mars Global Surveyor". Astronautix.com. Retrieved 2009-04-06.
  70. ^ Crepeau, Bob (2006-01-01). Niels Bohr: The Atomic Model. Great Neck Publishing. ISBN 1-4298-0723-7. {{cite book}}: |journal= ignored (help)
  71. ^ Berman, R. (1956). "Cryogenics". Annual Review of Physical Chemistry. 7: 1–20. Bibcode:1956ARPC....7....1B. doi:10.1146/annurev.pc.07.100156.000245. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  72. ^ Gagnon, Steve. "Hydrogen". Jefferson Lab. Retrieved 2008-02-05.
  73. ^ Haubold, Hans (November 15, 2007). "Solar Thermonuclear Energy Generation". Columbia University. Retrieved 2008-02-12. {{cite web}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  74. ^ Storrie-Lombardi, Lisa J. (2000). "Surveys for z > 3 Damped Lyman-alpha Absorption Systems: the Evolution of Neutral Gas". Astrophysical Journal. 543: 552–576. arXiv:astro-ph/0006044. Bibcode:2000ApJ...543..552S. doi:10.1086/317138. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  75. ^ Dresselhaus, Mildred; et al. (May 15, 2003). "Basic Research Needs for the Hydrogen Economy" (PDF). Argonne National Laboratory, U.S. Department of Energy, Office of Science Laboratory. Retrieved 2008-02-05. {{cite web}}: Explicit use of et al. in: |author= (help)
  76. ^ Berger, Wolfgang H. (November 15, 2007). "The Future of Methane". University of California, San Diego. Retrieved 2008-02-12.
  77. ^ McCall Group, Oka Group (April 22, 2005). "H3+ Resource Center". Universities of Illinois and Chicago. Retrieved 2008-02-05.
  78. ^ Helm, H.; et al. "Coupling of Bound States to Continuum States in Neutral Triatomic Hydrogen" (PDF). Department of Molecular and Optical Physics, University of Freiburg, Germany. Retrieved 2009-11-25. {{cite web}}: Explicit use of et al. in: |author= (help)
  79. ^ Kruse, B. (2002). "Hydrogen Status og Muligheter" (PDF). Bellona. Retrieved 2008-02-12. {{cite web}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  80. ^ Venere, Emil (May 15, 2007). "New process generates hydrogen from aluminum alloy to run engines, fuel cells". Purdue University. Retrieved 2008-02-05.
  81. ^ a b c Oxtoby, D. W. (2002). Principles of Modern Chemistry (5th ed.). Thomson Brooks/Cole. ISBN 0-03-035373-4.
  82. ^ "Hydrogen Properties, Uses, Applications". Universal Industrial Gases, Inc. 2007. Retrieved 2008-03-11.
  83. ^ Funderburg, Eddie (2008). "Why Are Nitrogen Prices So High?". The Samuel Roberts Noble Foundation. Retrieved 2008-03-11.
  84. ^ Lees, Andrew (2007). "Chemicals from salt". BBC. Archived from the original on October 26, 2007. Retrieved 2008-03-11. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  85. ^ "Development of solar-powered thermochemical production of hydrogen from water" (PDF).
  86. ^ Perret, Robert. "Development of Solar-Powered Thermochemical Production of Hydrogen from Water, DOE Hydrogen Program, 2007" (PDF). Retrieved 2008-05-17.
  87. ^ Chemistry Operations (2003-12-15). "Hydrogen". Los Alamos National Laboratory. Retrieved 2008-02-05.
  88. ^ Takeshita, T.; Wallace, W.E.; Craig, R.S. (1974). "Hydrogen solubility in 1:5 compounds between yttrium or thorium and nickel or cobalt". Inorganic Chemistry. 13 (9): 2282–2283. doi:10.1021/ic50139a050.
  89. ^ Kirchheim, R.; Mutschele, T.; Kieninger, W.; Gleiter, H; Birringer, R; Koble, T (1988). "Hydrogen in amorphous and nanocrystalline metals". Materials Science and Engineering. 99: 457–462. doi:10.1016/0025-5416(88)90377-1.
  90. ^ Kirchheim, R. (1988). "Hydrogen solubility and diffusivity in defective and amorphous metals". Progress in Materials Science. 32 (4): 262–325. doi:10.1016/0079-6425(88)90010-2.
  91. ^ Durgutlu, Ahmet (2003). "Experimental investigation of the effect of hydrogen in argon as a shielding gas on TIG welding of austenitic stainless steel". Materials & Design. 25 (1): 19–23. doi:10.1016/j.matdes.2003.07.004.
  92. ^ "Atomic Hydrogen Welding". Specialty Welds. 2007.
  93. ^ Hardy, Walter N. (2003). "From H2 to cryogenic H masers to HiTc superconductors: An unlikely but rewarding path". Physica C: Superconductivity. 388–389: 1–6. Bibcode:2003PhyC..388....1H. doi:10.1016/S0921-4534(02)02591-1.
  94. ^ Barnes, Matthew (2004). "LZ-129, Hindenburg". The Great Zeppelins. Retrieved 2008-03-18.
  95. ^ Block, Matthias (2004-09-03). "Hydrogen as Tracer Gas for Leak Detection". 16th WCNDT 2004. Montreal, Canada: Sensistor Technologies. Retrieved 2008-03-25. {{cite conference}}: Unknown parameter |booktitle= ignored (|book-title= suggested) (help)
  96. ^ "Report from the Commission on Dietary Food Additive Intake" (PDF). European Union. Retrieved 2008-02-05.
  97. ^ Reinsch, J (1980). "The deuterium isotope effect upon the reaction of fatty acyl-CoA dehydrogenase and butyryl-CoA". J. Biol. Chem. 255 (19): 9093–97. PMID 7410413. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  98. ^ Bergeron, Kenneth D. (2004). "The Death of no-dual-use". Bulletin of the Atomic Scientists. 60 (1). Educational Foundation for Nuclear Science, Inc.: 15. doi:10.2968/060001004.
  99. ^ Quigg, Catherine T. (1984). "Tritium Warning". Bulletin of the Atomic Scientists. 40 (3): 56–57. {{cite journal}}: Unknown parameter |month= ignored (help)
  100. ^ "International Temperature Scale of 1990" (PDF). Procès-Verbaux du Comité International des Poids et Mesures. 1989. pp. T23–T42. Retrieved 2008-03-25. {{cite conference}}: Unknown parameter |booktitle= ignored (|book-title= suggested) (help)
  101. ^ a b c McCarthy, John (1995-12-31). "Hydrogen". Stanford University. Retrieved 2008-03-14.
  102. ^ "Nuclear Fusion Power". World Nuclear Association. 2007. Retrieved 2008-03-16. {{cite web}}: Unknown parameter |month= ignored (help)
  103. ^ "Chapter 13: Nuclear Energy — Fission and Fusion". Energy Story. California Energy Commission. 2006. Retrieved 2008-03-14.
  104. ^ "DOE Seeks Applicants for Solicitation on the Employment Effects of a Transition to a Hydrogen Economy". Hydrogen Program (Press release). US Department of Energy. 2006-03-22. Retrieved 2008-03-16.
  105. ^ a b "Carbon Capture Strategy Could Lead to Emission-Free Cars" (Press release). Georgia Tech. 2008-02-11. Retrieved 2008-03-16.
  106. ^ Heffel, James W. (2002). "NOx emission and performance data for a hydrogen fueled internal combustion engine at 1500 rpm using exhaust gas recirculation". International Journal of Hydrogen Energy. 28 (8): 901–908. doi:10.1016/S0360-3199(02)00157-X.
  107. ^ Romm, Joseph J. (2004). The Hype About Hydrogen: Fact And Fiction In The Race To Save The Climate (1st ed.). Island Press. ISBN 1-55963-703-X.
  108. ^ Le Comber, P. G.; Jones, D. I.; Spear, W. E. (1977). "Hall effect and impurity conduction in substitutionally doped amorphous silicon". Philosophical Magazine. 35 (5): 1173–1187. Bibcode:1977PMag...35.1173C. doi:10.1080/14786437708232943. {{cite journal}}: Unknown parameter |unused_data= ignored (help)
  109. ^ Van de Walle, Chris G. (2000). "Hydrogen as a cause of doping in zinc oxide". Physical Review Letters. 85 (5): 1012–1015. Bibcode:2000PhRvL..85.1012V. doi:10.1103/PhysRevLett.85.1012. PMID 10991462.
  110. ^ Janotti, Anderson; Van De Walle, CG (2007). "Hydrogen multicentre bonds". Nature Materials. 6 (1): 44–47. Bibcode:2007NatMa...6...44J. doi:10.1038/nmat1795. PMID 17143265. {{cite journal}}: Unknown parameter |unused_data= ignored (help)
  111. ^ Kilic, Cetin; Zunger, Alex (2002). "n-type doping of oxides by hydrogen". Applied Physics Letters. 81 (1): 73–75. Bibcode:2002ApPhL..81...73K. doi:10.1063/1.1482783. {{cite journal}}: Unknown parameter |unused_data= ignored (help)
  112. ^ Peacock, P. W.; Robertson, J. (2003). "Behavior of hydrogen in high dielectric constant oxide gate insulators". Applied Physics Letters. 83 (10): 2025–2027. Bibcode:2003ApPhL..83.2025P. doi:10.1063/1.1609245. {{cite journal}}: Unknown parameter |unused_data= ignored (help)
  113. ^ Cammack, Richard (2001). Hydrogen as a Fuel: Learning from Nature. Taylor & Francis Ltd. pp. 202–203. ISBN 0-415-24242-8. {{cite book}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  114. ^ Kruse, O. (2005). "Improved photobiological H2 production in engineered green algal cells". The Journal of Biological Chemistry. 280 (40): 34170–7. doi:10.1074/jbc.M503840200. PMID 16100118. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)CS1 maint: unflagged free DOI (link)
  115. ^ Smith, H. O. (2005). "IV.E.6 Hydrogen from Water in a Novel Recombinant Oxygen-Tolerant Cyanobacteria System" (PDF). FY2005 Progress Report. United States Department of Energy. Retrieved 2008-02-05. {{cite web}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  116. ^ Williams, Chris (2006-02-24). "Pond life: the future of energy". Science. The Register. Retrieved 2008-03-24.
  117. ^ a b Smith, H. O. (1997). "Safety Standard for Hydrogen and Hydrogen Systems" (PDF). NASA. Retrieved 2008-02-05. {{cite web}}: More than one of |author= and |last= specified (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  118. ^ "Liquid Hydrogen MSDS" (PDF). Praxair, Inc. 2004. Retrieved 2008-04-16. {{cite web}}: Unknown parameter |month= ignored (help)
  119. ^ "'Bugs' and hydrogen embrittlement". Science News. 128 (3). Washington, D.C.: 41 1985-07-20. doi:10.2307/3970088. JSTOR 3970088.
  120. ^ Hayes, B. "Union Oil Amine Absorber Tower". TWI. Retrieved 29 January 2010.
  121. ^ "Hydrogen Safety". Humboldt State University. Retrieved 2010-04-14.

Further reading

Listen to this article
(3 parts, 32 minutes)
  1. Part 1
Spoken Wikipedia icon
These audio files were created from a revision of this article dated
Error: no date provided
, and do not reflect subsequent edits.
(Audio help · More spoken articles)

Template:Link FA Template:Link FA Template:Link FA Template:Link FA Template:Link FA Template:Link FA Template:Link GA Template:Link GA Template:Link GA

Retrieved from "https://en.wikipedia.org/w/index.php?title=Hydrogen&oldid=489025527"