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Hydrogen

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This article is about the chemical element. For other uses, seeHydrogen (disambiguation).

Chemical element with atomic number 1 (H)
Hydrogen, 1H
A clear tube with blue and purple light emanating from it
Purple glow in hydrogen's plasma state
Hydrogen
AppearanceColorless gas
Standard atomic weightAr°(H)
Hydrogen in theperiodic table
HydrogenHelium
LithiumBerylliumBoronCarbonNitrogenOxygenFluorineNeon
SodiumMagnesiumAluminiumSiliconPhosphorusSulfurChlorineArgon
PotassiumCalciumScandiumTitaniumVanadiumChromiumManganeseIronCobaltNickelCopperZincGalliumGermaniumArsenicSeleniumBromineKrypton
RubidiumStrontiumYttriumZirconiumNiobiumMolybdenumTechnetiumRutheniumRhodiumPalladiumSilverCadmiumIndiumTinAntimonyTelluriumIodineXenon
CaesiumBariumLanthanumCeriumPraseodymiumNeodymiumPromethiumSamariumEuropiumGadoliniumTerbiumDysprosiumHolmiumErbiumThuliumYtterbiumLutetiumHafniumTantalumTungstenRheniumOsmiumIridiumPlatinumGoldMercury (element)ThalliumLeadBismuthPoloniumAstatineRadon
FranciumRadiumActiniumThoriumProtactiniumUraniumNeptuniumPlutoniumAmericiumCuriumBerkeliumCaliforniumEinsteiniumFermiumMendeleviumNobeliumLawrenciumRutherfordiumDubniumSeaborgiumBohriumHassiumMeitneriumDarmstadtiumRoentgeniumCoperniciumNihoniumFleroviumMoscoviumLivermoriumTennessineOganesson


H

Li
(none) ←hydrogenhelium
Atomic number(Z)1
Groupgroup 1: hydrogen andalkali metals
Periodperiod 1
Block s-block
Electron configuration1s1
Electrons per shell1
Physical properties
Phaseat 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)1101001 k10 k100 k
at T (K)1520
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 structurehexagonal (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 sound1310m/s (gas, 27 °C)
CAS Number12385-13-6
1333-74-0 (H2)
History
Namingname means 'water-former' in Greek
Discovery and first isolationHenry Cavendish[7][9][10] (1766)
Named byAntoine Lavoisier[7][8] (1783)
Isotopes of hydrogen
Main isotopes[11]Decay
Isotopeabun­dancehalf-life(t1/2)modepro­duct
1H99.9855%stable
2H0.0145%stable
3Htrace12.32 yβ3He
Abundance of deuterium is highly variable
 Category: Hydrogen
| references

Hydrogen is achemical element; it has thesymbol H andatomic number 1. It is thelightest andmost abundant chemical element in the universe, constituting about 75% of allnormal matter. Understandard conditions, hydrogen is agas ofdiatomic molecules with theformula H2, calleddihydrogen, or sometimeshydrogen gas,molecular hydrogen, or simply hydrogen. Dihydrogen is colorless, odorless, non-toxic, and highlycombustible.Stars, including theSun, mainly consist of hydrogen in aplasma state, while on Earth, hydrogen is found as the gas H2 (dihydrogen) and inmolecules, such as inwater andorganic compounds. The most commonisotope of hydrogen,1H, consists of oneproton, oneelectron, and noneutrons.

Hydrogen gas was first produced artificially in the 17th century by thereaction ofacids with metals.Henry Cavendish, in 1766–1781, identified hydrogen gas as a distinct substance and discovered its property of producing water when burned: this is the origin of hydrogen's name, which means'water-former' (fromAncient Greek:ὕδωρ,romanizedhúdōr,lit.'water', andγεννάω,gennáō, 'I bring forth'). Understanding thecolors of light absorbed and emitted by hydrogen was a crucial part of the development ofquantum mechanics.

Hydrogen, typicallynonmetallic except underextreme pressure, readily formscovalent bonds with most nonmetals, contributing to the formation of compounds like water and various organic substances. Its role is crucial inacid-base reactions, which mainly involve proton exchange amongsoluble molecules. Inionic compounds, hydrogen can take the form of either a negatively-chargedanion, where it is known ashydride, or as a positively-chargedcation,H+, called a proton. Although tightly bonded to water molecules, protons strongly affect the behavior ofaqueous solutions, as reflected in the importance ofpH. Hydride, on the other hand, is rarely observed because it tends to deprotonate solvents, yielding H2.

In theearly universe, neutral hydrogen atomsformed about 370,000 years after the Big Bang as the universe expanded and plasma had cooled enough for electrons to remain bound to protons. After starsbegan to form, most of the hydrogen in theintergalactic medium was re-ionized.

Nearly allhydrogen production is done by transformingfossil fuels, particularlysteam reforming ofnatural gas. It can also be produced from water or saline byelectrolysis, but this process is more expensive. Its main industrial uses include fossil fuel processing andammonia production for fertilizer. Emerging uses for hydrogen include the use offuel cells to generate electricity.

Properties

Atomic hydrogen

Electron energy levels

Main article:Hydrogen atom

Theground stateenergy level of the electron in a hydrogen atom is −13.6 electronvolts (eV),[12] equivalent to anultravioletphoton of roughly 91 nanometers wavelength.[13] The energy levels of hydrogen are referred to by consecutivequantum numbers, withn=1{\displaystyle n=1} being the ground state. Thehydrogen spectral series corresponds to emission of light due to transitions from higher to lower energy levels.[14]: 105  Each energy level is further split byspin interactions between the electron and proton into fourhyperfine levels.[15]

High-precision values for the hydrogen atom energy levels are required for definitions of physical constants. Quantum calculations have identified nine contributions to the energy levels. Theeigenvalue from theDirac equation is the largest contribution. Other terms includerelativistic recoil, theself-energy, and thevacuum polarization terms.[16]

Isotopes

Main article:Isotopes of hydrogen
Diagram showing the structure of each of Hydrogen-1 (mass number 1, 1 electron, 1 proton), Hydrogen-2 or deuterium (mass number 2, 1 electron, 1 proton, 1 neutron), and Hydrogen-3 or tritium (mass number 3, 1 electron, 1 proton, 2 neutrons)
The three naturally-occurring isotopes of hydrogen: hydrogen-1 (protium), hydrogen-2 (deuterium), and hydrogen-3 (tritium)

Hydrogen has three naturally-occurring isotopes, denoted1
H
,2
H
and 3
H
. Other, highly-unstablenuclides (4
H
to7
H
) have beensynthesized in laboratories but not observed in nature.[17][18]

1
H
is the most common hydrogen isotope, with an abundance of >99.98%. Because thenucleus of this isotope consists of only a single proton, it is given the descriptive but rarely used formal nameprotium.[19] It is the only stable isotope with no neutrons (seediproton for a discussion of why others do not exist).[20]

2
H
, the other stable hydrogen isotope, is known asdeuterium and contains one proton and oneneutron in the nucleus. Nearly all deuterium nuclei in the universe are thought to have been produced inBig Bang nucleosynthesis, and have endured since then.[21]: 24.2  Deuterium is not radioactive, and is not a significant toxicity hazard. Water enriched in molecules that include deuterium instead of normal hydrogen is calledheavy water. Deuterium and its compounds are used as a non-radioactive label in chemical experiments and in solvents for1
H
-NMR spectroscopy.[22] Heavy water is used as aneutron moderator and coolant for nuclear reactors. Deuterium is also a potential fuel for commercialnuclear fusion.[23]

3
H
is known astritium and contains one proton and two neutrons in its nucleus. It is radioactive, decaying intohelium-3 throughbeta decay with ahalf-life of 12.32 years.[24] It is radioactive enough to be used inluminous paint to enhance the visibility of data displays, such as for painting the hands and dial-markers of watches. The watch glass prevents the small amount of radiation from escaping the case.[25] Small amounts of tritium are produced naturally bycosmic rays striking atmospheric gases; tritium has also been released innuclear weapons tests.[26] It is used in nuclear fusion,[27] as a tracer inisotope geochemistry,[28] and in specializedself-powered lighting devices.[29] Tritium has also been used in chemical and biological labeling experiments as aradiolabel.[30]

Unique among the elements, distinct names are assigned to hydrogen's isotopes in common use. During the early study of radioactivity, heavy radioisotopes were given their own names, but these are mostly no longer used. The symbols D and T (instead of2
H
and3
H
) are sometimes used for deuterium and tritium, but the symbol P was already used forphosphorus and thus was not available for protium.[31] In itsnomenclatural guidelines, theInternational Union of Pure and Applied Chemistry (IUPAC) allows any of D, T,2
H
, and3
H
to be used, though2
H
and3
H
are preferred.[32]

Antihydrogen (H) is theantimatter counterpart to hydrogen. It consists of ananti­proton with apositron.[33][34] Theexotic atommuonium (symbol Mu), composed of anantimuon and anelectron, is the anti­matter analogue of hydrogen;IUPAC nomenclature incorporates such hypothetical compounds as muonium chloride (MuCl) and sodium muonide (NaMu), analogous tohydrogen chloride andsodium hydride respectively.[35]

Dihydrogen

Understandard conditions, hydrogen is agas ofdiatomic molecules with theformula H2, officially called "dihydrogen",[36]: 308  but also called "molecular hydrogen",[37] or simply hydrogen. Dihydrogen is a colorless, odorless, flammable gas.[37]

Combustion

Combustion of hydrogen with the oxygen in the air. When the bottom cap is removed, allowing air to enter, hydrogen in the container rises and burns as it mixes with the air.

Hydrogen gas is highly flammable, reacting withoxygen in air to produce liquid water:

2 H2(g) + O2(g) → 2 H2O(l)

Theamount of heat released permole of hydrogen is−286 kilojoules (kJ), or141.865 megajoules (MJ) for a one-kilogram (2.2 lb) mass.[38]

Hydrogen gas forms explosive mixtures with air in concentrations from4%–74%[39] and with chlorine at5%–95%. The hydrogenautoignition temperature, the temperature of spontaneous ignition in air, is 500 °C (932 °F).[40] In a high-pressurehydrogen leak, the shock wave from the leak itself can heat air to the autoignition temperature, leading to flaming and possibly explosion.[41]

Hydrogen flames emit faint blue andultraviolet light.[42]Flame detectors are used to detect hydrogen fires as they are nearly invisible to the naked eye in daylight.[43][44]

Spin isomers

Main article:Spin isomers of hydrogen

MolecularH2 exists as twonuclear isomers that differ in thespin states of their nuclei.[45] In theortho­hydrogen form, the spins of the two nuclei are parallel, forming a spintriplet state having atotal molecular spinS=1{\displaystyle S=1}; in thepara­hydrogen form the spins are anti­parallel and form a spinsinglet state having spinS=0{\displaystyle S=0}. The equilibrium ratio of ortho- to para-hydrogen depends on temperature. At room temperature or warmer, equilibrium hydrogen gas contains about 25% of the para form and 75% of the ortho form.[46] The ortho form is anexcited state, having higher energy than the para form by1.455 kJ/mol,[47] and it converts to the para form over the course of several minutes when cooled to low temperature.[48] The thermal properties of these isomers differ because each has distinctrotational quantum states.[49]

The ortho-to-para ratio inH2 is an important consideration in theliquefaction and storage ofliquid hydrogen: the conversion from ortho to para isexothermic, and produces sufficient heat to evaporate most of the liquid if the conversion to para­hydrogen does not occur during the cooling process.[50]Catalysts for the ortho-para inter­conversion, such asferric oxide andactivated carbon compounds, are therefore used during hydrogen cooling to avoid this loss of liquid.[51]

Phases

Phase diagram of hydrogen on logarithmic scales. Lines show boundaries between phases, with the end of the liquid-gas line indicating the critical point. The triple point of hydrogen is just off-scale to the left.
Phase diagram of hydrogen with alogarithmic scale. The left edge corresponds to about oneatmosphere.[52]

Liquid hydrogen can exist at temperatures below hydrogen'scritical point of 33kelvins (−240.2 °C; −400.3 °F).[53] However, for it to be in a fully liquid state atatmospheric pressure, H2 needs to be cooled to 20.28 K (−252.87 °C; −423.17 °F). Hydrogen was liquefied byJames Dewar in 1898 by usingregenerative cooling and his invention, thevacuum flask.[54]

Liquid hydrogen becomessolid hydrogen atstandard pressure below hydrogen'smelting point of 14.01 K (−259.14 °C; −434.45 °F). Distinct solid phases exist, known as Phase I through Phase V, each exhibiting a characteristic molecular arrangement.[55] Liquid and solid phases can exist in combination at thetriple point; this mixture is known asslush hydrogen.[56]

Metallic hydrogen, a phase obtained at extremely high pressures (in excess of 400 million Pa (58,000 psi)), is an electrical conductor. It is believed to exist deep withingiant planets likeJupiter.[55][57]

Whenionized, hydrogen becomes aplasma. This is the form in which hydrogen exists withinstars.[58]

Thermal and physical properties

Thermal and physical properties of hydrogen (H2) at atmospheric pressure[59][60]
Temperature (K)Density (kg/m3)Specific heat (kJ/kg K)Dynamic viscosity (kg/m s)Kinematic viscosity (m2/s)Thermal conductivity (W/m K)Thermal diffusivity (m2/s)Prandtl Number
1000.2425511.234.21E-061.74E-056.70E-022.46E-050.707
1500.1637112.6025.60E-063.42E-050.09814.75E-050.718
2000.122713.546.81E-065.55E-050.12827.72E-050.719
2500.0981914.0597.92E-068.06E-050.15611.13E-040.713
3000.0818514.3148.96E-061.10E-040.1821.55E-040.706
3500.0701614.4369.95E-061.42E-040.2062.03E-040.697
4000.0613514.4911.09E-051.77E-040.2282.57E-040.69
4500.0546214.4991.18E-052.16E-040.2513.16E-040.682
5000.0491814.5071.26E-052.57E-040.2723.82E-040.675
5500.0446914.5321.35E-053.02E-040.2924.52E-040.668
6000.0408514.5371.43E-053.50E-040.3155.31E-040.664
7000.0349214.5741.59E-054.55E-040.3516.90E-040.659
8000.030614.6751.74E-055.69E-040.3848.56E-040.664
9000.0272314.8211.88E-056.90E-040.4121.02E-030.676
10000.0242414.992.01E-058.30E-040.4481.23E-030.673
11000.0220415.172.13E-059.66E-040.4881.46E-030.662
12000.020215.372.26E-051.12E-030.5281.70E-030.659
13000.0186515.592.39E-051.28E-030.5681.96E-030.655
14000.0173215.812.51E-051.45E-030.612.23E-030.65
15000.0161616.022.63E-051.63E-030.6552.53E-030.643
16000.015216.282.74E-051.80E-030.6972.82E-030.639
17000.014316.582.85E-051.99E-030.7423.13E-030.637
18000.013516.962.96E-052.19E-030.7863.44E-030.639
19000.012817.493.07E-052.40E-030.8353.73E-030.643
20000.012118.253.18E-052.63E-030.8783.98E-030.661

History

Main article:Timeline of hydrogen technologies

18th century

Robert Boyle, who discovered the reaction betweeniron filings and dilute acids

In 1671, Irish scientistRobert Boyle discovered and described the reaction betweeniron filings and diluteacids, which results in the production of hydrogen gas.[61][62]Boyle did not note that the gas was flammable, but hydrogen would play a key role in overturning thephlogiston theory of combustion.[63]

In 1766,Henry Cavendish was the first to recognize hydrogen gas as a discrete substance, by naming the gas from ametal-acid reaction "inflammable air". He speculated that "inflammable air" was in fact identical to the hypothetical substance "phlogiston"[64][65] and further finding in 1781 that the gas produces water when burned. He is usually given credit for the discovery of hydrogen as an element.[10][9]

Antoine Lavoisier, who identified the element that came to be known as hydrogen

In 1783,Antoine Lavoisier identified the element that came to be known as hydrogen[66] when he andLaplace reproduced Cavendish's finding that water is produced when hydrogen is burned.[9]Lavoisier produced hydrogen for his experiments onmass conservation by treating metalliciron with a stream of water through an incandescent iron tube heated in a fire. Anaerobicoxidation 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 react similarly with water, leading to the production of hydrogen.[67] In some situations, this H2-producing process is problematic, for instance in the case ofzirconium cladding onnuclear fuel rods.[68]

19th century

By 1806 hydrogen was used to fillballoons.[69]François Isaac de Rivaz built the firstde Rivaz engine, an internal combustion engine powered by a mixture of hydrogen and oxygen, in 1806.Edward Daniel Clarke invented the hydrogen gas blowpipe in 1819. TheDöbereiner's lamp andlimelight were invented in 1823. Hydrogen wasliquefied for the first time byJames Dewar in 1898 by usingregenerative cooling and his invention, thevacuum flask. He producedsolid hydrogen the next year.[9]

One of the firstquantum effects to be explicitly noticed, although not understood at the time, wasJames Clerk Maxwell's observation that thespecific heat capacity ofH2 unaccountably departs from that of adiatomic 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 inH2 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.[70]

20th century

The existence of thehydride anion was suggested byGilbert N. Lewis in 1916 forgroup 1 andgroup 2 salt-like compounds. In 1920,Moers electrolyzed moltenlithium hydride (LiH), producing astoichiometric quantity of hydrogen at theanode.[71]

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

Because of its simple atomic structure, consisting only of a proton and an electron, thehydrogen atom, together with thespectrum of light produced from it or absorbed by it, has been central to thedevelopment of the theory of atomic structure.[72] The energy levels of hydrogen can be calculated fairly accurately using theBohr model of the atom, in which the electron "orbits" the proton, like how Earth orbits the Sun. However, the electron and proton are held together byelectrostatic attraction, while planets and celestial objects are held bygravity. Due to thediscretization ofangular momentum postulated in earlyquantum mechanics byBohr, the electron in theBohr model can only occupy certain allowed distances from the proton, and therefore only certain allowed energies.[73]

Hydrogen's unique position as the only neutral atom for which theSchrödinger equation can be directly solved, has significantly contributed to the understanding of quantum mechanics through the exploration of its energetics.[74] Furthermore, study of the corresponding simplicity of the hydrogen molecule and the correspondingcation,H+2, brought understanding of the nature of thechemical bond, which followed shortly after the quantum mechanical treatment of the hydrogen atom had been developed in the mid-1920s.[75]

Hydrogen-lifted airship

Airship Hindenburg over New York
TheHindenburg overNew York City in 1937

BecauseH2 has only 7% the density of air, it was once widely used as alifting gas in balloons andairships.[76] The first hydrogen-filled balloon was invented byJacques Charles in 1783. Hydrogen provided the lift for the first reliable form of air-travel following the 1852 invention of the first hydrogen-lifted airship byHenri Giffard. German countFerdinand von Zeppelin promoted the idea of rigid airships lifted by hydrogen that later were calledZeppelins, the first of which had its maiden flight in 1900.[9] 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 in the form ofblimps were used as observation platforms and bombers during World War II, especially on theUS Eastern seaboard.[77]

The first non-stop transatlantic crossing was made by the British airship R34 in 1919 and regular passenger service resumed in the 1920s. Hydrogen was used in theHindenburg, which caught fire overNew Jersey on 6 May 1937.[9] The hydrogen that filled the airship was ignited, possibly by static electricity, and burst into flames.[78] Following thisdisaster, commercial hydrogen airship travelceased. Hydrogen is still used, in preference to non-flammable but more expensivehelium, as a lifting gas forweather balloons.[79]

Deuterium and tritium

Deuterium was discovered in December 1931 byHarold Urey, andtritium was prepared in 1934 byErnest Rutherford,Mark Oliphant, andPaul Harteck.[10]Heavy water, which consists of deuterium in the place of regular hydrogen, was discovered by Urey's group in 1932.[9]

Chemistry

Reactions of H2

Adihydrogen complex of iron, [HFe(H2)(dppe)2]+

H2 is relatively unreactive. The thermodynamic basis of this low reactivity is the very strongH–H bond, with abond dissociation energy of435.7 kJ/mol.[80] It does form coordination complexes calleddihydrogen complexes. These species provide insights into the early steps in the interactions of hydrogen with metal catalysts. According toneutron diffraction, the metal and two H atoms form a triangle in these complexes. TheH-H bond remains intact but is elongated. They are acidic.[81]

Although exotic on Earth, theH+3 ion is common in the universe. It is a triangular species, like the aforementioned dihydrogen complexes. It is known asprotonated molecular hydrogen or the trihydrogen cation.[82]

Hydrogen reacts withchlorine to produce HCl, and withbromine to produce HBr, via achain reaction. The reaction requires initiation. For example, in the case of Br2, the dibromine molecule is split apart:Br2 + (UV light) → 2Br•. Propagating reactions consume hydrogen molecules and produce HBr, as well as Br and H atoms:

Br• + H2 → HBr + H
H + Br2 → HBr +Br

Finally the terminating reaction:

H + HBr → H2 + Br•
2 Br• → Br2

consumes the remaining atoms.[83]: 289 

The addition of H2 tounsaturated organic compounds, such asalkenes andalkynes, is calledhydrogenation. Even if the reaction isenergetically favorable, it does not occur spontaneously even at higher temperatures. In the presence of acatalyst like finely dividedplatinum ornickel, the reaction proceeds at room temperature.[84]: 477 

Hydrogen-containing compounds

Main article:Hydrogen compounds

Hydrogen can exist in both +1 and −1 oxidation states, forming compounds throughionic andcovalent bonding. The element is part of a wide range of substances, including water,hydrocarbons, and numerous otherorganic compounds.[85] The H+ ion—commonly referred to as a proton due to its single proton and absence of electrons—is central toacid–base chemistry, although the proton does not move freely. In theBrønsted–Lowry framework, acids are defined by their ability to donate H+ ions to bases.[86]

Hydrogen forms a vast variety of compounds withcarbon, known as hydrocarbons, and an even greater diversity with other elements (heteroatoms), giving rise to the broad class of organic compounds often associated with living organisms.[85]

A sample ofsodium hydride

Hydrogen compounds with hydrogen in the oxidation state −1 are known ashydrides, which are usually formed between hydrogen and metals. The hydrides can be ionic (aka saline), covalent, or metallic. With heating, H2 reacts efficiently with thealkali andalkaline earth metals to give theionic hydrides of the formulas MH and MH2, respectively. These salt-like crystalline compounds have high melting points and all react with water to liberate hydrogen. Covalent hydrides includeboranes and polymericaluminium hydride.Transition metals formmetal hydrides via continuous dissolution of hydrogen into the metal.[87] A well-known hydride islithium aluminium hydride: the[AlH4] anion carries hydridic centers firmly attached to the Al(III).[88] Perhaps the most extensive series of hydrides are theboranes, compounds consisting only of boron and hydrogen.[89]

Hydrides can bond to theseelectropositive elements not only as a terminalligand but also asbridging ligands. In diborane (B2H6), four hydrogen atoms are terminal, while two bridge between the two boron atoms.[24]

Hydrogen bonding

Main article:Hydrogen bond

When bonded to a moreelectronegative element, particularlyfluorine,oxygen, ornitrogen, hydrogen can participate in a form of medium-strength noncovalent bonding with another electronegative element with alone pair like oxygen or nitrogen. This phenomenon, calledhydrogen bonding, is critical to the stability of many biological molecules.[90]: 375 [91] Hydrogen bonding alters molecule structures,viscosity,solubility, melting and boiling points, and evenprotein folding dynamics.[92]

Protons and acids

Further information:Acid–base reaction
An "A-Tbase pair" in DNA illustrating how hydrogen bonds are critical to thegenetic code. The drawing illustrates that in many chemical depictions,C-H bonds are not always shown explicitly, an indication of their pervasiveness.

In water, hydrogen bonding plays an important role in reaction thermodynamics. A hydrogen bond can shift over to proton transfer.Under theBrønsted–Lowry acid–base theory, acids are proton donors, while bases are proton acceptors.[93]: 28 A bare proton (H+) essentially cannot exist in anything other than a vacuum. Otherwise it attaches to other atoms, ions, or molecules. Even chemical species as inert asmethane can be protonated. The term "proton" is used loosely and metaphorically to refer to solvated hydrogencations attached to other solvated chemical species; it is denoted "H+" without any implication that any single protons exist freely in solution as a species. To avoid the implication of the naked proton in solution, acidic aqueous solutions are sometimes considered to contain the "hydronium ion" ([H3O]+), or still more accurately,[H9O4]+.[94] Otheroxonium ions are found when water is in acidic solution with other solvents.[95]

The concentration of these solvated protons determines thepH of a solution, alogarithmic scale that reflects its acidity or basicity. Lower pH values indicate higher concentrations of hydronium ions, corresponding to more acidic conditions.[96]

Occurrence

Cosmic

A white-green cotton-like clog on black background.
NGC 604, a giantregion of ionized hydrogen in theTriangulum Galaxy

Hydrogen, as atomic H, is the mostabundantchemical element in the universe, making up 75% ofnormal matter bymass.[97] and >90% by number of atoms.[98] In theearly universe, protonsformed in the first second after the Big Bang; neutral hydrogen atoms formed about 370,000 years later during therecombination epoch as the universe expanded and plasma had cooled enough for electrons to remain bound to protons.[99]

In astrophysics, neutral hydrogen in theinterstellar medium is calledH I and ionized hydrogen is calledH II.[100] Radiation from stars ionizes H I to H II, creatingspheres of ionized H II around stars. In thechronology of the universe neutral hydrogen dominated until the birth of stars during the era ofreionization, which then produced bubbles of ionized hydrogen that grew and merged over hundreds of millions of years.[101]These are the source of the 21-centimeterhydrogen line, at1420 MHz, that is detected in order to probe primordial hydrogen. The large amount of neutral hydrogen found in thedamped Lyman-alpha systems is thought to dominate thecosmologicalbaryonic density of the universe up to aredshift ofz = 4.[102]

Hydrogen is found in great abundance in stars andgas giant planets.Molecular clouds ofH2 are associated withstar formation. Hydrogen plays a vital role in poweringstars through theproton-proton reaction in lower-mass stars, and through theCNO cycle ofnuclear fusion in stars more massive than theSun.[103]

Protonated molecular hydrogen (H+3) is found in theinterstellar medium, where it is generated by ionization of molecular hydrogen bycosmic rays. This ion has also been observed in theupper atmosphere of Jupiter. The ion is long-lived in 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.[104] Neutraltriatomic hydrogenH3 can exist only in an excited form and is unstable.[105]

Terrestrial

Hydrogen is the third most abundant element on the Earth's surface,[106] mostly existing withinchemical compounds such ashydrocarbons and water.[24] Elemental hydrogen is normally in the form of a gas,H2, atstandard conditions. It is present in a very low concentration in Earth's atmosphere (around0.53 parts per million on amolar basis[107]) because of its light weight, which enables it toescape the atmosphere more rapidly than heavier gases. Despite its low concentration in the atmosphere, terrestrial hydrogen is sufficiently abundant to support the metabolism of several varieties of bacteria.[108]

Large underground deposits of hydrogen gas have been discovered in several countries includingMali,France andAustralia.[109] As of 2024, it is uncertain how much underground hydrogen can be extracted economically.[109]

Production and storage

Main article:Hydrogen production

Industrial routes

Nearly all of the world's current supply of hydrogen gas (H2) is produced from fossil fuels.[110][111]: 1  Many methods exist for producing H2, but three dominate commercially: steam reforming often coupled to water-gas shift, partial oxidation of hydrocarbons, and water electrolysis.[112]

Steam reforming

Inputs and outputs of steam reforming (SMR) and water gas shift (WGS) reaction of natural gas, a process used in hydrogen production

Hydrogen is mainly produced bysteam methane reforming (SMR), the reaction of water and methane.[113][114] Thus, at high temperature (1,000–1,400 K [730–1,130 °C; 1,340–2,060 °F]),steam (water vapor) reacts withmethane to yieldcarbon monoxide and H2.

CH4 + H2O → CO + 3 H2

Producing onetonne of hydrogen through this process emits6.6–9.3 tonnes of carbon dioxide.[115] The production of natural gas feedstock also produces emissions such asvented andfugitive methane, which further contributes to the overall carbon footprint of hydrogen.[116]

This reaction is favored at low pressures but is nonetheless conducted at high pressures (2.0 MPa [20 atm; 590 inHg]) because high-pressure H2 is the most marketable product, andpressure 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 ofmethanol and many other 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 ofcoke or carbon:

CH4 → C + 2 H2

Therefore, steam reforming typically employs an excess of H2O. Additional hydrogen can be recovered from the steam by using carbon monoxide through thewater gas shift reaction (WGS). This process requires aniron oxide catalyst:[114]

CO + H2O → CO2 + H2

Hydrogen is sometimes produced and consumed in the same industrial process, without being separated. In theHaber process forammonia production, hydrogen is generated from natural gas.[117]

Partial oxidation of hydrocarbons

Other methods for CO andH2 production include partial oxidation of hydrocarbons:[45]

2 CH4 + O2 → 2 CO + 4 H2

Although less important commercially, coal can serve as a prelude to the above shift reaction:[114]

C + H2O → CO + H2

Olefin production units may produce substantial quantities of byproduct hydrogen, particularly fromcracking light feedstocks likeethane orpropane.[118]

Water electrolysis

Inputs and outputs of the electrolysis of water production of hydrogen

Electrolysis of water is a conceptually simple method of producing hydrogen.

2 H2O(l) → 2 H2(g) + O2(g)

Commercialelectrolyzers usenickel-based catalysts in strongly alkaline solution.Platinum is a better catalyst but is expensive.[119] The hydrogen created through electrolysis using renewable energy is commonly referred to as "green hydrogen".[120]

Electrolysis ofbrine to yieldchlorine[121] also produces high-purity hydrogen as a co-product, which is used for a variety of transformations such ashydrogenations.[122]

The electrolysis process is more expensive than producing hydrogen from methane withoutcarbon capture and storage.[123]

Innovation inhydrogen electrolyzers could make large-scale production of hydrogen from electricity more cost-competitive.[124]

Methane pyrolysis

Hydrogen can be produced bypyrolysis ofnatural gas (methane), producing hydrogen gas and solid carbon with the aid of a catalyst and74 kJ/mol input heat:

CH4(g) → C(s) + 2 H2(g)H° = 74 kJ/mol)

The carbon may be sold as a manufacturing feedstock or fuel, or landfilled.This route could have a lower carbon footprint than existing hydrogen production processes, but mechanisms for removing the carbon and preventing it from reacting with the catalyst remain obstacles for industrial-scale use.[125]: 17 [126]

Thermochemical

Water splitting is the process by which water is decomposed into its components. Relevant to the biological scenario is this equation:

2 H2O → 4 H+ + O2 + 4 e

The reaction occurs in thelight-dependent reactions in allphotosynthetic organisms. A few organisms, including the algaChlamydomonas reinhardtii andcyanobacteria, have evolved a second step in thedark reactions in which protons and electrons are reduced to formH2 gas by specializedhydrogenases in thechloroplast.[127]

Efforts have been undertaken togenetically modify cyanobacterial hydrogenases to more efficiently generateH2 gas even in the presence of oxygen.[128] Efforts have also been undertaken with genetically‐modified alga in abioreactor.[129]

Relevant to the thermal water-splitting scenario is this simple equation:

2 H2O → 2 H2 + O2

Over 200 thermochemical cycles can be used forwater splitting. Many of these cycles such as theiron oxide cycle,cerium(IV) oxide–cerium(III) oxide cycle,zinc zinc-oxide cycle,sulfur-iodine cycle,copper-chlorine cycle andhybrid sulfur cycle have been evaluated for their commercial potential to produce hydrogen and oxygen from water and heat without using electricity.[130] A number of labs (including inFrance,Germany,Greece,Japan, and theUnited States) are developing thermochemical methods to produce hydrogen from solar energy and water.[131]

Natural routes

Biohydrogen

Further information:Biohydrogen

H2 is produced in organisms by enzymes calledhydrogenases. This process allows the host organism to usefermentation as a source of energy.[132] These same enzymes also canoxidize H2, such that the host organisms can subsist by reducing oxidized substrates using electrons extracted from H2.[133]

Hydrogenase enzymes featureiron ornickel-iron centers at theiractive sites.[134] The natural cycle of hydrogen production and consumption by organisms is called thehydrogen cycle.[135]

Some bacteria such asMycobacterium smegmatis can use the small amount of hydrogen in the atmosphere as a source of energy when other sources are lacking. Their hydrogenases feature small channels that exclude oxygen from the active site, permitting the reaction to occur even though the hydrogen concentration is very low and the oxygen concentration is as in normal air.[107][136]

Confirming the existence of hydrogenase‐employing microbesin the human gut,H2 occurs in human breath. The concentration in the breath of fasting people at rest is typically underparts per million (ppm), but can reach50 ppm when people with intestinal disorders consume molecules they cannot absorb during diagnostichydrogen breath tests.[137]

Serpentinization

Serpentinization is a geological mechanism which produces highly-reducing conditions.[138] Under these conditions, water is capable of oxidizingferrous (Fe2+
) ions infayalite, generating hydrogen gas:[139][140]

Fe2SiO4 + H2O → 2 Fe3O4 + SiO2 + H2

Closely related to this geological process is theSchikorr reaction:

3 Fe(OH)2 → Fe3O4 + 2 H2O + H2

This process also is relevant to the corrosion ofiron andsteel inoxygen-freegroundwater and inreducing soils below thewater table.[141]

Laboratory syntheses

H2 is produced in laboratory settings, such as in the small-scaleelectrolysis of water using metalelectrodes and water containing anelectrolyte, which liberates hydrogen gas at thecathode:[96]

2H+(aq) + 2 e → H2(g)

Hydrogen is also often a by-product of other reactions. Many metals react with water to produce H2, but the rate of hydrogen evolution depends on the metal, the pH, and the presence of alloying agents. Most often, hydrogen evolution is induced by acids. Thealkali andalkaline earth metals as well asaluminium,zinc,manganese, andiron, react readily with aqueous acids.[96]

Zn + 2 H+ → Zn2+ + H2

Many metals, such as aluminium, are slow to react with water because they formpassivated oxide coatings. An alloy of aluminium andgallium, however, does react with water. In high-pH solutions, aluminium can react with H2:[96]

2 Al + 6 H2O + 2 OH → 2 [Al(OH)4] + 3 H2

Storage

If H2 is to be used as an energy source, its storage is important. It dissolves only poorly in solvents. For example, atroom temperature and 0.1millipascals (9.9×10−10 atm),approx. 0.05 moles of hydrogen dissolve into one kilogram (2.2 lb) ofdiethyl ether.[87] H2 can be stored in compressed form, although compressing costs energy. Liquefaction is impractical given hydrogen's lowcritical temperature. In contrast, ammonia and many hydrocarbons can be liquified at room temperature under pressure. For these reasons, hydrogencarriers—materials that reversibly bind H2—have attracted much attention. The key question is then the weight percent of H2-equivalents within the carrier material. For example, hydrogen can be reversibly absorbed into manyrare earths andtransition metals[142] and is soluble in both nanocrystalline andamorphous metals.[143] Hydrogensolubility in metals is influenced by local distortions or impurities in thecrystal lattice.[144] These properties may be useful when hydrogen is purified by passage through hotpalladium disks, but the gas's high solubility is also a metallurgical problem, contributing to theembrittlement of many metals,[145] complicating the design of pipelines and storage tanks.[146]

The most problematic aspect of metal hydrides for storage is their modest H2 content, often on the order of 1%. For this reason, there is interest in storage of H2 in compounds of lowmolecular weight. For example,ammonia borane (H3N−BH3) contains 19.8 weight percent of H2. The problem with this material is that after release of H2, the resulting boron nitride does not re-add H2: i.e., ammonia borane is an irreversible hydrogen carrier.[147] More attractive arehydrocarbons such astetrahydroquinoline, which reversibly release some H2 when heated in the presence of a catalyst:[148]

C9H10NH ⇌ C9H7N + 2 H2

Applications

See also:Hydrogen economy
Hydrogen Ladder: Ranking of hydrogen applications and uses in the medium term, but analysts disagree[149]

Petrochemical industry

Large quantities ofH2 are used in the "upgrading" offossil fuels. Key consumers ofH2 includehydrodesulfurization andhydrocracking. Many of these reactions can be classified ashydrogenolysis, i.e., the cleavage of bonds by hydrogen. Illustrative is the separation ofsulfur from liquid fossil fuels:[112][150]

R2S + 2 H2 → H2S + 2 RH

Hydrogenation

Hydrogenation, the addition ofH2 to various substrates, is done on a large scale. Hydrogenation ofN2 produces ammonia by theHaber process:[150]

N2 + 3 H2 → 2 NH3

This process consumes a few percent of the energy budget in the entire industry and is the biggest consumer of hydrogen. The resulting ammonia is used extensively infertilizer production; these fertilizers have become essential feedstocks in modern agriculture.[151] Hydrogenation is also used to convertunsaturated fats andoils to saturated fats and oils. The major application is the production ofmargarine.Methanol is produced by hydrogenation of carbon dioxide; the mixture of hydrogen and carbon dioxide used for this process is known assyngas. It is similarly the source of hydrogen in the manufacture ofhydrochloric acid.H2 is also used as areducing agent for the conversion of someores to the metals.[152][96]

Fuel

The potential for using hydrogen (H2) as a fuel has been widely discussed. Hydrogen can be used infuel cells to produce electricity,[153] or burned to generate heat.[154] When hydrogen is consumed in fuel cells, the only emission at the point of use is water vapor.[154] When burned, hydrogen produces relatively little pollution at the point of combustion, but can lead to thermal formation of harmfulnitrogen oxides.[154]

If hydrogen is produced with low or zero greenhouse gas emissions (green hydrogen), it can play a significant role in decarbonizing energy systems where there are challenges and limitations to replacing fossil fuels with direct use of electricity.[155][123]

Hydrogen fuel can produce the intense heat required for industrial production of steel, cement, glass, and chemicals, thus contributing to the decarbonization of industry alongside other technologies, such aselectric arc furnaces for steelmaking.[156] However, it is likely to play a larger role in providing industrial feedstock for cleaner production of ammonia and organic chemicals.[155] For example, insteelmaking, hydrogen could function as a clean fuel and also as a low-carbon catalyst, replacing coal-derivedcoke (carbon):[157]

2FeO + C → 2Fe + CO2
vs
FeO + H2 → Fe + H2O

Hydrogen used to decarbonize transportation is likely to find its largest applications in shipping, aviation and, to a lesser extent, heavy goods vehicles, through the use of hydrogen-derived synthetic fuels such asammonia andmethanol and fuel cell technology.[155] For light-duty vehicles including cars, hydrogen is far behind otheralternative fuel vehicles, especially compared with the rate of adoption ofbattery electric vehicles, and may not play a significant role in future.[158]

A black inverted funnel with blue glow emerging from its opening.
ASpace Shuttle Main Engine burns hydrogen with oxygen, producing a nearly invisible flame at full thrust.

Liquid hydrogen andliquid oxygen together serve ascryogenic propellants inliquid-propellant rockets, as in theSpace Shuttle main engines.NASA has investigated the use ofrocket propellant made from atomic hydrogen, boron or carbon that is frozen into solid molecular hydrogen particles suspended in liquid helium. Upon warming, the mixture vaporizes to allow the atomic species to recombine, heating the mixture to high temperature.[159]

Hydrogen produced when there is a surplus ofvariable renewable electricity could in principle be stored and later used to generate heat or to re-generate electricity.[160] It can be further transformed intosynthetic fuels such asammonia andmethanol.[161] Disadvantages of hydrogen fuel include high costs of storage and distribution due to hydrogen's explosivity, its large volume compared to other fuels, and its tendency toembrittle materials.[116]

Nickel–hydrogen battery

The very long-lived, rechargeablenickel–hydrogen battery developed for satellite power systems uses pressurized gaseous H2.[162] TheInternational Space Station,[163]Mars Odyssey[164] and theMars Global Surveyor[165] are equipped with nickel-hydrogen batteries. In the dark part of its orbit, theHubble Space Telescope is also powered by nickel-hydrogen batteries, which were finally replaced in May 2009,[166] more than 19 years after launch and 13 years beyond their design life.[167]

Semiconductor industry

Hydrogen is employed insemiconductor manufacturing to saturate broken ("dangling") bonds ofamorphous silicon andamorphous carbon, which helps in stabilizing the materials' properties.[168] Hydrogen, introduced as an unintended side-effect of production, acts as a shallowelectron donor leading ton-type conductivity inZnO, with important uses intransducers andphosphors.[169][170] Detailed analysis of ZnO and ofMgO shows evidence of four and six-fold hydrogen multicentre bonds.[171]Thedoping behavior of hydrogen varies with material.[172][173]

Niche and evolving uses

Beyond than the uses mentioned above, hydrogen is used in smaller scales in the following applications:

Safety and precautions

Main article:Hydrogen safety
Hydrogen
Hazards
GHS labelling:
GHS02: Flammable
Danger
H220
P202,P210,P271,P377,P381,P403[185]
NFPA 704 (fire diamond)
Chemical compound

In hydrogen pipelines and steel storage vessels, hydrogen molecules are prone to reacting with metals, causinghydrogen embrittlement and leaks in the pipeline or storage vessel.[186] Since it is lighter than air, hydrogen does not easily accumulate to form a combustible gas mixture.[186] However, even without ignition sources, high-pressure hydrogen leakage may cause spontaneous combustion anddetonation.[186]

Hydrogen is flammable when mixed even in small amounts with air. Ignition can occur at avolumetric ratio of hydrogen to air as low as 4%.[187] In approximately 70% of hydrogen ignition accidents, the ignition source cannot be found, and it is widely believed by scholars that spontaneous ignition of hydrogen occurs.[186]

Hydrogen fire, while being extremely hot, is almost invisible to the human eye, and thus can lead to accidental burns.[44] Hydrogen is non-toxic,[188] but like most gasesit can cause asphyxiation in the absence of adequate ventilation.[189]

See also

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