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Oxygen, ₈O

Liquid oxygen boiling (O2)
Oxygen
Allotropes	O2, O3 (ozone) and more (see Allotropes of oxygen)
Appearance	gas: colorless liquid and solid: pale blue
Standard atomic weight Ar°(O)	[15.99903, 15.99977] 15.999±0.001 (abridged)[1]
Abundance
in the Earth’s crust	461000 ppm
Oxygen 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 – ↑ O ↓ S nitrogen ← oxygen → fluorine
Atomic number (Z)	8
Group	group 16 (chalcogens)
Period	period 2
Block	p-block
Electron configuration	[He] 2s2 2p4
Electrons per shell	2, 6
Physical properties
Phase at STP	gas
Melting point	(O2) 54.36 K ​(−218.79 °C, ​−361.82 °F)
Boiling point	(O2) 90.188 K ​(−182.962 °C, ​−297.332 °F)
Density (at STP)	1.429 g/L
when liquid (at b.p.)	1.141 g/cm3
Triple point	54.361 K, ​0.1463 kPa
Critical point	154.581 K, 5.043 MPa
Heat of fusion	(O2) 0.444 kJ/mol
Heat of vaporization	(O2) 6.82 kJ/mol
Molar heat capacity	(O2) 29.378 J/(mol·K)
Vapor pressure P (Pa) 1 10 100 1 k 10 k 100 k at T (K)       61 73 90
Atomic properties
Oxidation states	−2, −1, 0, +1, +2
Electronegativity	Pauling scale: 3.44
Ionization energies	1st: 1313.9 kJ/mol 2nd: 3388.3 kJ/mol 3rd: 5300.5 kJ/mol (more)
Covalent radius	66±2 pm
Van der Waals radius	152 pm
Spectral lines of oxygen
Other properties
Natural occurrence	primordial
Crystal structure	​cubic
Speed of sound	330 m/s (gas, at 27 °C)
Thermal conductivity	26.58×10−3  W/(m⋅K)
Magnetic ordering	paramagnetic
Molar magnetic susceptibility	+3449.0×10−6 cm3/mol (293 K)[2]
CAS Number	7782-44-7
History
Discovery	Carl Wilhelm Scheele (1771)
Named by	Antoine Lavoisier (1777)
Main isotopes of oxygen v e
Iso­tope Decay abun­dance half-life (t1/2) mode pro­duct 16O [99.738%, 99.776%] stable 17O [0.0367%, 0.0400%] stable 18O [0.187%, 0.222%] stable
Category: Oxygen view talk edit | references

Oxygen is the chemical element with the symbol O and atomic number 8. It is a member of the chalcogen group in the periodic table, a highly reactive nonmetal, and an oxidizing agent that readily forms oxides with most elements as well as with other compounds. Oxygen is Earth’s most abundant element, and after hydrogen and helium, it is the third-most abundant element in the universe. At standard temperature and pressure, two atoms of the element bind to form dioxygen, a colorless and odorless diatomic gas with the formula O
₂. Diatomic oxygen gas currently constitutes 20.95% of the Earth’s atmosphere, though this has changed considerably over long periods of time. Oxygen makes up almost half of the Earth’s crust in the form of oxides.^[3]

Many major classes of organic molecules in living organisms contain oxygen atoms, such as proteins, nucleic acids, carbohydrates, and fats, as do the major constituent inorganic compounds of animal shells, teeth, and bone. Most of the mass of living organisms is oxygen as a component of water, the major constituent of lifeforms. Oxygen is continuously replenished in Earth’s atmosphere by photosynthesis, which uses the energy of sunlight to produce oxygen from water and carbon dioxide. Oxygen is too chemically reactive to remain a free element in air without being continuously replenished by the photosynthetic action of living organisms. Another form (allotrope) of oxygen, ozone (O
₃), strongly absorbs ultraviolet UVB radiation and the high-altitude ozone layer helps protect the biosphere from ultraviolet radiation. However, ozone present at the surface is a byproduct of smog and thus a pollutant.

Oxygen was isolated by Michael Sendivogius before 1604, but it is commonly believed that the element was discovered independently by Carl Wilhelm Scheele, in Uppsala, in 1773 or earlier, and Joseph Priestley in Wiltshire, in 1774. Priority is often given for Priestley because his work was published first. Priestley, however, called oxygen «dephlogisticated air», and did not recognize it as a chemical element. The name oxygen was coined in 1777 by Antoine Lavoisier, who first recognized oxygen as a chemical element and correctly characterized the role it plays in combustion.

Common uses of oxygen include production of steel, plastics and textiles, brazing, welding and cutting of steels and other metals, rocket propellant, oxygen therapy, and life support systems in aircraft, submarines, spaceflight and diving.

History of study

Early experiments

One of the first known experiments on the relationship between combustion and air was conducted by the 2nd century BCE Greek writer on mechanics, Philo of Byzantium. In his work Pneumatica, Philo observed that inverting a vessel over a burning candle and surrounding the vessel’s neck with water resulted in some water rising into the neck.^[4] Philo incorrectly surmised that parts of the air in the vessel were converted into the classical element fire and thus were able to escape through pores in the glass. Many centuries later Leonardo da Vinci built on Philo’s work by observing that a portion of air is consumed during combustion and respiration.^[5]

In the late 17th century, Robert Boyle proved that air is necessary for combustion. English chemist John Mayow (1641–1679) refined this work by showing that fire requires only a part of air that he called spiritus nitroaereus.^[6] In one experiment, he found that placing either a mouse or a lit candle in a closed container over water caused the water to rise and replace one-fourteenth of the air’s volume before extinguishing the subjects.^[7] From this, he surmised that nitroaereus is consumed in both respiration and combustion.

Mayow observed that antimony increased in weight when heated, and inferred that the nitroaereus must have combined with it.^[6] He also thought that the lungs separate nitroaereus from air and pass it into the blood and that animal heat and muscle movement result from the reaction of nitroaereus with certain substances in the body.^[6] Accounts of these and other experiments and ideas were published in 1668 in his work Tractatus duo in the tract «De respiratione».^[7]

Phlogiston theory

Robert Hooke, Ole Borch, Mikhail Lomonosov, and Pierre Bayen all produced oxygen in experiments in the 17th and the 18th century but none of them recognized it as a chemical element.^[8] This may have been in part due to the prevalence of the philosophy of combustion and corrosion called the phlogiston theory, which was then the favored explanation of those processes.^[9]

Established in 1667 by the German alchemist J. J. Becher, and modified by the chemist Georg Ernst Stahl by 1731,^[10] phlogiston theory stated that all combustible materials were made of two parts. One part, called phlogiston, was given off when the substance containing it was burned, while the dephlogisticated part was thought to be its true form, or calx.^[5]

Highly combustible materials that leave little residue, such as wood or coal, were thought to be made mostly of phlogiston; non-combustible substances that corrode, such as iron, contained very little. Air did not play a role in phlogiston theory, nor were any initial quantitative experiments conducted to test the idea; instead, it was based on observations of what happens when something burns, that most common objects appear to become lighter and seem to lose something in the process.^[5]

Discovery

Polish alchemist, philosopher, and physician Michael Sendivogius (Michał Sędziwój) in his work De Lapide Philosophorum Tractatus duodecim e naturae fonte et manuali experientia depromti (1604) described a substance contained in air, referring to it as ‘cibus vitae’ (food of life,^[11]) and according to Polish historian Roman Bugaj, this substance is identical with oxygen.^[12] Sendivogius, during his experiments performed between 1598 and 1604, properly recognized that the substance is equivalent to the gaseous byproduct released by the thermal decomposition of potassium nitrate. In Bugaj’s view, the isolation of oxygen and the proper association of the substance to that part of air which is required for life, provides sufficient evidence for the discovery of oxygen by Sendivogius.^[12] This discovery of Sendivogius was however frequently denied by the generations of scientists and chemists which succeeded him.^[11]

It is also commonly claimed that oxygen was first discovered by Swedish pharmacist Carl Wilhelm Scheele. He had produced oxygen gas by heating mercuric oxide (HgO) and various nitrates in 1771–72.^[13][14][5] Scheele called the gas «fire air» because it was then the only known agent to support combustion. He wrote an account of this discovery in a manuscript titled Treatise on Air and Fire, which he sent to his publisher in 1775. That document was published in 1777.^[15]

In the meantime, on August 1, 1774, an experiment conducted by the British clergyman Joseph Priestley focused sunlight on mercuric oxide contained in a glass tube, which liberated a gas he named «dephlogisticated air».^[14] He noted that candles burned brighter in the gas and that a mouse was more active and lived longer while breathing it. After breathing the gas himself, Priestley wrote: «The feeling of it to my lungs was not sensibly different from that of common air, but I fancied that my breast felt peculiarly light and easy for some time afterwards.»^[8] Priestley published his findings in 1775 in a paper titled «An Account of Further Discoveries in Air», which was included in the second volume of his book titled Experiments and Observations on Different Kinds of Air.^[5][16] Because he published his findings first, Priestley is usually given priority in the discovery.

The French chemist Antoine Laurent Lavoisier later claimed to have discovered the new substance independently. Priestley visited Lavoisier in October 1774 and told him about his experiment and how he liberated the new gas. Scheele had also dispatched a letter to Lavoisier on September 30, 1774, which described his discovery of the previously unknown substance, but Lavoisier never acknowledged receiving it. (A copy of the letter was found in Scheele’s belongings after his death.)^[15]

Lavoisier’s contribution

Lavoisier conducted the first adequate quantitative experiments on oxidation and gave the first correct explanation of how combustion works.^[14] He used these and similar experiments, all started in 1774, to discredit the phlogiston theory and to prove that the substance discovered by Priestley and Scheele was a chemical element.

In one experiment, Lavoisier observed that there was no overall increase in weight when tin and air were heated in a closed container.^[14] He noted that air rushed in when he opened the container, which indicated that part of the trapped air had been consumed. He also noted that the tin had increased in weight and that increase was the same as the weight of the air that rushed back in. This and other experiments on combustion were documented in his book Sur la combustion en général, which was published in 1777.^[14] In that work, he proved that air is a mixture of two gases; ‘vital air’, which is essential to combustion and respiration, and azote (Gk. ἄζωτον «lifeless»), which did not support either. Azote later became nitrogen in English, although it has kept the earlier name in French and several other European languages.^[14]

Etymology

Lavoisier renamed ‘vital air’ to oxygène in 1777 from the Greek roots ὀξύς (oxys) (acid, literally «sharp», from the taste of acids) and -γενής (-genēs) (producer, literally begetter), because he mistakenly believed that oxygen was a constituent of all acids.^[17] Chemists (such as Sir Humphry Davy in 1812) eventually determined that Lavoisier was wrong in this regard, but by then the name was too well established.^[18]

Oxygen entered the English language despite opposition by English scientists and the fact that the Englishman Priestley had first isolated the gas and written about it. This is partly due to a poem praising the gas titled «Oxygen» in the popular book The Botanic Garden (1791) by Erasmus Darwin, grandfather of Charles Darwin.^[15]

Later history

John Dalton’s original atomic hypothesis presumed that all elements were monatomic and that the atoms in compounds would normally have the simplest atomic ratios with respect to one another. For example, Dalton assumed that water’s formula was HO, leading to the conclusion that the atomic mass of oxygen was 8 times that of hydrogen, instead of the modern value of about 16.^[19] In 1805, Joseph Louis Gay-Lussac and Alexander von Humboldt showed that water is formed of two volumes of hydrogen and one volume of oxygen; and by 1811 Amedeo Avogadro had arrived at the correct interpretation of water’s composition, based on what is now called Avogadro’s law and the diatomic elemental molecules in those gases.^[20][a]

The first commercial method of producing oxygen was chemical, the so-called Brin process involving a reversible reaction of barium oxide. It was invented in 1852 and commercialized in 1884, but was displaced by newer methods in early 20th century.

By the late 19th century scientists realized that air could be liquefied and its components isolated by compressing and cooling it. Using a cascade method, Swiss chemist and physicist Raoul Pierre Pictet evaporated liquid sulfur dioxide in order to liquefy carbon dioxide, which in turn was evaporated to cool oxygen gas enough to liquefy it. He sent a telegram on December 22, 1877, to the French Academy of Sciences in Paris announcing his discovery of liquid oxygen.^[21] Just two days later, French physicist Louis Paul Cailletet announced his own method of liquefying molecular oxygen.^[21] Only a few drops of the liquid were produced in each case and no meaningful analysis could be conducted. Oxygen was liquefied in a stable state for the first time on March 29, 1883, by Polish scientists from Jagiellonian University, Zygmunt Wróblewski and Karol Olszewski.^[22]

In 1891 Scottish chemist James Dewar was able to produce enough liquid oxygen for study.^[23] The first commercially viable process for producing liquid oxygen was independently developed in 1895 by German engineer Carl von Linde and British engineer William Hampson. Both men lowered the temperature of air until it liquefied and then distilled the component gases by boiling them off one at a time and capturing them separately.^[24] Later, in 1901, oxyacetylene welding was demonstrated for the first time by burning a mixture of acetylene and compressed O
₂. This method of welding and cutting metal later became common.^[24]

In 1923, the American scientist Robert H. Goddard became the first person to develop a rocket engine that burned liquid fuel; the engine used gasoline for fuel and liquid oxygen as the oxidizer. Goddard successfully flew a small liquid-fueled rocket 56 m at 97 km/h on March 16, 1926, in Auburn, Massachusetts, US.^[24][25]

In academic laboratories, oxygen can be prepared by heating together potassium chlorate mixed with a small proportion of manganese dioxide.^[26]

Oxygen levels in the atmosphere are trending slightly downward globally, possibly because of fossil-fuel burning.^[27]

Characteristics

Properties and molecular structure

At standard temperature and pressure, oxygen is a colorless, odorless, and tasteless gas with the molecular formula O
₂, referred to as dioxygen.^[29]

As dioxygen, two oxygen atoms are chemically bound to each other. The bond can be variously described based on level of theory, but is reasonably and simply described as a covalent double bond that results from the filling of molecular orbitals formed from the atomic orbitals of the individual oxygen atoms, the filling of which results in a bond order of two. More specifically, the double bond is the result of sequential, low-to-high energy, or Aufbau, filling of orbitals, and the resulting cancellation of contributions from the 2s electrons, after sequential filling of the low σ and σ^* orbitals; σ overlap of the two atomic 2p orbitals that lie along the O–O molecular axis and π overlap of two pairs of atomic 2p orbitals perpendicular to the O–O molecular axis, and then cancellation of contributions from the remaining two 2p electrons after their partial filling of the π^* orbitals.^[28]

This combination of cancellations and σ and π overlaps results in dioxygen’s double-bond character and reactivity, and a triplet electronic ground state. An electron configuration with two unpaired electrons, as is found in dioxygen orbitals (see the filled π* orbitals in the diagram) that are of equal energy—i.e., degenerate—is a configuration termed a spin triplet state. Hence, the ground state of the O
₂ molecule is referred to as triplet oxygen.^[30][b] The highest-energy, partially filled orbitals are antibonding, and so their filling weakens the bond order from three to two. Because of its unpaired electrons, triplet oxygen reacts only slowly with most organic molecules, which have paired electron spins; this prevents spontaneous combustion.^[31]

In the triplet form, O
₂ molecules are paramagnetic. That is, they impart magnetic character to oxygen when it is in the presence of a magnetic field, because of the spin magnetic moments of the unpaired electrons in the molecule, and the negative exchange energy between neighboring O
₂ molecules.^[23] Liquid oxygen is so magnetic that, in laboratory demonstrations, a bridge of liquid oxygen may be supported against its own weight between the poles of a powerful magnet.^[32][c]

Singlet oxygen is a name given to several higher-energy species of molecular O
₂ in which all the electron spins are paired. It is much more reactive with common organic molecules than is normal (triplet) molecular oxygen. In nature, singlet oxygen is commonly formed from water during photosynthesis, using the energy of sunlight.^[33] It is also produced in the troposphere by the photolysis of ozone by light of short wavelength^[34] and by the immune system as a source of active oxygen.^[35] Carotenoids in photosynthetic organisms (and possibly animals) play a major role in absorbing energy from singlet oxygen and converting it to the unexcited ground state before it can cause harm to tissues.^[36]

Allotropes

The common allotrope of elemental oxygen on Earth is called dioxygen, O
₂, the major part of the Earth’s atmospheric oxygen (see Occurrence). O₂ has a bond length of 121 pm and a bond energy of 498 kJ/mol.^[37] O₂ is used by complex forms of life, such as animals, in cellular respiration. Other aspects of O
₂ are covered in the remainder of this article.

Trioxygen (O
₃) is usually known as ozone and is a very reactive allotrope of oxygen that is damaging to lung tissue.^[38] Ozone is produced in the upper atmosphere when O
₂ combines with atomic oxygen made by the splitting of O
₂ by ultraviolet (UV) radiation.^[17] Since ozone absorbs strongly in the UV region of the spectrum, the ozone layer of the upper atmosphere functions as a protective radiation shield for the planet.^[17] Near the Earth’s surface, it is a pollutant formed as a by-product of automobile exhaust.^[38] At low earth orbit altitudes, sufficient atomic oxygen is present to cause corrosion of spacecraft.^[39]

The metastable molecule tetraoxygen (O
₄) was discovered in 2001,^[40][41] and was assumed to exist in one of the six phases of solid oxygen. It was proven in 2006 that this phase, created by pressurizing O
₂ to 20 GPa, is in fact a rhombohedral O
₈ cluster.^[42] This cluster has the potential to be a much more powerful oxidizer than either O
₂ or O
₃ and may therefore be used in rocket fuel.^[40][41] A metallic phase was discovered in 1990 when solid oxygen is subjected to a pressure of above 96 GPa^[43] and it was shown in 1998 that at very low temperatures, this phase becomes superconducting.^[44]

Physical properties

Oxygen dissolves more readily in water than in nitrogen, and in freshwater more readily than in seawater. Water in equilibrium with air contains approximately 1 molecule of dissolved O
₂ for every 2 molecules of N
₂ (1:2), compared with an atmospheric ratio of approximately 1:4. The solubility of oxygen in water is temperature-dependent, and about twice as much (14.6 mg/L) dissolves at 0 °C than at 20 °C (7.6 mg/L).^[8][45] At 25 °C and 1 standard atmosphere (101.3 kPa) of air, freshwater can dissolve about 6.04 milliliters (mL) of oxygen per liter, and seawater contains about 4.95 mL per liter.^[46] At 5 °C the solubility increases to 9.0 mL (50% more than at 25 °C) per liter for freshwater and 7.2 mL (45% more) per liter for sea water.

Oxygen gas dissolved in water at sea-level

	5 °C	25 °C
Freshwater	9.00	6.04
Seawater	7.20	4.95

(milliliters per liter)

Oxygen condenses at 90.20 K (−182.95 °C, −297.31 °F) and freezes at 54.36 K (−218.79 °C, −361.82 °F).^[47] Both liquid and solid O
₂ are clear substances with a light sky-blue color caused by absorption in the red (in contrast with the blue color of the sky, which is due to Rayleigh scattering of blue light). High-purity liquid O
₂ is usually obtained by the fractional distillation of liquefied air.^[48] Liquid oxygen may also be condensed from air using liquid nitrogen as a coolant.^[49]

Liquid oxygen is a highly reactive substance and must be segregated from combustible materials.^[49]

The spectroscopy of molecular oxygen is associated with the atmospheric processes of aurora and airglow.^[50] The absorption in the Herzberg continuum and Schumann–Runge bands in the ultraviolet produces atomic oxygen that is important in the chemistry of the middle atmosphere.^[51] Excited-state singlet molecular oxygen is responsible for red chemiluminescence in solution.^[52]

Table of thermal and physical properties of oxygen (O2) at atmospheric pressure:^[53][54]

Temperature (K)	Density (kg/m^3)	Specific heat (kJ/kg °C)	Dynamic viscosity (kg/m s)	Kinematic viscosity (m^2/s)	Thermal conductivity (W/m °C)	Thermal diffusivity (m^2/s)	Prandtl Number
100	3.945	0.962	7.64E-06	1.94E-06	0.00925	2.44E-06	0.796
150	2.585	0.921	1.15E-05	4.44E-06	0.0138	5.80E-06	0.766
200	1.93	0.915	1.48E-05	7.64E-06	0.0183	1.04E-05	0.737
250	1.542	0.915	1.79E-05	1.16E-05	0.0226	1.60E-05	0.723
300	1.284	0.92	2.07E-05	1.61E-05	0.0268	2.27E-05	0.711
350	1.1	0.929	2.34E-05	2.12E-05	0.0296	2.90E-05	0.733
400	0.962	1.0408	2.58E-05	2.68E-05	0.033	3.64E-05	0.737
450	0.8554	0.956	2.81E-05	3.29E-05	0.0363	4.44E-05	0.741
500	0.7698	0.972	3.03E-05	3.94E-05	0.0412	5.51E-05	0.716
550	0.6998	0.988	3.24E-05	4.63E-05	0.0441	6.38E-05	0.726
600	0.6414	1.003	3.44E-05	5.36E-05	0.0473	7.35E-05	0.729
700	0.5498	1.031	3.81E-05	6.93E-05	0.0528	9.31E-05	0.744
800	0.481	1.054	4.15E-05	8.63E-05	0.0589	1.16E-04	0.743
900	0.4275	1.074	4.47E-05	1.05E-04	0.0649	1.41E-04	0.74
1000	0.3848	1.09	4.77E-05	1.24E-04	0.071	1.69E-04	0.733
1100	0.3498	1.103	5.06E-05	1.45E-04	0.0758	1.96E-04	0.736
1200	0.3206	1.0408	5.33E-05	1.661E-04	0.0819	2.29E-04	0.725
1300	0.296	1.125	5.88E-05	1.99E-04	0.0871	2.62E-04	0.721

Isotopes and stellar origin

Naturally occurring oxygen is composed of three stable isotopes, ¹⁶O, ¹⁷O, and ¹⁸O, with ¹⁶O being the most abundant (99.762% natural abundance).^[55]

Most ¹⁶O is synthesized at the end of the helium fusion process in massive stars but some is made in the neon burning process.^{[56] 17}O is primarily made by the burning of hydrogen into helium during the CNO cycle, making it a common isotope in the hydrogen burning zones of stars.^[56] Most ¹⁸O is produced when ¹⁴N (made abundant from CNO burning) captures a ⁴He nucleus, making ¹⁸O common in the helium-rich zones of evolved, massive stars.^[56]

Thirteen radioisotopes have been characterized, ranging from ¹¹O to ²⁶O.^[57] The most stable are ¹⁵O with a half-life of 122.24 seconds and ¹⁴O with a half-life of 70.606 seconds.^[55] All of the remaining radioactive isotopes have half-lives that are less than 27 s and the majority of these have half-lives that are less than 83 milliseconds.^[55] The most common decay mode of the isotopes lighter than ¹⁶O is β⁺ decay^[58][59][60] to yield nitrogen, and the most common mode for the isotopes heavier than ¹⁸O is beta decay to yield fluorine.^[55]

Occurrence

Ten most common elements in the Milky Way Galaxy estimated spectroscopically^[61]

Z	Element	Mass fraction in parts per million
1	Hydrogen	739,000	71 × mass of oxygen (red bar)
2	Helium	240,000	23 × mass of oxygen (red bar)
8	Oxygen	10,400
6	Carbon	4,600
10	Neon	1,340
26	Iron	1,090
7	Nitrogen	960
14	Silicon	650
12	Magnesium	580
16	Sulfur	440

Oxygen is the most abundant chemical element by mass in the Earth’s biosphere, air, sea and land. Oxygen is the third most abundant chemical element in the universe, after hydrogen and helium.^[62] About 0.9% of the Sun’s mass is oxygen.^[14] Oxygen constitutes 49.2% of the Earth’s crust by mass^[63] as part of oxide compounds such as silicon dioxide and is the most abundant element by mass in the Earth’s crust. It is also the major component of the world’s oceans (88.8% by mass).^[14] Oxygen gas is the second most common component of the Earth’s atmosphere, taking up 20.8% of its volume and 23.1% of its mass (some 10¹⁵ tonnes).^[14][64][d] Earth is unusual among the planets of the Solar System in having such a high concentration of oxygen gas in its atmosphere: Mars (with 0.1% O
₂ by volume) and Venus have much less. The O
₂ surrounding those planets is produced solely by the action of ultraviolet radiation on oxygen-containing molecules such as carbon dioxide.

The unusually high concentration of oxygen gas on Earth is the result of the oxygen cycle. This biogeochemical cycle describes the movement of oxygen within and between its three main reservoirs on Earth: the atmosphere, the biosphere, and the lithosphere. The main driving factor of the oxygen cycle is photosynthesis, which is responsible for modern Earth’s atmosphere. Photosynthesis releases oxygen into the atmosphere, while respiration, decay, and combustion remove it from the atmosphere. In the present equilibrium, production and consumption occur at the same rate.^[65]

Free oxygen also occurs in solution in the world’s water bodies. The increased solubility of O
₂ at lower temperatures (see Physical properties) has important implications for ocean life, as polar oceans support a much higher density of life due to their higher oxygen content.^[66] Water polluted with plant nutrients such as nitrates or phosphates may stimulate growth of algae by a process called eutrophication and the decay of these organisms and other biomaterials may reduce the O
₂ content in eutrophic water bodies. Scientists assess this aspect of water quality by measuring the water’s biochemical oxygen demand, or the amount of O
₂ needed to restore it to a normal concentration.^[67]

Analysis

Paleoclimatologists measure the ratio of oxygen-18 and oxygen-16 in the shells and skeletons of marine organisms to determine the climate millions of years ago (see oxygen isotope ratio cycle). Seawater molecules that contain the lighter isotope, oxygen-16, evaporate at a slightly faster rate than water molecules containing the 12% heavier oxygen-18, and this disparity increases at lower temperatures.^[68] During periods of lower global temperatures, snow and rain from that evaporated water tends to be higher in oxygen-16, and the seawater left behind tends to be higher in oxygen-18. Marine organisms then incorporate more oxygen-18 into their skeletons and shells than they would in a warmer climate.^[68] Paleoclimatologists also directly measure this ratio in the water molecules of ice core samples as old as hundreds of thousands of years.

Planetary geologists have measured the relative quantities of oxygen isotopes in samples from the Earth, the Moon, Mars, and meteorites, but were long unable to obtain reference values for the isotope ratios in the Sun, believed to be the same as those of the primordial solar nebula. Analysis of a silicon wafer exposed to the solar wind in space and returned by the crashed Genesis spacecraft has shown that the Sun has a higher proportion of oxygen-16 than does the Earth. The measurement implies that an unknown process depleted oxygen-16 from the Sun’s disk of protoplanetary material prior to the coalescence of dust grains that formed the Earth.^[69]

Oxygen presents two spectrophotometric absorption bands peaking at the wavelengths 687 and 760 nm. Some remote sensing scientists have proposed using the measurement of the radiance coming from vegetation canopies in those bands to characterize plant health status from a satellite platform.^[70] This approach exploits the fact that in those bands it is possible to discriminate the vegetation’s reflectance from its fluorescence, which is much weaker. The measurement is technically difficult owing to the low signal-to-noise ratio and the physical structure of vegetation; but it has been proposed as a possible method of monitoring the carbon cycle from satellites on a global scale.

Biological production and role of O₂

Photosynthesis and respiration

In nature, free oxygen is produced by the light-driven splitting of water during oxygenic photosynthesis. According to some estimates, green algae and cyanobacteria in marine environments provide about 70% of the free oxygen produced on Earth, and the rest is produced by terrestrial plants.^[71] Other estimates of the oceanic contribution to atmospheric oxygen are higher, while some estimates are lower, suggesting oceans produce ~45% of Earth’s atmospheric oxygen each year.^[72]

A simplified overall formula for photosynthesis is^[73]

6 CO₂ + 6 H
₂O + photons → C
₆H
₁₂O
₆ + 6 O
₂

or simply

carbon dioxide + water + sunlight → glucose + dioxygen

Photolytic oxygen evolution occurs in the thylakoid membranes of photosynthetic organisms and requires the energy of four photons.^[e] Many steps are involved, but the result is the formation of a proton gradient across the thylakoid membrane, which is used to synthesize adenosine triphosphate (ATP) via photophosphorylation.^[74] The O
₂ remaining (after production of the water molecule) is released into the atmosphere.^[f]

Oxygen is used in mitochondria in the generation of ATP during oxidative phosphorylation. The reaction for aerobic respiration is essentially the reverse of photosynthesis and is simplified as

C
₆H
₁₂O
₆ + 6 O
₂ → 6 CO₂ + 6 H
₂O + 2880 kJ/mol

In vertebrates, O
₂ diffuses through membranes in the lungs and into red blood cells. Hemoglobin binds O
₂, changing color from bluish red to bright red^[38] (CO
₂ is released from another part of hemoglobin through the Bohr effect). Other animals use hemocyanin (molluscs and some arthropods) or hemerythrin (spiders and lobsters).^[64] A liter of blood can dissolve 200 cm³ of O
₂.^[64]

Until the discovery of anaerobic metazoa,^[75] oxygen was thought to be a requirement for all complex life.^[76]

Reactive oxygen species, such as superoxide ion (O⁻
₂) and hydrogen peroxide (H
₂O
₂), are reactive by-products of oxygen use in organisms.^[64] Parts of the immune system of higher organisms create peroxide, superoxide, and singlet oxygen to destroy invading microbes. Reactive oxygen species also play an important role in the hypersensitive response of plants against pathogen attack.^[74] Oxygen is damaging to obligately anaerobic organisms, which were the dominant form of early life on Earth until O
₂ began to accumulate in the atmosphere about 2.5 billion years ago during the Great Oxygenation Event, about a billion years after the first appearance of these organisms.^[77][78]

An adult human at rest inhales 1.8 to 2.4 grams of oxygen per minute.^[79] This amounts to more than 6 billion tonnes of oxygen inhaled by humanity per year.^[g]

Living organisms

Partial pressures of oxygen in the human body (PO₂

Unit	Alveolar pulmonary gas pressures	Arterial blood oxygen	Venous blood gas
kPa	14.2	11[h]-13[h]	4.0[h]-5.3[h]
mmHg	107	75[80]-100[80]	30[81]-40[81]

)

The free oxygen partial pressure in the body of a living vertebrate organism is highest in the respiratory system, and decreases along any arterial system, peripheral tissues, and venous system, respectively. Partial pressure is the pressure that oxygen would have if it alone occupied the volume.^[82]

Build-up in the atmosphere

Free oxygen gas was almost nonexistent in Earth’s atmosphere before photosynthetic archaea and bacteria evolved, probably about 3.5 billion years ago. Free oxygen first appeared in significant quantities during the Paleoproterozoic eon (between 3.0 and 2.3 billion years ago).^[83] Even if there was much dissolved iron in the oceans when oxygenic photosynthesis was getting more common, it appears the banded iron formations were created by anoxyenic or micro-aerophilic iron-oxidizing bacteria which dominated the deeper areas of the photic zone, while oxygen-producing cyanobacteria covered the shallows.^[84] Free oxygen began to outgas from the oceans 3–2.7 billion years ago, reaching 10% of its present level around 1.7 billion years ago.^[83][85]

The presence of large amounts of dissolved and free oxygen in the oceans and atmosphere may have driven most of the extant anaerobic organisms to extinction during the Great Oxygenation Event (oxygen catastrophe) about 2.4 billion years ago. Cellular respiration using O
₂ enables aerobic organisms to produce much more ATP than anaerobic organisms.^[86] Cellular respiration of O
₂ occurs in all eukaryotes, including all complex multicellular organisms such as plants and animals.

Since the beginning of the Cambrian period 540 million years ago, atmospheric O
₂ levels have fluctuated between 15% and 30% by volume.^[87] Towards the end of the Carboniferous period (about 300 million years ago) atmospheric O
₂ levels reached a maximum of 35% by volume,^[87] which may have contributed to the large size of insects and amphibians at this time.^[88]

Variations in atmospheric oxygen concentration have shaped past climates. When oxygen declined, atmospheric density dropped, which in turn increased surface evaporation, causing precipitation increases and warmer temperatures.^[89]

At the current rate of photosynthesis it would take about 2,000 years to regenerate the entire O
₂ in the present atmosphere.^[90]

In the field of astrobiology and in the search for extraterrestrial life oxygen is a strong biosignature. That said it might not be a definite biosignature, being possibly produced abiotically on celestial bodies with processes and conditions (such as a peculiar hydrosphere) which allow free oxygen,^[91][92][93] like with Europa’s and Ganymede’s thin
oxygen atmospheres.^[94]

Industrial production

One hundred million tonnes of O
₂ are extracted from air for industrial uses annually by two primary methods.^[15] The most common method is fractional distillation of liquefied air, with N
₂ distilling as a vapor while O
₂ is left as a liquid.^[15]

The other primary method of producing O
₂ is passing a stream of clean, dry air through one bed of a pair of identical zeolite molecular sieves, which absorbs the nitrogen and delivers a gas stream that is 90% to 93% O
₂.^[15] Simultaneously, nitrogen gas is released from the other nitrogen-saturated zeolite bed, by reducing the chamber operating pressure and diverting part of the oxygen gas from the producer bed through it, in the reverse direction of flow. After a set cycle time the operation of the two beds is interchanged, thereby allowing for a continuous supply of gaseous oxygen to be pumped through a pipeline. This is known as pressure swing adsorption. Oxygen gas is increasingly obtained by these non-cryogenic technologies (see also the related vacuum swing adsorption).^[95]

Oxygen gas can also be produced through electrolysis of water into molecular oxygen and hydrogen. DC electricity must be used: if AC is used, the gases in each limb consist of hydrogen and oxygen in the explosive ratio 2:1. A similar method is the electrocatalytic O
₂ evolution from oxides and oxoacids. Chemical catalysts can be used as well, such as in chemical oxygen generators or oxygen candles that are used as part of the life-support equipment on submarines, and are still part of standard equipment on commercial airliners in case of depressurization emergencies. Another air separation method is forcing air to dissolve through ceramic membranes based on zirconium dioxide by either high pressure or an electric current, to produce nearly pure O
₂ gas.^[67]

Storage

Oxygen storage methods include high-pressure oxygen tanks, cryogenics and chemical compounds. For reasons of economy, oxygen is often transported in bulk as a liquid in specially insulated tankers, since one liter of liquefied oxygen is equivalent to 840 liters of gaseous oxygen at atmospheric pressure and 20 °C (68 °F).^[15] Such tankers are used to refill bulk liquid-oxygen storage containers, which stand outside hospitals and other institutions that need large volumes of pure oxygen gas. Liquid oxygen is passed through heat exchangers, which convert the cryogenic liquid into gas before it enters the building. Oxygen is also stored and shipped in smaller cylinders containing the compressed gas; a form that is useful in certain portable medical applications and oxy-fuel welding and cutting.^[15]

Applications

Medical

Uptake of O
₂ from the air is the essential purpose of respiration, so oxygen supplementation is used in medicine. Treatment not only increases oxygen levels in the patient’s blood, but has the secondary effect of decreasing resistance to blood flow in many types of diseased lungs, easing work load on the heart. Oxygen therapy is used to treat emphysema, pneumonia, some heart disorders (congestive heart failure), some disorders that cause increased pulmonary artery pressure, and any disease that impairs the body’s ability to take up and use gaseous oxygen.^[96]

Treatments are flexible enough to be used in hospitals, the patient’s home, or increasingly by portable devices. Oxygen tents were once commonly used in oxygen supplementation, but have since been replaced mostly by the use of oxygen masks or nasal cannulas.^[97]

Hyperbaric (high-pressure) medicine uses special oxygen chambers to increase the partial pressure of O
₂ around the patient and, when needed, the medical staff.^[98] Carbon monoxide poisoning, gas gangrene, and decompression sickness (the ‘bends’) are sometimes addressed with this therapy.^[99] Increased O
₂ concentration in the lungs helps to displace carbon monoxide from the heme group of hemoglobin.^[100][101] Oxygen gas is poisonous to the anaerobic bacteria that cause gas gangrene, so increasing its partial pressure helps kill them.^[102][103] Decompression sickness occurs in divers who decompress too quickly after a dive, resulting in bubbles of inert gas, mostly nitrogen and helium, forming in the blood. Increasing the pressure of O
₂ as soon as possible helps to redissolve the bubbles back into the blood so that these excess gasses can be exhaled naturally through the lungs.^{[96][104][105]} Normobaric oxygen administration at the highest available concentration is frequently used as first aid for any diving injury that may involve inert gas bubble formation in the tissues. There is epidemiological support for its use from a statistical study of cases recorded in a long term database.^{[106][107][108]}

Life support and recreational use

An application of O
₂ as a low-pressure breathing gas is in modern space suits, which surround their occupant’s body with the breathing gas. These devices use nearly pure oxygen at about one-third normal pressure, resulting in a normal blood partial pressure of O
₂. This trade-off of higher oxygen concentration for lower pressure is needed to maintain suit flexibility.^[109][110]

Scuba and surface-supplied underwater divers and submariners also rely on artificially delivered O
₂. Submarines, submersibles and atmospheric diving suits usually operate at normal atmospheric pressure. Breathing air is scrubbed of carbon dioxide by chemical extraction and oxygen is replaced to maintain a constant partial pressure. Ambient pressure divers breathe air or gas mixtures with an oxygen fraction suited to the operating depth. Pure or nearly pure O
₂ use in diving at pressures higher than atmospheric is usually limited to rebreathers, or decompression at relatively shallow depths (~6 meters depth, or less),^[111][112] or medical treatment in recompression chambers at pressures up to 2.8 bar, where acute oxygen toxicity can be managed without the risk of drowning. Deeper diving requires significant dilution of O
₂ with other gases, such as nitrogen or helium, to prevent oxygen toxicity.^[111]

People who climb mountains or fly in non-pressurized fixed-wing aircraft sometimes have supplemental O
₂ supplies.^[i] Pressurized commercial airplanes have an emergency supply of O
₂ automatically supplied to the passengers in case of cabin depressurization. Sudden cabin pressure loss activates chemical oxygen generators above each seat, causing oxygen masks to drop. Pulling on the masks «to start the flow of oxygen» as cabin safety instructions dictate, forces iron filings into the sodium chlorate inside the canister.^[67] A steady stream of oxygen gas is then produced by the exothermic reaction.

Oxygen, as a mild euphoric, has a history of recreational use in oxygen bars and in sports. Oxygen bars are establishments found in the United States since the late 1990s that offer higher than normal O
₂ exposure for a minimal fee.^[113] Professional athletes, especially in American football, sometimes go off-field between plays to don oxygen masks to boost performance. The pharmacological effect is doubted; a placebo effect is a more likely explanation.^[113] Available studies support a performance boost from oxygen enriched mixtures only if it is inhaled during aerobic exercise.^[114]

Other recreational uses that do not involve breathing include pyrotechnic applications, such as George Goble’s five-second ignition of barbecue grills.^[115]

Industrial

Smelting of iron ore into steel consumes 55% of commercially produced oxygen.^[67] In this process, O
₂ is injected through a high-pressure lance into molten iron, which removes sulfur impurities and excess carbon as the respective oxides, SO
₂ and CO
₂. The reactions are exothermic, so the temperature increases to 1,700 °C.^[67]

Another 25% of commercially produced oxygen is used by the chemical industry.^[67] Ethylene is reacted with O
₂ to create ethylene oxide, which, in turn, is converted into ethylene glycol; the primary feeder material used to manufacture a host of products, including antifreeze and polyester polymers (the precursors of many plastics and fabrics).^[67]

Most of the remaining 20% of commercially produced oxygen is used in medical applications, metal cutting and welding, as an oxidizer in rocket fuel, and in water treatment.^[67] Oxygen is used in oxyacetylene welding, burning acetylene with O
₂ to produce a very hot flame. In this process, metal up to 60 cm (24 in) thick is first heated with a small oxy-acetylene flame and then quickly cut by a large stream of O
₂.^[116]

Compounds

The oxidation state of oxygen is −2 in almost all known compounds of oxygen. The oxidation state −1 is found in a few compounds such as peroxides.^[117] Compounds containing oxygen in other oxidation states are very uncommon: −1/2 (superoxides), −1/3 (ozonides), 0 (elemental, hypofluorous acid), +1/2 (dioxygenyl), +1 (dioxygen difluoride), and +2 (oxygen difluoride).^[118]

Oxides and other inorganic compounds

Water (H
₂O) is an oxide of hydrogen and the most familiar oxygen compound. Hydrogen atoms are covalently bonded to oxygen in a water molecule but also have an additional attraction (about 23.3 kJ/mol per hydrogen atom) to an adjacent oxygen atom in a separate molecule.^[119] These hydrogen bonds between water molecules hold them approximately 15% closer than what would be expected in a simple liquid with just van der Waals forces.^[120][j]

Due to its electronegativity, oxygen forms chemical bonds with almost all other elements to give corresponding oxides. The surface of most metals, such as aluminium and titanium, are oxidized in the presence of air and become coated with a thin film of oxide that passivates the metal and slows further corrosion. Many oxides of the transition metals are non-stoichiometric compounds, with slightly less metal than the chemical formula would show. For example, the mineral FeO (wüstite) is written as , where x is usually around 0.05.^[121]

Oxygen is present in the atmosphere in trace quantities in the form of carbon dioxide (CO
₂). The Earth’s crustal rock is composed in large part of oxides of silicon (silica SiO
₂, as found in granite and quartz), aluminium (aluminium oxide Al
₂O
₃, in bauxite and corundum), iron (iron(III) oxide Fe
₂O
₃, in hematite and rust), and calcium carbonate (in limestone). The rest of the Earth’s crust is also made of oxygen compounds, in particular various complex silicates (in silicate minerals). The Earth’s mantle, of much larger mass than the crust, is largely composed of silicates of magnesium and iron.

Water-soluble silicates in the form of Na
₄SiO
₄, Na
₂SiO
₃, and Na
₂Si
₂O
₅ are used as detergents and adhesives.^[122]

Oxygen also acts as a ligand for transition metals, forming transition metal dioxygen complexes, which feature metal–O
₂. This class of compounds includes the heme proteins hemoglobin and myoglobin.^[123] An exotic and unusual reaction occurs with PtF
₆, which oxidizes oxygen to give O₂⁺PtF₆⁻, dioxygenyl hexafluoroplatinate.^[124]

Organic compounds

Among the most important classes of organic compounds that contain oxygen are (where «R» is an organic group): alcohols (R-OH); ethers (R-O-R); ketones (R-CO-R); aldehydes (R-CO-H); carboxylic acids (R-COOH); esters (R-COO-R); acid anhydrides (R-CO-O-CO-R); and amides (R-C(O)-NR
₂). There are many important organic solvents that contain oxygen, including: acetone, methanol, ethanol, isopropanol, furan, THF, diethyl ether, dioxane, ethyl acetate, DMF, DMSO, acetic acid, and formic acid. Acetone ((CH
₃)
₂CO) and phenol (C
₆H
₅OH) are used as feeder materials in the synthesis of many different substances. Other important organic compounds that contain oxygen are: glycerol, formaldehyde, glutaraldehyde, citric acid, acetic anhydride, and acetamide. Epoxides are ethers in which the oxygen atom is part of a ring of three atoms. The element is similarly found in almost all biomolecules that are important to (or generated by) life.

Oxygen reacts spontaneously with many organic compounds at or below room temperature in a process called autoxidation.^[125] Most of the organic compounds that contain oxygen are not made by direct action of O
₂. Organic compounds important in industry and commerce that are made by direct oxidation of a precursor include ethylene oxide and peracetic acid.^[122]

Safety and precautions

Oxygen

Hazards
GHS labelling:
Pictograms
Hazard statements	H272
Precautionary statements	P220, P244, P370+P376, P403
NFPA 704 (fire diamond)	0 0 1 OX

The NFPA 704 standard rates compressed oxygen gas as nonhazardous to health, nonflammable and nonreactive, but an oxidizer. Refrigerated liquid oxygen (LOX) is given a health hazard rating of 3 (for increased risk of hyperoxia from condensed vapors, and for hazards common to cryogenic liquids such as frostbite), and all other ratings are the same as the compressed gas form.^[126]

Toxicity

Oxygen gas (O
₂) can be toxic at elevated partial pressures, leading to convulsions and other health problems.^{[111][k][128]} Oxygen toxicity usually begins to occur at partial pressures more than 50 kilopascals (kPa), equal to about 50% oxygen composition at standard pressure or 2.5 times the normal sea-level O
₂ partial pressure of about 21 kPa. This is not a problem except for patients on mechanical ventilators, since gas supplied through oxygen masks in medical applications is typically composed of only 30–50% O
₂ by volume (about 30 kPa at standard pressure).^[8]

At one time, premature babies were placed in incubators containing O
₂-rich air, but this practice was discontinued after some babies were blinded by the oxygen content being too high.^[8]

Breathing pure O
₂ in space applications, such as in some modern space suits, or in early spacecraft such as Apollo, causes no damage due to the low total pressures used.^[109][129] In the case of spacesuits, the O
₂ partial pressure in the breathing gas is, in general, about 30 kPa (1.4 times normal), and the resulting O
₂ partial pressure in the astronaut’s arterial blood is only marginally more than normal sea-level O
₂ partial pressure.^[130]

Oxygen toxicity to the lungs and central nervous system can also occur in deep scuba diving and surface supplied diving.^[8][111] Prolonged breathing of an air mixture with an O
₂ partial pressure more than 60 kPa can eventually lead to permanent pulmonary fibrosis.^[131] Exposure to an O
₂ partial pressures greater than 160 kPa (about 1.6 atm) may lead to convulsions (normally fatal for divers). Acute oxygen toxicity (causing seizures, its most feared effect for divers) can occur by breathing an air mixture with 21% O
₂ at 66 m (217 ft) or more of depth; the same thing can occur by breathing 100% O
₂ at only 6 m (20 ft).^{[131][132][133][134]}

Combustion and other hazards

Highly concentrated sources of oxygen promote rapid combustion. Fire and explosion hazards exist when concentrated oxidants and fuels are brought into close proximity; an ignition event, such as heat or a spark, is needed to trigger combustion.^[31] Oxygen is the oxidant, not the fuel.

Concentrated O
₂ will allow combustion to proceed rapidly and energetically.^[31] Steel pipes and storage vessels used to store and transmit both gaseous and liquid oxygen will act as a fuel; and therefore the design and manufacture of O
₂ systems requires special training to ensure that ignition sources are minimized.^[31] The fire that killed the Apollo 1 crew in a launch pad test spread so rapidly because the capsule was pressurized with pure O
₂ but at slightly more than atmospheric pressure, instead of the 1⁄3 normal pressure that would be used in a mission.^[l][136]

Liquid oxygen spills, if allowed to soak into organic matter, such as wood, petrochemicals, and asphalt can cause these materials to detonate unpredictably on subsequent mechanical impact.^[31]

See also

Notes

References

General references

• Cook, Gerhard A.; Lauer, Carol M. (1968). «Oxygen». In Clifford A. Hampel (ed.). The Encyclopedia of the Chemical Elements. New York: Reinhold Book Corporation. pp. 499–512. LCCN 68-29938.
• Emsley, John (2001). «Oxygen». Nature’s Building Blocks: An A–Z Guide to the Elements. Oxford, England: Oxford University Press. pp. 297–304. ISBN 978-0-19-850340-8.
• Raven, Peter H.; Evert, Ray F.; Eichhorn, Susan E. (2005). Biology of Plants (7th ed.). New York: W. H. Freeman and Company Publishers. pp. 115–27. ISBN 978-0-7167-1007-3.

External links

• Oxygen at The Periodic Table of Videos (University of Nottingham)
• Oxidizing Agents > Oxygen
• Oxygen (O₂) Properties, Uses, Applications
• Roald Hoffmann article on «The Story of O»
• WebElements.com – Oxygen
• Oxygen on In Our Time at the BBC
• Scripps Institute: Atmospheric Oxygen has been dropping for 20 years

Oxygen, ₈O

Liquid oxygen boiling (O2)
Oxygen
Allotropes	O2, O3 (ozone) and more (see Allotropes of oxygen)
Appearance	gas: colorless liquid and solid: pale blue
Standard atomic weight Ar°(O)	[15.99903, 15.99977] 15.999±0.001 (abridged)[1]
Abundance
in the Earth’s crust	461000 ppm
Oxygen 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 – ↑ O ↓ S nitrogen ← oxygen → fluorine
Atomic number (Z)	8
Group	group 16 (chalcogens)
Period	period 2
Block	p-block
Electron configuration	[He] 2s2 2p4
Electrons per shell	2, 6
Physical properties
Phase at STP	gas
Melting point	(O2) 54.36 K ​(−218.79 °C, ​−361.82 °F)
Boiling point	(O2) 90.188 K ​(−182.962 °C, ​−297.332 °F)
Density (at STP)	1.429 g/L
when liquid (at b.p.)	1.141 g/cm3
Triple point	54.361 K, ​0.1463 kPa
Critical point	154.581 K, 5.043 MPa
Heat of fusion	(O2) 0.444 kJ/mol
Heat of vaporization	(O2) 6.82 kJ/mol
Molar heat capacity	(O2) 29.378 J/(mol·K)
Vapor pressure P (Pa) 1 10 100 1 k 10 k 100 k at T (K)       61 73 90
Atomic properties
Oxidation states	−2, −1, 0, +1, +2
Electronegativity	Pauling scale: 3.44
Ionization energies	1st: 1313.9 kJ/mol 2nd: 3388.3 kJ/mol 3rd: 5300.5 kJ/mol (more)
Covalent radius	66±2 pm
Van der Waals radius	152 pm
Spectral lines of oxygen
Other properties
Natural occurrence	primordial
Crystal structure	​cubic
Speed of sound	330 m/s (gas, at 27 °C)
Thermal conductivity	26.58×10−3  W/(m⋅K)
Magnetic ordering	paramagnetic
Molar magnetic susceptibility	+3449.0×10−6 cm3/mol (293 K)[2]
CAS Number	7782-44-7
History
Discovery	Carl Wilhelm Scheele (1771)
Named by	Antoine Lavoisier (1777)
Main isotopes of oxygen v e
Iso­tope Decay abun­dance half-life (t1/2) mode pro­duct 16O [99.738%, 99.776%] stable 17O [0.0367%, 0.0400%] stable 18O [0.187%, 0.222%] stable
Category: Oxygen view talk edit | references

Oxygen is the chemical element with the symbol O and atomic number 8. It is a member of the chalcogen group in the periodic table, a highly reactive nonmetal, and an oxidizing agent that readily forms oxides with most elements as well as with other compounds. Oxygen is Earth’s most abundant element, and after hydrogen and helium, it is the third-most abundant element in the universe. At standard temperature and pressure, two atoms of the element bind to form dioxygen, a colorless and odorless diatomic gas with the formula O
₂. Diatomic oxygen gas currently constitutes 20.95% of the Earth’s atmosphere, though this has changed considerably over long periods of time. Oxygen makes up almost half of the Earth’s crust in the form of oxides.^[3]

Many major classes of organic molecules in living organisms contain oxygen atoms, such as proteins, nucleic acids, carbohydrates, and fats, as do the major constituent inorganic compounds of animal shells, teeth, and bone. Most of the mass of living organisms is oxygen as a component of water, the major constituent of lifeforms. Oxygen is continuously replenished in Earth’s atmosphere by photosynthesis, which uses the energy of sunlight to produce oxygen from water and carbon dioxide. Oxygen is too chemically reactive to remain a free element in air without being continuously replenished by the photosynthetic action of living organisms. Another form (allotrope) of oxygen, ozone (O
₃), strongly absorbs ultraviolet UVB radiation and the high-altitude ozone layer helps protect the biosphere from ultraviolet radiation. However, ozone present at the surface is a byproduct of smog and thus a pollutant.

Oxygen was isolated by Michael Sendivogius before 1604, but it is commonly believed that the element was discovered independently by Carl Wilhelm Scheele, in Uppsala, in 1773 or earlier, and Joseph Priestley in Wiltshire, in 1774. Priority is often given for Priestley because his work was published first. Priestley, however, called oxygen «dephlogisticated air», and did not recognize it as a chemical element. The name oxygen was coined in 1777 by Antoine Lavoisier, who first recognized oxygen as a chemical element and correctly characterized the role it plays in combustion.

Common uses of oxygen include production of steel, plastics and textiles, brazing, welding and cutting of steels and other metals, rocket propellant, oxygen therapy, and life support systems in aircraft, submarines, spaceflight and diving.

History of study

Early experiments

One of the first known experiments on the relationship between combustion and air was conducted by the 2nd century BCE Greek writer on mechanics, Philo of Byzantium. In his work Pneumatica, Philo observed that inverting a vessel over a burning candle and surrounding the vessel’s neck with water resulted in some water rising into the neck.^[4] Philo incorrectly surmised that parts of the air in the vessel were converted into the classical element fire and thus were able to escape through pores in the glass. Many centuries later Leonardo da Vinci built on Philo’s work by observing that a portion of air is consumed during combustion and respiration.^[5]

In the late 17th century, Robert Boyle proved that air is necessary for combustion. English chemist John Mayow (1641–1679) refined this work by showing that fire requires only a part of air that he called spiritus nitroaereus.^[6] In one experiment, he found that placing either a mouse or a lit candle in a closed container over water caused the water to rise and replace one-fourteenth of the air’s volume before extinguishing the subjects.^[7] From this, he surmised that nitroaereus is consumed in both respiration and combustion.

Mayow observed that antimony increased in weight when heated, and inferred that the nitroaereus must have combined with it.^[6] He also thought that the lungs separate nitroaereus from air and pass it into the blood and that animal heat and muscle movement result from the reaction of nitroaereus with certain substances in the body.^[6] Accounts of these and other experiments and ideas were published in 1668 in his work Tractatus duo in the tract «De respiratione».^[7]

Phlogiston theory

Robert Hooke, Ole Borch, Mikhail Lomonosov, and Pierre Bayen all produced oxygen in experiments in the 17th and the 18th century but none of them recognized it as a chemical element.^[8] This may have been in part due to the prevalence of the philosophy of combustion and corrosion called the phlogiston theory, which was then the favored explanation of those processes.^[9]

Established in 1667 by the German alchemist J. J. Becher, and modified by the chemist Georg Ernst Stahl by 1731,^[10] phlogiston theory stated that all combustible materials were made of two parts. One part, called phlogiston, was given off when the substance containing it was burned, while the dephlogisticated part was thought to be its true form, or calx.^[5]

Highly combustible materials that leave little residue, such as wood or coal, were thought to be made mostly of phlogiston; non-combustible substances that corrode, such as iron, contained very little. Air did not play a role in phlogiston theory, nor were any initial quantitative experiments conducted to test the idea; instead, it was based on observations of what happens when something burns, that most common objects appear to become lighter and seem to lose something in the process.^[5]

Discovery

Polish alchemist, philosopher, and physician Michael Sendivogius (Michał Sędziwój) in his work De Lapide Philosophorum Tractatus duodecim e naturae fonte et manuali experientia depromti (1604) described a substance contained in air, referring to it as ‘cibus vitae’ (food of life,^[11]) and according to Polish historian Roman Bugaj, this substance is identical with oxygen.^[12] Sendivogius, during his experiments performed between 1598 and 1604, properly recognized that the substance is equivalent to the gaseous byproduct released by the thermal decomposition of potassium nitrate. In Bugaj’s view, the isolation of oxygen and the proper association of the substance to that part of air which is required for life, provides sufficient evidence for the discovery of oxygen by Sendivogius.^[12] This discovery of Sendivogius was however frequently denied by the generations of scientists and chemists which succeeded him.^[11]

It is also commonly claimed that oxygen was first discovered by Swedish pharmacist Carl Wilhelm Scheele. He had produced oxygen gas by heating mercuric oxide (HgO) and various nitrates in 1771–72.^[13][14][5] Scheele called the gas «fire air» because it was then the only known agent to support combustion. He wrote an account of this discovery in a manuscript titled Treatise on Air and Fire, which he sent to his publisher in 1775. That document was published in 1777.^[15]

In the meantime, on August 1, 1774, an experiment conducted by the British clergyman Joseph Priestley focused sunlight on mercuric oxide contained in a glass tube, which liberated a gas he named «dephlogisticated air».^[14] He noted that candles burned brighter in the gas and that a mouse was more active and lived longer while breathing it. After breathing the gas himself, Priestley wrote: «The feeling of it to my lungs was not sensibly different from that of common air, but I fancied that my breast felt peculiarly light and easy for some time afterwards.»^[8] Priestley published his findings in 1775 in a paper titled «An Account of Further Discoveries in Air», which was included in the second volume of his book titled Experiments and Observations on Different Kinds of Air.^[5][16] Because he published his findings first, Priestley is usually given priority in the discovery.

The French chemist Antoine Laurent Lavoisier later claimed to have discovered the new substance independently. Priestley visited Lavoisier in October 1774 and told him about his experiment and how he liberated the new gas. Scheele had also dispatched a letter to Lavoisier on September 30, 1774, which described his discovery of the previously unknown substance, but Lavoisier never acknowledged receiving it. (A copy of the letter was found in Scheele’s belongings after his death.)^[15]

Lavoisier’s contribution

Lavoisier conducted the first adequate quantitative experiments on oxidation and gave the first correct explanation of how combustion works.^[14] He used these and similar experiments, all started in 1774, to discredit the phlogiston theory and to prove that the substance discovered by Priestley and Scheele was a chemical element.

In one experiment, Lavoisier observed that there was no overall increase in weight when tin and air were heated in a closed container.^[14] He noted that air rushed in when he opened the container, which indicated that part of the trapped air had been consumed. He also noted that the tin had increased in weight and that increase was the same as the weight of the air that rushed back in. This and other experiments on combustion were documented in his book Sur la combustion en général, which was published in 1777.^[14] In that work, he proved that air is a mixture of two gases; ‘vital air’, which is essential to combustion and respiration, and azote (Gk. ἄζωτον «lifeless»), which did not support either. Azote later became nitrogen in English, although it has kept the earlier name in French and several other European languages.^[14]

Etymology

Lavoisier renamed ‘vital air’ to oxygène in 1777 from the Greek roots ὀξύς (oxys) (acid, literally «sharp», from the taste of acids) and -γενής (-genēs) (producer, literally begetter), because he mistakenly believed that oxygen was a constituent of all acids.^[17] Chemists (such as Sir Humphry Davy in 1812) eventually determined that Lavoisier was wrong in this regard, but by then the name was too well established.^[18]

Oxygen entered the English language despite opposition by English scientists and the fact that the Englishman Priestley had first isolated the gas and written about it. This is partly due to a poem praising the gas titled «Oxygen» in the popular book The Botanic Garden (1791) by Erasmus Darwin, grandfather of Charles Darwin.^[15]

Later history

John Dalton’s original atomic hypothesis presumed that all elements were monatomic and that the atoms in compounds would normally have the simplest atomic ratios with respect to one another. For example, Dalton assumed that water’s formula was HO, leading to the conclusion that the atomic mass of oxygen was 8 times that of hydrogen, instead of the modern value of about 16.^[19] In 1805, Joseph Louis Gay-Lussac and Alexander von Humboldt showed that water is formed of two volumes of hydrogen and one volume of oxygen; and by 1811 Amedeo Avogadro had arrived at the correct interpretation of water’s composition, based on what is now called Avogadro’s law and the diatomic elemental molecules in those gases.^[20][a]

The first commercial method of producing oxygen was chemical, the so-called Brin process involving a reversible reaction of barium oxide. It was invented in 1852 and commercialized in 1884, but was displaced by newer methods in early 20th century.

By the late 19th century scientists realized that air could be liquefied and its components isolated by compressing and cooling it. Using a cascade method, Swiss chemist and physicist Raoul Pierre Pictet evaporated liquid sulfur dioxide in order to liquefy carbon dioxide, which in turn was evaporated to cool oxygen gas enough to liquefy it. He sent a telegram on December 22, 1877, to the French Academy of Sciences in Paris announcing his discovery of liquid oxygen.^[21] Just two days later, French physicist Louis Paul Cailletet announced his own method of liquefying molecular oxygen.^[21] Only a few drops of the liquid were produced in each case and no meaningful analysis could be conducted. Oxygen was liquefied in a stable state for the first time on March 29, 1883, by Polish scientists from Jagiellonian University, Zygmunt Wróblewski and Karol Olszewski.^[22]

In 1891 Scottish chemist James Dewar was able to produce enough liquid oxygen for study.^[23] The first commercially viable process for producing liquid oxygen was independently developed in 1895 by German engineer Carl von Linde and British engineer William Hampson. Both men lowered the temperature of air until it liquefied and then distilled the component gases by boiling them off one at a time and capturing them separately.^[24] Later, in 1901, oxyacetylene welding was demonstrated for the first time by burning a mixture of acetylene and compressed O
₂. This method of welding and cutting metal later became common.^[24]

In 1923, the American scientist Robert H. Goddard became the first person to develop a rocket engine that burned liquid fuel; the engine used gasoline for fuel and liquid oxygen as the oxidizer. Goddard successfully flew a small liquid-fueled rocket 56 m at 97 km/h on March 16, 1926, in Auburn, Massachusetts, US.^[24][25]

In academic laboratories, oxygen can be prepared by heating together potassium chlorate mixed with a small proportion of manganese dioxide.^[26]

Oxygen levels in the atmosphere are trending slightly downward globally, possibly because of fossil-fuel burning.^[27]

Characteristics

Properties and molecular structure

At standard temperature and pressure, oxygen is a colorless, odorless, and tasteless gas with the molecular formula O
₂, referred to as dioxygen.^[29]

As dioxygen, two oxygen atoms are chemically bound to each other. The bond can be variously described based on level of theory, but is reasonably and simply described as a covalent double bond that results from the filling of molecular orbitals formed from the atomic orbitals of the individual oxygen atoms, the filling of which results in a bond order of two. More specifically, the double bond is the result of sequential, low-to-high energy, or Aufbau, filling of orbitals, and the resulting cancellation of contributions from the 2s electrons, after sequential filling of the low σ and σ^* orbitals; σ overlap of the two atomic 2p orbitals that lie along the O–O molecular axis and π overlap of two pairs of atomic 2p orbitals perpendicular to the O–O molecular axis, and then cancellation of contributions from the remaining two 2p electrons after their partial filling of the π^* orbitals.^[28]

This combination of cancellations and σ and π overlaps results in dioxygen’s double-bond character and reactivity, and a triplet electronic ground state. An electron configuration with two unpaired electrons, as is found in dioxygen orbitals (see the filled π* orbitals in the diagram) that are of equal energy—i.e., degenerate—is a configuration termed a spin triplet state. Hence, the ground state of the O
₂ molecule is referred to as triplet oxygen.^[30][b] The highest-energy, partially filled orbitals are antibonding, and so their filling weakens the bond order from three to two. Because of its unpaired electrons, triplet oxygen reacts only slowly with most organic molecules, which have paired electron spins; this prevents spontaneous combustion.^[31]

In the triplet form, O
₂ molecules are paramagnetic. That is, they impart magnetic character to oxygen when it is in the presence of a magnetic field, because of the spin magnetic moments of the unpaired electrons in the molecule, and the negative exchange energy between neighboring O
₂ molecules.^[23] Liquid oxygen is so magnetic that, in laboratory demonstrations, a bridge of liquid oxygen may be supported against its own weight between the poles of a powerful magnet.^[32][c]

Singlet oxygen is a name given to several higher-energy species of molecular O
₂ in which all the electron spins are paired. It is much more reactive with common organic molecules than is normal (triplet) molecular oxygen. In nature, singlet oxygen is commonly formed from water during photosynthesis, using the energy of sunlight.^[33] It is also produced in the troposphere by the photolysis of ozone by light of short wavelength^[34] and by the immune system as a source of active oxygen.^[35] Carotenoids in photosynthetic organisms (and possibly animals) play a major role in absorbing energy from singlet oxygen and converting it to the unexcited ground state before it can cause harm to tissues.^[36]

Allotropes

The common allotrope of elemental oxygen on Earth is called dioxygen, O
₂, the major part of the Earth’s atmospheric oxygen (see Occurrence). O₂ has a bond length of 121 pm and a bond energy of 498 kJ/mol.^[37] O₂ is used by complex forms of life, such as animals, in cellular respiration. Other aspects of O
₂ are covered in the remainder of this article.

Trioxygen (O
₃) is usually known as ozone and is a very reactive allotrope of oxygen that is damaging to lung tissue.^[38] Ozone is produced in the upper atmosphere when O
₂ combines with atomic oxygen made by the splitting of O
₂ by ultraviolet (UV) radiation.^[17] Since ozone absorbs strongly in the UV region of the spectrum, the ozone layer of the upper atmosphere functions as a protective radiation shield for the planet.^[17] Near the Earth’s surface, it is a pollutant formed as a by-product of automobile exhaust.^[38] At low earth orbit altitudes, sufficient atomic oxygen is present to cause corrosion of spacecraft.^[39]

The metastable molecule tetraoxygen (O
₄) was discovered in 2001,^[40][41] and was assumed to exist in one of the six phases of solid oxygen. It was proven in 2006 that this phase, created by pressurizing O
₂ to 20 GPa, is in fact a rhombohedral O
₈ cluster.^[42] This cluster has the potential to be a much more powerful oxidizer than either O
₂ or O
₃ and may therefore be used in rocket fuel.^[40][41] A metallic phase was discovered in 1990 when solid oxygen is subjected to a pressure of above 96 GPa^[43] and it was shown in 1998 that at very low temperatures, this phase becomes superconducting.^[44]

Physical properties

Oxygen dissolves more readily in water than in nitrogen, and in freshwater more readily than in seawater. Water in equilibrium with air contains approximately 1 molecule of dissolved O
₂ for every 2 molecules of N
₂ (1:2), compared with an atmospheric ratio of approximately 1:4. The solubility of oxygen in water is temperature-dependent, and about twice as much (14.6 mg/L) dissolves at 0 °C than at 20 °C (7.6 mg/L).^[8][45] At 25 °C and 1 standard atmosphere (101.3 kPa) of air, freshwater can dissolve about 6.04 milliliters (mL) of oxygen per liter, and seawater contains about 4.95 mL per liter.^[46] At 5 °C the solubility increases to 9.0 mL (50% more than at 25 °C) per liter for freshwater and 7.2 mL (45% more) per liter for sea water.

Oxygen gas dissolved in water at sea-level

	5 °C	25 °C
Freshwater	9.00	6.04
Seawater	7.20	4.95

(milliliters per liter)

Oxygen condenses at 90.20 K (−182.95 °C, −297.31 °F) and freezes at 54.36 K (−218.79 °C, −361.82 °F).^[47] Both liquid and solid O
₂ are clear substances with a light sky-blue color caused by absorption in the red (in contrast with the blue color of the sky, which is due to Rayleigh scattering of blue light). High-purity liquid O
₂ is usually obtained by the fractional distillation of liquefied air.^[48] Liquid oxygen may also be condensed from air using liquid nitrogen as a coolant.^[49]

Liquid oxygen is a highly reactive substance and must be segregated from combustible materials.^[49]

The spectroscopy of molecular oxygen is associated with the atmospheric processes of aurora and airglow.^[50] The absorption in the Herzberg continuum and Schumann–Runge bands in the ultraviolet produces atomic oxygen that is important in the chemistry of the middle atmosphere.^[51] Excited-state singlet molecular oxygen is responsible for red chemiluminescence in solution.^[52]

Table of thermal and physical properties of oxygen (O2) at atmospheric pressure:^[53][54]

Temperature (K)	Density (kg/m^3)	Specific heat (kJ/kg °C)	Dynamic viscosity (kg/m s)	Kinematic viscosity (m^2/s)	Thermal conductivity (W/m °C)	Thermal diffusivity (m^2/s)	Prandtl Number
100	3.945	0.962	7.64E-06	1.94E-06	0.00925	2.44E-06	0.796
150	2.585	0.921	1.15E-05	4.44E-06	0.0138	5.80E-06	0.766
200	1.93	0.915	1.48E-05	7.64E-06	0.0183	1.04E-05	0.737
250	1.542	0.915	1.79E-05	1.16E-05	0.0226	1.60E-05	0.723
300	1.284	0.92	2.07E-05	1.61E-05	0.0268	2.27E-05	0.711
350	1.1	0.929	2.34E-05	2.12E-05	0.0296	2.90E-05	0.733
400	0.962	1.0408	2.58E-05	2.68E-05	0.033	3.64E-05	0.737
450	0.8554	0.956	2.81E-05	3.29E-05	0.0363	4.44E-05	0.741
500	0.7698	0.972	3.03E-05	3.94E-05	0.0412	5.51E-05	0.716
550	0.6998	0.988	3.24E-05	4.63E-05	0.0441	6.38E-05	0.726
600	0.6414	1.003	3.44E-05	5.36E-05	0.0473	7.35E-05	0.729
700	0.5498	1.031	3.81E-05	6.93E-05	0.0528	9.31E-05	0.744
800	0.481	1.054	4.15E-05	8.63E-05	0.0589	1.16E-04	0.743
900	0.4275	1.074	4.47E-05	1.05E-04	0.0649	1.41E-04	0.74
1000	0.3848	1.09	4.77E-05	1.24E-04	0.071	1.69E-04	0.733
1100	0.3498	1.103	5.06E-05	1.45E-04	0.0758	1.96E-04	0.736
1200	0.3206	1.0408	5.33E-05	1.661E-04	0.0819	2.29E-04	0.725
1300	0.296	1.125	5.88E-05	1.99E-04	0.0871	2.62E-04	0.721

Isotopes and stellar origin

Naturally occurring oxygen is composed of three stable isotopes, ¹⁶O, ¹⁷O, and ¹⁸O, with ¹⁶O being the most abundant (99.762% natural abundance).^[55]

Most ¹⁶O is synthesized at the end of the helium fusion process in massive stars but some is made in the neon burning process.^{[56] 17}O is primarily made by the burning of hydrogen into helium during the CNO cycle, making it a common isotope in the hydrogen burning zones of stars.^[56] Most ¹⁸O is produced when ¹⁴N (made abundant from CNO burning) captures a ⁴He nucleus, making ¹⁸O common in the helium-rich zones of evolved, massive stars.^[56]

Thirteen radioisotopes have been characterized, ranging from ¹¹O to ²⁶O.^[57] The most stable are ¹⁵O with a half-life of 122.24 seconds and ¹⁴O with a half-life of 70.606 seconds.^[55] All of the remaining radioactive isotopes have half-lives that are less than 27 s and the majority of these have half-lives that are less than 83 milliseconds.^[55] The most common decay mode of the isotopes lighter than ¹⁶O is β⁺ decay^[58][59][60] to yield nitrogen, and the most common mode for the isotopes heavier than ¹⁸O is beta decay to yield fluorine.^[55]

Occurrence

Ten most common elements in the Milky Way Galaxy estimated spectroscopically^[61]

Z	Element	Mass fraction in parts per million
1	Hydrogen	739,000	71 × mass of oxygen (red bar)
2	Helium	240,000	23 × mass of oxygen (red bar)
8	Oxygen	10,400
6	Carbon	4,600
10	Neon	1,340
26	Iron	1,090
7	Nitrogen	960
14	Silicon	650
12	Magnesium	580
16	Sulfur	440

Oxygen is the most abundant chemical element by mass in the Earth’s biosphere, air, sea and land. Oxygen is the third most abundant chemical element in the universe, after hydrogen and helium.^[62] About 0.9% of the Sun’s mass is oxygen.^[14] Oxygen constitutes 49.2% of the Earth’s crust by mass^[63] as part of oxide compounds such as silicon dioxide and is the most abundant element by mass in the Earth’s crust. It is also the major component of the world’s oceans (88.8% by mass).^[14] Oxygen gas is the second most common component of the Earth’s atmosphere, taking up 20.8% of its volume and 23.1% of its mass (some 10¹⁵ tonnes).^[14][64][d] Earth is unusual among the planets of the Solar System in having such a high concentration of oxygen gas in its atmosphere: Mars (with 0.1% O
₂ by volume) and Venus have much less. The O
₂ surrounding those planets is produced solely by the action of ultraviolet radiation on oxygen-containing molecules such as carbon dioxide.

The unusually high concentration of oxygen gas on Earth is the result of the oxygen cycle. This biogeochemical cycle describes the movement of oxygen within and between its three main reservoirs on Earth: the atmosphere, the biosphere, and the lithosphere. The main driving factor of the oxygen cycle is photosynthesis, which is responsible for modern Earth’s atmosphere. Photosynthesis releases oxygen into the atmosphere, while respiration, decay, and combustion remove it from the atmosphere. In the present equilibrium, production and consumption occur at the same rate.^[65]

Free oxygen also occurs in solution in the world’s water bodies. The increased solubility of O
₂ at lower temperatures (see Physical properties) has important implications for ocean life, as polar oceans support a much higher density of life due to their higher oxygen content.^[66] Water polluted with plant nutrients such as nitrates or phosphates may stimulate growth of algae by a process called eutrophication and the decay of these organisms and other biomaterials may reduce the O
₂ content in eutrophic water bodies. Scientists assess this aspect of water quality by measuring the water’s biochemical oxygen demand, or the amount of O
₂ needed to restore it to a normal concentration.^[67]

Analysis

Paleoclimatologists measure the ratio of oxygen-18 and oxygen-16 in the shells and skeletons of marine organisms to determine the climate millions of years ago (see oxygen isotope ratio cycle). Seawater molecules that contain the lighter isotope, oxygen-16, evaporate at a slightly faster rate than water molecules containing the 12% heavier oxygen-18, and this disparity increases at lower temperatures.^[68] During periods of lower global temperatures, snow and rain from that evaporated water tends to be higher in oxygen-16, and the seawater left behind tends to be higher in oxygen-18. Marine organisms then incorporate more oxygen-18 into their skeletons and shells than they would in a warmer climate.^[68] Paleoclimatologists also directly measure this ratio in the water molecules of ice core samples as old as hundreds of thousands of years.

Planetary geologists have measured the relative quantities of oxygen isotopes in samples from the Earth, the Moon, Mars, and meteorites, but were long unable to obtain reference values for the isotope ratios in the Sun, believed to be the same as those of the primordial solar nebula. Analysis of a silicon wafer exposed to the solar wind in space and returned by the crashed Genesis spacecraft has shown that the Sun has a higher proportion of oxygen-16 than does the Earth. The measurement implies that an unknown process depleted oxygen-16 from the Sun’s disk of protoplanetary material prior to the coalescence of dust grains that formed the Earth.^[69]

Oxygen presents two spectrophotometric absorption bands peaking at the wavelengths 687 and 760 nm. Some remote sensing scientists have proposed using the measurement of the radiance coming from vegetation canopies in those bands to characterize plant health status from a satellite platform.^[70] This approach exploits the fact that in those bands it is possible to discriminate the vegetation’s reflectance from its fluorescence, which is much weaker. The measurement is technically difficult owing to the low signal-to-noise ratio and the physical structure of vegetation; but it has been proposed as a possible method of monitoring the carbon cycle from satellites on a global scale.

Biological production and role of O₂

Photosynthesis and respiration

In nature, free oxygen is produced by the light-driven splitting of water during oxygenic photosynthesis. According to some estimates, green algae and cyanobacteria in marine environments provide about 70% of the free oxygen produced on Earth, and the rest is produced by terrestrial plants.^[71] Other estimates of the oceanic contribution to atmospheric oxygen are higher, while some estimates are lower, suggesting oceans produce ~45% of Earth’s atmospheric oxygen each year.^[72]

A simplified overall formula for photosynthesis is^[73]

6 CO₂ + 6 H
₂O + photons → C
₆H
₁₂O
₆ + 6 O
₂

or simply

carbon dioxide + water + sunlight → glucose + dioxygen

Photolytic oxygen evolution occurs in the thylakoid membranes of photosynthetic organisms and requires the energy of four photons.^[e] Many steps are involved, but the result is the formation of a proton gradient across the thylakoid membrane, which is used to synthesize adenosine triphosphate (ATP) via photophosphorylation.^[74] The O
₂ remaining (after production of the water molecule) is released into the atmosphere.^[f]

Oxygen is used in mitochondria in the generation of ATP during oxidative phosphorylation. The reaction for aerobic respiration is essentially the reverse of photosynthesis and is simplified as

C
₆H
₁₂O
₆ + 6 O
₂ → 6 CO₂ + 6 H
₂O + 2880 kJ/mol

In vertebrates, O
₂ diffuses through membranes in the lungs and into red blood cells. Hemoglobin binds O
₂, changing color from bluish red to bright red^[38] (CO
₂ is released from another part of hemoglobin through the Bohr effect). Other animals use hemocyanin (molluscs and some arthropods) or hemerythrin (spiders and lobsters).^[64] A liter of blood can dissolve 200 cm³ of O
₂.^[64]

Until the discovery of anaerobic metazoa,^[75] oxygen was thought to be a requirement for all complex life.^[76]

Reactive oxygen species, such as superoxide ion (O⁻
₂) and hydrogen peroxide (H
₂O
₂), are reactive by-products of oxygen use in organisms.^[64] Parts of the immune system of higher organisms create peroxide, superoxide, and singlet oxygen to destroy invading microbes. Reactive oxygen species also play an important role in the hypersensitive response of plants against pathogen attack.^[74] Oxygen is damaging to obligately anaerobic organisms, which were the dominant form of early life on Earth until O
₂ began to accumulate in the atmosphere about 2.5 billion years ago during the Great Oxygenation Event, about a billion years after the first appearance of these organisms.^[77][78]

An adult human at rest inhales 1.8 to 2.4 grams of oxygen per minute.^[79] This amounts to more than 6 billion tonnes of oxygen inhaled by humanity per year.^[g]

Living organisms

Partial pressures of oxygen in the human body (PO₂

Unit	Alveolar pulmonary gas pressures	Arterial blood oxygen	Venous blood gas
kPa	14.2	11[h]-13[h]	4.0[h]-5.3[h]
mmHg	107	75[80]-100[80]	30[81]-40[81]

)

The free oxygen partial pressure in the body of a living vertebrate organism is highest in the respiratory system, and decreases along any arterial system, peripheral tissues, and venous system, respectively. Partial pressure is the pressure that oxygen would have if it alone occupied the volume.^[82]

Build-up in the atmosphere

Free oxygen gas was almost nonexistent in Earth’s atmosphere before photosynthetic archaea and bacteria evolved, probably about 3.5 billion years ago. Free oxygen first appeared in significant quantities during the Paleoproterozoic eon (between 3.0 and 2.3 billion years ago).^[83] Even if there was much dissolved iron in the oceans when oxygenic photosynthesis was getting more common, it appears the banded iron formations were created by anoxyenic or micro-aerophilic iron-oxidizing bacteria which dominated the deeper areas of the photic zone, while oxygen-producing cyanobacteria covered the shallows.^[84] Free oxygen began to outgas from the oceans 3–2.7 billion years ago, reaching 10% of its present level around 1.7 billion years ago.^[83][85]

The presence of large amounts of dissolved and free oxygen in the oceans and atmosphere may have driven most of the extant anaerobic organisms to extinction during the Great Oxygenation Event (oxygen catastrophe) about 2.4 billion years ago. Cellular respiration using O
₂ enables aerobic organisms to produce much more ATP than anaerobic organisms.^[86] Cellular respiration of O
₂ occurs in all eukaryotes, including all complex multicellular organisms such as plants and animals.

Since the beginning of the Cambrian period 540 million years ago, atmospheric O
₂ levels have fluctuated between 15% and 30% by volume.^[87] Towards the end of the Carboniferous period (about 300 million years ago) atmospheric O
₂ levels reached a maximum of 35% by volume,^[87] which may have contributed to the large size of insects and amphibians at this time.^[88]

Variations in atmospheric oxygen concentration have shaped past climates. When oxygen declined, atmospheric density dropped, which in turn increased surface evaporation, causing precipitation increases and warmer temperatures.^[89]

At the current rate of photosynthesis it would take about 2,000 years to regenerate the entire O
₂ in the present atmosphere.^[90]

In the field of astrobiology and in the search for extraterrestrial life oxygen is a strong biosignature. That said it might not be a definite biosignature, being possibly produced abiotically on celestial bodies with processes and conditions (such as a peculiar hydrosphere) which allow free oxygen,^[91][92][93] like with Europa’s and Ganymede’s thin
oxygen atmospheres.^[94]

Industrial production

One hundred million tonnes of O
₂ are extracted from air for industrial uses annually by two primary methods.^[15] The most common method is fractional distillation of liquefied air, with N
₂ distilling as a vapor while O
₂ is left as a liquid.^[15]

The other primary method of producing O
₂ is passing a stream of clean, dry air through one bed of a pair of identical zeolite molecular sieves, which absorbs the nitrogen and delivers a gas stream that is 90% to 93% O
₂.^[15] Simultaneously, nitrogen gas is released from the other nitrogen-saturated zeolite bed, by reducing the chamber operating pressure and diverting part of the oxygen gas from the producer bed through it, in the reverse direction of flow. After a set cycle time the operation of the two beds is interchanged, thereby allowing for a continuous supply of gaseous oxygen to be pumped through a pipeline. This is known as pressure swing adsorption. Oxygen gas is increasingly obtained by these non-cryogenic technologies (see also the related vacuum swing adsorption).^[95]

Oxygen gas can also be produced through electrolysis of water into molecular oxygen and hydrogen. DC electricity must be used: if AC is used, the gases in each limb consist of hydrogen and oxygen in the explosive ratio 2:1. A similar method is the electrocatalytic O
₂ evolution from oxides and oxoacids. Chemical catalysts can be used as well, such as in chemical oxygen generators or oxygen candles that are used as part of the life-support equipment on submarines, and are still part of standard equipment on commercial airliners in case of depressurization emergencies. Another air separation method is forcing air to dissolve through ceramic membranes based on zirconium dioxide by either high pressure or an electric current, to produce nearly pure O
₂ gas.^[67]

Storage

Oxygen storage methods include high-pressure oxygen tanks, cryogenics and chemical compounds. For reasons of economy, oxygen is often transported in bulk as a liquid in specially insulated tankers, since one liter of liquefied oxygen is equivalent to 840 liters of gaseous oxygen at atmospheric pressure and 20 °C (68 °F).^[15] Such tankers are used to refill bulk liquid-oxygen storage containers, which stand outside hospitals and other institutions that need large volumes of pure oxygen gas. Liquid oxygen is passed through heat exchangers, which convert the cryogenic liquid into gas before it enters the building. Oxygen is also stored and shipped in smaller cylinders containing the compressed gas; a form that is useful in certain portable medical applications and oxy-fuel welding and cutting.^[15]

Applications

Medical

Uptake of O
₂ from the air is the essential purpose of respiration, so oxygen supplementation is used in medicine. Treatment not only increases oxygen levels in the patient’s blood, but has the secondary effect of decreasing resistance to blood flow in many types of diseased lungs, easing work load on the heart. Oxygen therapy is used to treat emphysema, pneumonia, some heart disorders (congestive heart failure), some disorders that cause increased pulmonary artery pressure, and any disease that impairs the body’s ability to take up and use gaseous oxygen.^[96]

Treatments are flexible enough to be used in hospitals, the patient’s home, or increasingly by portable devices. Oxygen tents were once commonly used in oxygen supplementation, but have since been replaced mostly by the use of oxygen masks or nasal cannulas.^[97]

Hyperbaric (high-pressure) medicine uses special oxygen chambers to increase the partial pressure of O
₂ around the patient and, when needed, the medical staff.^[98] Carbon monoxide poisoning, gas gangrene, and decompression sickness (the ‘bends’) are sometimes addressed with this therapy.^[99] Increased O
₂ concentration in the lungs helps to displace carbon monoxide from the heme group of hemoglobin.^[100][101] Oxygen gas is poisonous to the anaerobic bacteria that cause gas gangrene, so increasing its partial pressure helps kill them.^[102][103] Decompression sickness occurs in divers who decompress too quickly after a dive, resulting in bubbles of inert gas, mostly nitrogen and helium, forming in the blood. Increasing the pressure of O
₂ as soon as possible helps to redissolve the bubbles back into the blood so that these excess gasses can be exhaled naturally through the lungs.^{[96][104][105]} Normobaric oxygen administration at the highest available concentration is frequently used as first aid for any diving injury that may involve inert gas bubble formation in the tissues. There is epidemiological support for its use from a statistical study of cases recorded in a long term database.^{[106][107][108]}

Life support and recreational use

An application of O
₂ as a low-pressure breathing gas is in modern space suits, which surround their occupant’s body with the breathing gas. These devices use nearly pure oxygen at about one-third normal pressure, resulting in a normal blood partial pressure of O
₂. This trade-off of higher oxygen concentration for lower pressure is needed to maintain suit flexibility.^[109][110]

Scuba and surface-supplied underwater divers and submariners also rely on artificially delivered O
₂. Submarines, submersibles and atmospheric diving suits usually operate at normal atmospheric pressure. Breathing air is scrubbed of carbon dioxide by chemical extraction and oxygen is replaced to maintain a constant partial pressure. Ambient pressure divers breathe air or gas mixtures with an oxygen fraction suited to the operating depth. Pure or nearly pure O
₂ use in diving at pressures higher than atmospheric is usually limited to rebreathers, or decompression at relatively shallow depths (~6 meters depth, or less),^[111][112] or medical treatment in recompression chambers at pressures up to 2.8 bar, where acute oxygen toxicity can be managed without the risk of drowning. Deeper diving requires significant dilution of O
₂ with other gases, such as nitrogen or helium, to prevent oxygen toxicity.^[111]

People who climb mountains or fly in non-pressurized fixed-wing aircraft sometimes have supplemental O
₂ supplies.^[i] Pressurized commercial airplanes have an emergency supply of O
₂ automatically supplied to the passengers in case of cabin depressurization. Sudden cabin pressure loss activates chemical oxygen generators above each seat, causing oxygen masks to drop. Pulling on the masks «to start the flow of oxygen» as cabin safety instructions dictate, forces iron filings into the sodium chlorate inside the canister.^[67] A steady stream of oxygen gas is then produced by the exothermic reaction.

Oxygen, as a mild euphoric, has a history of recreational use in oxygen bars and in sports. Oxygen bars are establishments found in the United States since the late 1990s that offer higher than normal O
₂ exposure for a minimal fee.^[113] Professional athletes, especially in American football, sometimes go off-field between plays to don oxygen masks to boost performance. The pharmacological effect is doubted; a placebo effect is a more likely explanation.^[113] Available studies support a performance boost from oxygen enriched mixtures only if it is inhaled during aerobic exercise.^[114]

Other recreational uses that do not involve breathing include pyrotechnic applications, such as George Goble’s five-second ignition of barbecue grills.^[115]

Industrial

Smelting of iron ore into steel consumes 55% of commercially produced oxygen.^[67] In this process, O
₂ is injected through a high-pressure lance into molten iron, which removes sulfur impurities and excess carbon as the respective oxides, SO
₂ and CO
₂. The reactions are exothermic, so the temperature increases to 1,700 °C.^[67]

Another 25% of commercially produced oxygen is used by the chemical industry.^[67] Ethylene is reacted with O
₂ to create ethylene oxide, which, in turn, is converted into ethylene glycol; the primary feeder material used to manufacture a host of products, including antifreeze and polyester polymers (the precursors of many plastics and fabrics).^[67]

Most of the remaining 20% of commercially produced oxygen is used in medical applications, metal cutting and welding, as an oxidizer in rocket fuel, and in water treatment.^[67] Oxygen is used in oxyacetylene welding, burning acetylene with O
₂ to produce a very hot flame. In this process, metal up to 60 cm (24 in) thick is first heated with a small oxy-acetylene flame and then quickly cut by a large stream of O
₂.^[116]

Compounds

The oxidation state of oxygen is −2 in almost all known compounds of oxygen. The oxidation state −1 is found in a few compounds such as peroxides.^[117] Compounds containing oxygen in other oxidation states are very uncommon: −1/2 (superoxides), −1/3 (ozonides), 0 (elemental, hypofluorous acid), +1/2 (dioxygenyl), +1 (dioxygen difluoride), and +2 (oxygen difluoride).^[118]

Oxides and other inorganic compounds

Water (H
₂O) is an oxide of hydrogen and the most familiar oxygen compound. Hydrogen atoms are covalently bonded to oxygen in a water molecule but also have an additional attraction (about 23.3 kJ/mol per hydrogen atom) to an adjacent oxygen atom in a separate molecule.^[119] These hydrogen bonds between water molecules hold them approximately 15% closer than what would be expected in a simple liquid with just van der Waals forces.^[120][j]

Due to its electronegativity, oxygen forms chemical bonds with almost all other elements to give corresponding oxides. The surface of most metals, such as aluminium and titanium, are oxidized in the presence of air and become coated with a thin film of oxide that passivates the metal and slows further corrosion. Many oxides of the transition metals are non-stoichiometric compounds, with slightly less metal than the chemical formula would show. For example, the mineral FeO (wüstite) is written as , where x is usually around 0.05.^[121]

Oxygen is present in the atmosphere in trace quantities in the form of carbon dioxide (CO
₂). The Earth’s crustal rock is composed in large part of oxides of silicon (silica SiO
₂, as found in granite and quartz), aluminium (aluminium oxide Al
₂O
₃, in bauxite and corundum), iron (iron(III) oxide Fe
₂O
₃, in hematite and rust), and calcium carbonate (in limestone). The rest of the Earth’s crust is also made of oxygen compounds, in particular various complex silicates (in silicate minerals). The Earth’s mantle, of much larger mass than the crust, is largely composed of silicates of magnesium and iron.

Water-soluble silicates in the form of Na
₄SiO
₄, Na
₂SiO
₃, and Na
₂Si
₂O
₅ are used as detergents and adhesives.^[122]

Oxygen also acts as a ligand for transition metals, forming transition metal dioxygen complexes, which feature metal–O
₂. This class of compounds includes the heme proteins hemoglobin and myoglobin.^[123] An exotic and unusual reaction occurs with PtF
₆, which oxidizes oxygen to give O₂⁺PtF₆⁻, dioxygenyl hexafluoroplatinate.^[124]

Organic compounds

Among the most important classes of organic compounds that contain oxygen are (where «R» is an organic group): alcohols (R-OH); ethers (R-O-R); ketones (R-CO-R); aldehydes (R-CO-H); carboxylic acids (R-COOH); esters (R-COO-R); acid anhydrides (R-CO-O-CO-R); and amides (R-C(O)-NR
₂). There are many important organic solvents that contain oxygen, including: acetone, methanol, ethanol, isopropanol, furan, THF, diethyl ether, dioxane, ethyl acetate, DMF, DMSO, acetic acid, and formic acid. Acetone ((CH
₃)
₂CO) and phenol (C
₆H
₅OH) are used as feeder materials in the synthesis of many different substances. Other important organic compounds that contain oxygen are: glycerol, formaldehyde, glutaraldehyde, citric acid, acetic anhydride, and acetamide. Epoxides are ethers in which the oxygen atom is part of a ring of three atoms. The element is similarly found in almost all biomolecules that are important to (or generated by) life.

Oxygen reacts spontaneously with many organic compounds at or below room temperature in a process called autoxidation.^[125] Most of the organic compounds that contain oxygen are not made by direct action of O
₂. Organic compounds important in industry and commerce that are made by direct oxidation of a precursor include ethylene oxide and peracetic acid.^[122]

Safety and precautions

Oxygen

Hazards
GHS labelling:
Pictograms
Hazard statements	H272
Precautionary statements	P220, P244, P370+P376, P403
NFPA 704 (fire diamond)	0 0 1 OX

The NFPA 704 standard rates compressed oxygen gas as nonhazardous to health, nonflammable and nonreactive, but an oxidizer. Refrigerated liquid oxygen (LOX) is given a health hazard rating of 3 (for increased risk of hyperoxia from condensed vapors, and for hazards common to cryogenic liquids such as frostbite), and all other ratings are the same as the compressed gas form.^[126]

Toxicity

Oxygen gas (O
₂) can be toxic at elevated partial pressures, leading to convulsions and other health problems.^{[111][k][128]} Oxygen toxicity usually begins to occur at partial pressures more than 50 kilopascals (kPa), equal to about 50% oxygen composition at standard pressure or 2.5 times the normal sea-level O
₂ partial pressure of about 21 kPa. This is not a problem except for patients on mechanical ventilators, since gas supplied through oxygen masks in medical applications is typically composed of only 30–50% O
₂ by volume (about 30 kPa at standard pressure).^[8]

At one time, premature babies were placed in incubators containing O
₂-rich air, but this practice was discontinued after some babies were blinded by the oxygen content being too high.^[8]

Breathing pure O
₂ in space applications, such as in some modern space suits, or in early spacecraft such as Apollo, causes no damage due to the low total pressures used.^[109][129] In the case of spacesuits, the O
₂ partial pressure in the breathing gas is, in general, about 30 kPa (1.4 times normal), and the resulting O
₂ partial pressure in the astronaut’s arterial blood is only marginally more than normal sea-level O
₂ partial pressure.^[130]

Oxygen toxicity to the lungs and central nervous system can also occur in deep scuba diving and surface supplied diving.^[8][111] Prolonged breathing of an air mixture with an O
₂ partial pressure more than 60 kPa can eventually lead to permanent pulmonary fibrosis.^[131] Exposure to an O
₂ partial pressures greater than 160 kPa (about 1.6 atm) may lead to convulsions (normally fatal for divers). Acute oxygen toxicity (causing seizures, its most feared effect for divers) can occur by breathing an air mixture with 21% O
₂ at 66 m (217 ft) or more of depth; the same thing can occur by breathing 100% O
₂ at only 6 m (20 ft).^{[131][132][133][134]}

Combustion and other hazards

Highly concentrated sources of oxygen promote rapid combustion. Fire and explosion hazards exist when concentrated oxidants and fuels are brought into close proximity; an ignition event, such as heat or a spark, is needed to trigger combustion.^[31] Oxygen is the oxidant, not the fuel.

Concentrated O
₂ will allow combustion to proceed rapidly and energetically.^[31] Steel pipes and storage vessels used to store and transmit both gaseous and liquid oxygen will act as a fuel; and therefore the design and manufacture of O
₂ systems requires special training to ensure that ignition sources are minimized.^[31] The fire that killed the Apollo 1 crew in a launch pad test spread so rapidly because the capsule was pressurized with pure O
₂ but at slightly more than atmospheric pressure, instead of the 1⁄3 normal pressure that would be used in a mission.^[l][136]

Liquid oxygen spills, if allowed to soak into organic matter, such as wood, petrochemicals, and asphalt can cause these materials to detonate unpredictably on subsequent mechanical impact.^[31]

See also

Notes

References

General references

• Cook, Gerhard A.; Lauer, Carol M. (1968). «Oxygen». In Clifford A. Hampel (ed.). The Encyclopedia of the Chemical Elements. New York: Reinhold Book Corporation. pp. 499–512. LCCN 68-29938.
• Emsley, John (2001). «Oxygen». Nature’s Building Blocks: An A–Z Guide to the Elements. Oxford, England: Oxford University Press. pp. 297–304. ISBN 978-0-19-850340-8.
• Raven, Peter H.; Evert, Ray F.; Eichhorn, Susan E. (2005). Biology of Plants (7th ed.). New York: W. H. Freeman and Company Publishers. pp. 115–27. ISBN 978-0-7167-1007-3.

External links

• Oxygen at The Periodic Table of Videos (University of Nottingham)
• Oxidizing Agents > Oxygen
• Oxygen (O₂) Properties, Uses, Applications
• Roald Hoffmann article on «The Story of O»
• WebElements.com – Oxygen
• Oxygen on In Our Time at the BBC
• Scripps Institute: Atmospheric Oxygen has been dropping for 20 years

Строение атома кислорода

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Кислород (O) – жизненно важный газ, необходимый для дыхания, поддержания горения, окисления. Относится к группе халькогенов. Самый распространённый на Земле элемент. Строение атома кислорода позволяет ему соединяться с металлами и неметаллами, образуя оксиды.

Строение

По положению в периодической таблице Менделеева можно определить строение атома элемента кислорода. Это восьмой элемент, расположенный в VI группе, втором периоде. Относительная атомная масса – 16. Существует три изотопа элемента:

• ¹⁶O;
• ¹⁷O;
• ¹⁸O.

Наиболее распространён ¹⁶O.

Электронная конфигурация атома кислорода – 1s²2s²2p⁴. Ядро атома кислорода имеет заряд +8. Кислород относится к элементам р-семейства. На внешнем энергетическом уровне находится шесть валентных электронов. Два спаренных электрона находится на 2s-орбитали. На 2р-уровне находится два спаренных и два неспаренных электрона, поэтому во всех соединениях кислород проявляет вторую валентность.

Молекула кислорода имеет два атома – О₂. При присоединении ещё одного атома образуется озон – О₃.

Физические свойства

Кислород – бесцветный и безвкусный газ, плохо растворимый в воде и спирте. Хорошо растворим в жидком серебре. В сжиженном виде приобретает светло-голубой цвет, в твёрдом – синий. Занимает 21 % атмосферного воздуха.

Кислород поддерживает горение, поэтому его легко обнаружить с помощью тлеющей лучины (вспыхивает).

Химические свойства

Благодаря электронному строению обладает высокой степенью окисления. Однако большую активность проявляет при нагревании из-за прочных двойных связей между атомами. При комнатной температуре быстро реагирует с наиболее активными элементами – щелочными и щелочноземельными металлами, некоторыми неметаллами.

Соединяясь с элементами, образует оксиды. Окисляет органические вещества. Примеры реакций с простыми веществами:

• K + O₂ → KO₂;
• 3Fe + 2O₂ → Fe₃O₄;
• S + O₂ → SO₂.

С фосфором, серой, углеродом (графитом), водородом кислород реагирует при нагревании:

• 4Р + 5О₂ → 2Р₂О₅;
• S + O₂ → SO₂;
• С + О₂ → СО₂;
• 2Н₂ + О₂ → 2Н₂О.

Быстро пропуская фтор через щёлочь, получают реакцию кислорода с фтором:

2F₂ + 2NaOH → 2NaF + H₂O + OF₂.

Кислород с фтором непосредственно взаимодействует при электрическом разряде. В этом случае кислород играет роль восстановителя:

O₂ + F₂ → F₂O₂.

Кислород реагирует со сложными веществами, образуя оксиды:

• 2CuS + 3O₂ → 2CuO + 2SO₂;
• 2H₂S + 3O₂ → 2SO₂ + 2H₂O;
• 2C₆H₆ + 15O₂ → 12CO₂ + 6H₂O;
• CH₄ + 2O₂ → CO₂ + 2H₂O.

Кислород не реагирует с золотом и инертными газами. Взаимодействие с галогенами происходит в условиях ультрафиолета или электрического тока.

Что мы узнали?

Кислород – распространённый в природе бесцветный газ. Схема строения атома – +8 О)₂)₆. Кислород всегда проявляет валентность II за счёт двух неспаренных электронов. Кислород – сильный окислитель, проявляющий в некоторых реакциях свойства восстановителя. Взаимодействует с металлами и неметаллами, сложными неорганическими и органическими веществами. Наибольшую активность проявляет при нагревании. Не реагирует с благородными газами и золотом.

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Кислород, свойства атома, химические и физические свойства.

О 8  Кислород

15,99903-15,99977*     1s² 2s² 2p⁴

Кислород — элемент периодической системы химических элементов Д. И. Менделеева с атомным номером 8. Расположен в 16-й группе (по старой классификации — главной подгруппе шестой группы), втором периоде периодической системы.

Атом и молекула кислорода. Формула кислорода. Строение кислорода

Изотопы и модификации кислорода

Свойства кислорода (таблица): температура, плотность, давление и пр.

Физические свойства кислорода

Химические свойства кислорода. Взаимодействие кислорода. Реакции с кислородом

Получение кислорода

Применение кислорода

Таблица химических элементов Д.И. Менделеева

Атом и молекула кислорода. Формула кислорода. Строение кислорода:

Кислород – химический элемент периодической системы химических элементов Д. И. Менделеева с обозначением О и атомным номером 8. Расположен в 16-й группе (по старой классификации — главной подгруппе шестой группы), втором периоде периодической системы.

Кислород самый лёгкий элемент периодической таблицы химических элементов Д. И. Менделеева из группы халькогенов.

Кислород – химически активный неметалл.

Кислород обозначается символом О.

Как простое вещество кислород (химическая формула O₂) при нормальных условиях представляет собой двухатомный газ без цвета, вкуса и запаха. В жидком состоянии кислород имеет светло-голубой цвет, а в твёрдом – представляет собой кристаллы светло-синего цвета.

Молекула кислорода двухатомна. Также встречается аллотропная модификация кислорода – озон, молекула которого состоит из трёх атомов кислорода.

Химическая формула кислорода O₂ (или O₃ – озон).

Электронная конфигурация атома кислорода 1s² 2s² 2p⁴. Потенциал ионизации (первый электрон) атома кислорода равен 1313,94 кДж/моль (13,618055(7) эВ).

Строение атома кислорода. Атом кислорода (наиболее распространенный из трех изотопов кислорода (99,757 %) – ¹⁶₈О) состоит из положительно заряженного ядра (+8), вокруг которого по атомным оболочкам движутся восемь электронов. При этом 2 электрона находятся на внутреннем уровне, а 6 электронов – на внешнем. Поскольку кислород расположен во втором периоде, оболочки всего две. Первая – внутренняя оболочка представлена s-орбиталью. Вторая – внешняя оболочка представлена s- и р-орбиталями. Два спаренных электрона находится на 1s-орбитали, вторая пара электронов – на 2s-орбитали. На 2р-орбитали находится два спаренных и два неспаренных электрона. Поэтому во всех своих соединениях кислород проявляет валентность II. В свою очередь ядро атома кислорода состоит из восьми протонов и восьми нейтронов. Кислород относится к элементам p-семейства.

Радиус атома кислорода (вычисленный) составляет 48 пм.

Атомная масса атома кислорода составляет 15,99903-15,99977 а. е. м.

Кислород – самый распространённый химический элемент на Земле. В земной коре на его долю в составе различных соединений приходится около 46 % массы. Морские и пресные воды содержат по массе 86 % кислорода (если быть точнее – 85,82 %). В человеке его содержание составляет по массе 61 %. В атмосфере содержание свободного кислорода составляет 20,9476 % по объёму и 23,15 % по массе. На Солнце – 0,9 %, а во Вселенной – 1 %.

При высокой температуре молекула кислорода О₂ обратимо диссоциирует на атомарный кислород. При 2000 °C на атомарный кислород диссоциирует 0,03 % молекулярного кислорода, при 2600 °C – 1 %, при +4000 °C – 59 %, при 6000 °C — 99,5 %.

Изотопы и модификации кислорода:

Свойства кислорода (таблица): температура, плотность, давление и пр.

Подробные сведения на сайте ChemicalStudy.ru

100	Общие сведения*
101	Название	Кислород
102	Прежнее название
103	Латинское название	Oxygenium
104	Английское название	Oxygen
105	Символ	О
106	Атомный номер (номер в таблице)	8
107	Тип	Неметалл
108	Группа
109	Открыт	Карл Вильгельм Шееле, Швеция, 1771 г., Джозеф Пристли, Великобритания, 1 августа 1774 г.
110	Год открытия	1771 г.
111	Внешний вид и пр.	Газ без цвета, запаха и вкуса
112	Происхождение	Природный материал
113	Модификации
114	Аллотропные модификации	4 аллотропные модификации, обусловленные различным составом молекул: – кислород (O2), – озон (O3), – ε-кислород (O4 или O8) с простой моноклинной кристаллической решёткой, – ζ-кислород, металлическая фаза кислорода (On). 4 аллотропные модификации кислорода (O2), отличающихся строением кристаллической решётки: – α-кислород (α-O2) с простой моноклинной кристаллической  решёткой, – β-кислород (β-O2) с ромбоэдрической  (тригональной) кристаллической  решёткой, – γ-кислород (γ-O2) с простой кубической кристаллической  решёткой, – δ-кислород (δ-O2)
115	Температура и иные условия перехода аллотропных модификаций друг в друга
116	Конденсат Бозе-Эйнштейна
117	Двумерные материалы
118	Содержание в атмосфере и воздухе (по массе)	23,15 %
119	Содержание в земной коре (по массе)	46 %
120	Содержание в морях и океанах (по массе)	86 %
121	Содержание во Вселенной и космосе (по массе)	1 %
122	Содержание в Солнце (по массе)	0,9 %
123	Содержание в метеоритах (по массе)	40 %
124	Содержание в организме человека (по массе)	61 %
200	Свойства атома
201	Атомная масса (молярная масса)*	15,99903-15,99977 а. е. м. (г/моль)
202	Электронная конфигурация	1s2 2s2 2p4
203	Электронная оболочка	K2 L6 M0 N0 O0 P0 Q0 R0
204	Радиус атома (вычисленный)	48 пм
205	Эмпирический радиус атома	60 пм
206	Ковалентный радиус*	73 пм
207	Радиус иона (кристаллический)	O2- 124 (4) пм, 126 (6) пм, 128 (8) (в скобках указано координационное число – характеристика, которая определяет число ближайших частиц (ионов или атомов) в молекуле или кристалле)
208	Радиус Ван-дер-Ваальса	152 пм
209	Электроны, Протоны, Нейтроны	8 электронов, 8 протонов, 8 нейтронов
210	Семейство (блок)	элемент p-семейства
211	Период в периодической таблице	2
212	Группа в периодической таблице	16-ая группа (по старой классификации – главная подгруппа 6-ой группы)
213	Эмиссионный спектр излучения
300	Химические свойства
301	Степени окисления	-2, -1, -0,5, 0, +1, +2
302	Валентность	II
303	Электроотрицательность	3,44 (шкала Полинга)
304	Энергия ионизации (первый электрон)	1313,94 кДж/моль (13,618055(7) эВ)
305	Электродный потенциал	0 В
306	Энергия сродства атома к электрону	140,9760(2) кДж/моль (1,4611136(9) эВ) – кислород 16O, 140,9755(3) кДж/моль (1,461108(4) эВ) –кислород 17O, 140,9752(3) кДж/моль (1,461105(3) эВ) –кислород 18O
400	Физические свойства
401	Плотность*	0,001429 г/см3 (при 20 °C и иных стандартных условиях, состояние вещества – газ), 0,00142897 г/см3 (при 0 °C и иных стандартных условиях, состояние вещества – газ), 1,141 г/см³ (при  -183 °C и иных стандартных условиях, состояние вещества – жидкость), 1,27 г/см3 (при  -219 °C и иных стандартных условиях, состояние вещества – твердое тело)
402	Температура плавления*	-218,79 °C (54,36 K, -361,82 °F)
403	Температура кипения*	-182,962 °C (90,188 K, -297,332 °F)
404	Температура сублимации
405	Температура разложения
406	Температура самовоспламенения смеси газа с воздухом
407	Удельная теплота плавления (энтальпия плавления ΔHпл)*	0,444 кДж/моль
408	Удельная теплота испарения (энтальпия кипения ΔHкип)*	6,82 кДж/моль
409	Удельная теплоемкость при постоянном давлении	0,911 Дж/г·K (при 15 °C), 0,9125 Дж/г·K (при 100 °C), 0,915 Дж/г·K (при 200 °C), 0,926 Дж/г·K (при 400 °C), 0,938 Дж/г·K (при 600 °C)
410	Молярная теплоёмкость*	29,378 Дж/(K·моль)
411	Молярный объём	11,196 см³/моль
412	Теплопроводность	0,02658 Вт/(м·К) (при стандартных условиях), 0,027 Вт/(м·К) (при 300 K)
500	Кристаллическая решётка
511	Кристаллическая решётка #1	α-кислород (α-O2)
512	Структура решётки	Простая моноклинная
513	Параметры решётки	a = 5,403 Å, b = 3,429 Å, c = 5,086 Å, β = 135,53°
514	Отношение c/a
515	Температура Дебая	155 К
516	Название пространственной группы симметрии	C12/m1
517	Номер пространственной группы симметрии	12
521	Кристаллическая решётка #2	β-кислород (β-O2)
522	Структура решётки	Ромбоэдрическая (тригональная)
523	Параметры решётки	a = 4,21 Å, α = 46,25°
524	Отношение c/a
525	Температура Дебая
526	Название пространственной группы симметрии
527	Номер пространственной группы симметрии
531	Кристаллическая решётка #3	γ-кислород (γ-O2)
532	Структура решётки	Простая кубическая
533	Параметры решётки	a = 6,83 Å
534	Отношение c/a
535	Температура Дебая
536	Название пространственной группы симметрии
537	Номер пространственной группы симметрии
900	Дополнительные сведения
901	Номер CAS	7782-44-7

Примечание:

100* Данные в таблице приводятся применительно к кислороду (O₂).

201* Указан диапазон значений атомной массы в связи с различной распространённостью изотопов данного элемента в природе.

206* Ковалентный радиус кислорода согласно [1] составляет 66±2 пм.

401* Плотность кислорода согласно [1] составляет 0,001429 г/см³ (при 0 °C и иных стандартных условиях, состояние вещества – газ).

402* Температура плавления кислорода согласно [3] составляет -218,35 °C (54,8 K, -361,03 °F).

403* Температура кипения кислорода согласно [3] составляет -182,96 °C (90,19 K, -297,33 °F).

407* Удельная теплота плавления (энтальпия плавления ΔH_пл) кислорода согласно [4] составляет 0,446 кДж/моль.

408* Удельная теплота испарения (энтальпия кипения ΔH_кип) кислорода согласно [3] и [4] составляет 3,4099 кДж/моль и 6,828 кДж/моль соответственно.

410* Молярная теплоемкость кислорода согласно [3] составляет 29,4 Дж/(K·моль).

Физические свойства кислорода:

Химические свойства кислорода. Взаимодействие кислорода. Реакции с кислородом:

Получение кислорода:

Применение кислорода:

Таблица химических элементов Д.И. Менделеева

1. 1. Водород
2. 2. Гелий
3. 3. Литий
4. 4. Бериллий
5. 5. Бор
6. 6. Углерод
7. 7. Азот
8. 8. Кислород
9. 9. Фтор
10. 10. Неон
11. 11. Натрий
12. 12. Магний
13. 13. Алюминий
14. 14. Кремний
15. 15. Фосфор
16. 16. Сера
17. 17. Хлор
18. 18. Аргон
19. 19. Калий
20. 20. Кальций
21. 21. Скандий
22. 22. Титан
23. 23. Ванадий
24. 24. Хром
25. 25. Марганец
26. 26. Железо
27. 27. Кобальт
28. 28. Никель
29. 29. Медь
30. 30. Цинк
31. 31. Галлий
32. 32. Германий
33. 33. Мышьяк
34. 34. Селен
35. 35. Бром
36. 36. Криптон
37. 37. Рубидий
38. 38. Стронций
39. 39. Иттрий
40. 40. Цирконий
41. 41. Ниобий
42. 42. Молибден
43. 43. Технеций
44. 44. Рутений
45. 45. Родий
46. 46. Палладий
47. 47. Серебро
48. 48. Кадмий
49. 49. Индий
50. 50. Олово
51. 51. Сурьма
52. 52. Теллур
53. 53. Йод
54. 54. Ксенон
55. 55. Цезий
56. 56. Барий
57. 57. Лантан
58. 58. Церий
59. 59. Празеодим
60. 60. Неодим
61. 61. Прометий
62. 62. Самарий
63. 63. Европий
64. 64. Гадолиний
65. 65. Тербий
66. 66. Диспрозий
67. 67. Гольмий
68. 68. Эрбий
69. 69. Тулий
70. 70. Иттербий
71. 71. Лютеций
72. 72. Гафний
73. 73. Тантал
74. 74. Вольфрам
75. 75. Рений
76. 76. Осмий
77. 77. Иридий
78. 78. Платина
79. 79. Золото
80. 80. Ртуть
81. 81. Таллий
82. 82. Свинец
83. 83. Висмут
84. 84. Полоний
85. 85. Астат
86. 86. Радон
87. 87. Франций
88. 88. Радий
89. 89. Актиний
90. 90. Торий
91. 91. Протактиний
92. 92. Уран
93. 93. Нептуний
94. 94. Плутоний
95. 95. Америций
96. 96. Кюрий
97. 97. Берклий
98. 98. Калифорний
99. 99. Эйнштейний
100. 100. Фермий
101. 101. Менделеевий
102. 102. Нобелий
103. 103. Лоуренсий
104. 104. Резерфордий
105. 105. Дубний
106. 106. Сиборгий
107. 107. Борий
108. 108. Хассий
109. 109. Мейтнерий
110. 110. Дармштадтий
111. 111. Рентгений
112. 112. Коперниций
113. 113. Нихоний
114. 114. Флеровий
115. 115. Московий
116. 116. Ливерморий
117. 117. Теннессин
118. 118. Оганесон

Таблица химических элементов Д.И. Менделеева

Источники:

1. https://en.wikipedia.org/wiki/Oxygen
2. https://de.wikipedia.org/wiki/Sauerstoff
3. https://ru.wikipedia.org/wiki/Кислород
4. http://chemister.ru/Database/properties.php?dbid=1&id=218
5. https://chemicalstudy.ru/kislorod-svoystva-atoma-himicheskie-i-fizicheskie-svoystva/

Примечание: © Фото https://www.pexels.com, https://pixabay.com

кислород атомная масса степень окисления валентность плотность температура кипения плавления физические химические свойства структура теплопроводность электропроводность кристаллическая решетка
атом нарисовать строение число протонов в ядре строение электронных оболочек электронная формула конфигурация схема строения электронной оболочки заряд ядра состав масса орбита уровни модель радиус энергия электрона переход скорость спектр длина волны молекулярная масса объем атома
электронные формулы сколько атомов в молекуле кислорода
сколько электронов в атоме свойства металлические неметаллические термодинамические 

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