ᱦᱟᱭᱰᱨᱳᱡᱟᱱ

Hydrogen, ₁H
	Purple glow in its plasma state
Hydrogen
Appearance	colorless gas
Standard atomic weight Ar, std(H)	[1.00784, 1.00811] conventional: 1.008
Hydrogen in the periodic table
	– ← hydrogen → helium
Atomic number (Z)	1
Group	1: H and alkali metals
Period	period 1
Block	s-block
Element category	Reactive nonmetal
Electron configuration	1s1
Electrons per shell	1
Physical properties
Phase at STP	gas
Melting point	13.99 K (−259.16 °C, −434.49 °F)
Boiling point	20.271 K (−252.879 °C, −423.182 °F)
Density (at STP)	0.08988 g/L
when liquid (at m.p.)	0.07 g/cm3 (solid: 0.0763 g/cm3)
when liquid (at b.p.)	0.07099 g/cm3
Triple point	13.8033 K, 7.041 kPa
Critical point	32.938 K, 1.2858 MPa
Heat of fusion	(H2) 0.117 kJ/mol
Heat of	(H2) 0.904 kJ/mol
Molar heat capacity	(H2) 28.836 J/(mol·K)
Atomic properties
Oxidation states	−1, +1 (an amphoteric oxide)
Electronegativity	Pauling scale: 2.20
energies	1st: 1312.0 kJ/mol ; ;
Covalent radius	31±5 pm
Van der Waals radius	120 pm
	Spectral lines of hydrogen
Other properties
Natural occurrence	primordial
Crystal structure	hexagonal
Speed of sound	1310 m/s (gas, 27 °C)
Thermal conductivity	0.1805 W/(m·K)
Magnetic ordering	diamagnetic
Magnetic susceptibility	−3.98·10−6 cm3/mol (298 K)
CAS Number	12385-13-6 ; 1333-74-0 (H2)
History
Discovery	Henry Cavendish (1766)
Named by	Antoine Lavoisier (1783)
Main isotopes of hydrogen
	view; talk; edit; \| references

ᱪᱷᱟᱸᱪ:Testcases other

ᱦᱟᱭᱰᱨᱳᱡᱟᱱ ᱫᱚ ᱢᱤᱫ ᱠᱮᱢᱤᱠᱟᱞ ᱤᱞᱤᱢᱮᱱᱴ ᱠᱟᱱᱟ ᱱᱚᱶᱟ ᱨᱮᱱᱟᱜ ᱠᱷᱟᱴᱚ ᱪᱤᱛᱟᱹᱨ ᱫᱚ H ᱠᱟᱱᱟ ᱟᱨ ᱱᱚᱶᱟ ᱨᱮᱱᱟᱜ ᱮᱴᱳᱢᱤᱠ ᱞᱮᱠᱷᱟ ᱫᱚ ᱑ ᱠᱟᱱᱟ ᱾ ᱱᱚᱶᱟ ᱨᱮᱱᱟᱜ ᱦᱟᱢᱟᱞ ᱑ᱹ᱐᱐᱘ ᱠᱟᱱᱟ, ᱦᱟᱭᱰᱨᱳᱡᱟᱱ ᱫᱚ ᱯᱮᱨᱤᱭᱳᱰᱤᱠ ᱴᱮᱵᱟᱞ ᱨᱮᱱᱟᱜ ᱥᱟᱱᱟᱢ ᱠᱷᱚᱱ ᱪᱮᱛᱟᱱ ᱤᱞᱤᱢᱮᱱᱴ ᱠᱟᱱᱟ ᱾ ᱦᱟᱭᱰᱨᱳᱡᱟᱱ ᱫᱚ ᱠᱚᱱᱥᱴᱤᱴᱭᱩᱴᱤᱝ ᱨᱮᱯᱷᱞᱤ ᱨᱮ ᱗᱕% ᱠᱮᱢᱤᱠᱟᱞ ᱥᱟᱵᱽᱥᱴᱟᱱᱥ ᱨᱮᱱᱟᱜ ᱵᱟᱨᱭᱳᱱᱤᱠ ᱢᱟᱥ ᱠᱟᱱᱟ ᱾^[᱗]^{[note ᱑]}

H⁺^[᱘]

ᱛᱟᱦᱮᱱᱟ

ᱱᱚᱶᱟ ᱫᱚ ᱡᱟᱦᱟᱸ ᱨᱮᱜᱮ ᱦᱟᱭᱰᱨᱳᱡᱟᱱ ᱢᱟᱨᱟᱝ ᱥᱟᱨᱮᱡ ᱢᱚᱛᱨᱚ ᱨᱮ ᱫᱟ ᱦᱚᱭ ᱨᱮ ᱧᱟᱢᱚᱜᱚᱜ ᱠᱟᱱᱟ ᱾ ᱪᱮᱛᱟᱱ ᱦᱚᱭ ᱨᱮ ᱱᱚᱶᱟ ᱨᱮᱱᱟᱜ ᱢᱚᱛᱨᱚ ᱟᱱᱟ ᱠᱷᱚᱱ ᱦᱚᱸ ᱵᱟᱹᱲᱛᱤ ᱛᱟᱦᱮᱱ ᱠᱟᱱᱟ ᱾ ᱥᱤᱧ ᱪᱟᱸᱫᱚ ᱣᱟᱜ ᱯᱚᱨᱤᱢᱟᱱᱰᱮᱨ ᱨᱮ ᱱᱚᱶᱟ ᱨᱮᱱᱟᱜ ᱵᱟᱹᱲᱛᱤ ᱢᱮᱱᱟᱜᱼᱟ ᱾ ᱫᱷᱟᱹᱨᱛᱤ ᱨᱮ ᱥᱮᱞᱮᱫ ᱫᱚᱥᱟ ᱨᱮ ᱱᱚᱶᱟ ᱫᱟᱜ, ᱫᱟᱨᱮ, ᱡᱤᱭᱟᱞᱤ ᱴᱤᱥᱩ, ᱠᱟᱥᱴᱷ, ᱟᱱᱟᱡᱽ, ᱥᱩᱱᱩᱢ, ᱯᱷᱮᱴᱥ, ᱯᱮᱴᱨᱳᱞᱤᱭᱚᱢ, ᱥᱟᱱᱟᱢ ᱡᱤᱣᱮᱫ ᱢᱮᱴᱟᱨ ᱨᱮ ᱧᱟᱢᱚᱜᱚᱜᱼᱟ ᱾ ᱮᱥᱤᱰ ᱨᱮᱱᱟᱜ ᱱᱚᱶᱟ ᱞᱟᱠᱛᱤᱭᱟᱱ ᱜᱷᱟᱴᱚᱠ ᱠᱚ ᱠᱟᱱᱟ ᱾ ᱵᱮᱥ (Base) ᱟᱨ ᱳᱨᱜᱮᱱᱤᱠ ᱠᱚᱢᱯᱣᱩᱱᱰ ᱨᱮ ᱦᱚᱸ ᱱᱚᱶᱟ ᱧᱟᱢᱚᱜᱚᱜ ᱠᱟᱱᱟ ᱾

ᱨᱤᱭᱮᱠᱥᱚᱱ ᱨᱮᱱᱟᱜ ᱛᱟᱞᱠᱟ

H₂+Cl₂ -> 2HCl
2H₂+O₂ -> 2H₂O

ᱯᱨᱳᱥᱮᱥ

Hydrogen spectrum test

ᱱᱮᱪᱩᱨᱟᱞ ᱜᱮᱥ ᱫᱚ ᱞᱚᱞᱚ ᱟᱨ ᱟᱫᱷᱟᱱ ᱟᱭᱢᱟ ᱜᱟᱱ ᱯᱨᱳᱥᱮᱥ ᱛᱮ ᱪᱟᱞᱟᱜ ᱠᱟᱱ ᱨᱮ ᱦᱟᱭᱰᱨᱳᱡᱟᱱ ᱟᱨ ᱠᱟᱨᱵᱚᱱ ᱢᱳᱱᱳᱟᱹᱠᱥᱟᱭᱤᱰ ᱨᱮᱱᱟᱜ ᱢᱮᱥᱟ ᱧᱟᱢᱚᱜ ᱠᱟᱱᱟ
CH₄+H₂O -> CO + 3H₂

ᱵᱟᱦᱨᱮ ᱡᱚᱱᱚᱲ

https://web.archive.org/web/20100125010949/http://www.bbc.co.uk

ᱥᱟᱹᱠᱷᱭᱟᱹᱛ

↑ Wiberg, Egon; Wiberg, Nils; Holleman, Arnold Frederick (2001). Inorganic chemistry. Academic Press. p. 240. ISBN 978-0123526519.
↑ Lide, D. R., ed. (2005). "Magnetic susceptibility of the elements and inorganic compounds". CRC Handbook of Chemistry and Physics (PDF) (86th ed.). Boca Raton (FL): CRC Press. ISBN 978-0-8493-0486-6.
↑ Weast, Robert (1984). CRC, Handbook of Chemistry and Physics. Boca Raton, Florida: Chemical Rubber Company Publishing. pp. E110. ISBN 978-0-8493-0464-4.
↑ "Hydrogen". Van Nostrand's Encyclopedia of Chemistry. Wylie-Interscience. 2005. pp. 797–799. ISBN 978-0-471-61525-5.
↑ Emsley, John (2001). Nature's Building Blocks. Oxford: Oxford University Press. pp. 183–191. ISBN 978-0-19-850341-5.
↑ Stwertka, Albert (1996). A Guide to the Elements. Oxford University Press. pp. 16–21. ISBN 978-0-19-508083-4.
↑ Boyd, Padi (19 ᱡᱩᱞᱟᱭ 2014). "What is the chemical composition of stars?". NASA. Archived from the original on 15 ᱡᱟᱱᱩᱣᱟᱨᱤ 2015. Retrieved 5 ᱯᱷᱮᱵᱽᱨᱩᱣᱟᱨᱤ 2008.
↑ Laursen, S.; Chang, J.; Medlin, W.; Gürmen, N.; Fogler, H. S. (27 ᱡᱩᱞᱟᱭ 2004). "An extremely brief introduction to computational quantum chemistry". Molecular Modeling in Chemical Engineering. University of Michigan. Archived from the original on 20 ᱢᱮ 2015. Retrieved 4 ᱢᱮ 2015.

Preview of references

↑ However, most of the universe's mass is not in the form of baryons or chemical elements. See dark matter and dark energy.

[1] Wiberg, Egon; Wiberg, Nils; Holleman, Arnold Frederick (2001). Inorganic chemistry. Academic Press. p. 240. ISBN 978-0123526519.

[2] Lide, D. R., ed. (2005). "Magnetic susceptibility of the elements and inorganic compounds". CRC Handbook of Chemistry and Physics (PDF) (86th ed.). Boca Raton (FL): CRC Press. ISBN 978-0-8493-0486-6.

[3] Weast, Robert (1984). CRC, Handbook of Chemistry and Physics. Boca Raton, Florida: Chemical Rubber Company Publishing. pp. E110. ISBN 978-0-8493-0464-4.

[Nostrand-4] "Hydrogen". Van Nostrand's Encyclopedia of Chemistry. Wylie-Interscience. 2005. pp. 797–799. ISBN 978-0-471-61525-5.

[nbb-5] Emsley, John (2001). Nature's Building Blocks. Oxford: Oxford University Press. pp. 183–191. ISBN 978-0-19-850341-5.

[Stwertka-6] Stwertka, Albert (1996). A Guide to the Elements. Oxford University Press. pp. 16–21. ISBN 978-0-19-508083-4.

[7] Boyd, Padi (19 ᱡᱩᱞᱟᱭ 2014). "What is the chemical composition of stars?". NASA. Archived from the original on 15 ᱡᱟᱱᱩᱣᱟᱨᱤ 2015. Retrieved 5 ᱯᱷᱮᱵᱽᱨᱩᱣᱟᱨᱤ 2008.

[Laursen04-9] Laursen, S.; Chang, J.; Medlin, W.; Gürmen, N.; Fogler, H. S. (27 ᱡᱩᱞᱟᱭ 2004). "An extremely brief introduction to computational quantum chemistry". Molecular Modeling in Chemical Engineering. University of Michigan. Archived from the original on 20 ᱢᱮ 2015. Retrieved 4 ᱢᱮ 2015.

[8] However, most of the universe's mass is not in the form of baryons or chemical elements. See dark matter and dark energy.

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