Hydrogen (H)
nonmetalGas
मानक परमाणु भार
1.008 u [1.00784, 1.00811]इलेक्ट्रॉन विन्यास
1s1गलनांक
-259.34 °Cक्वथनांक
-252.87 °Cघनत्व
0.08988 kg/m³ऑक्सीकरण अवस्थाएँ
−1, +1विद्युतऋणात्मकता (पॉलिंग)
2.2आयनन ऊर्जा (प्रथम)
13.598435 eVखोज का वर्ष
1766परमाणु त्रिज्या
25 pmविवरण
The lightest chemical element, hydrogen sits above the alkali metals but is a nonmetal under ordinary conditions. Its single proton and one electron make it the simplest atom and a reference point for much of chemistry. On Earth it is usually bound in water and organic matter, while industry uses it as a chemical feedstock, reducing agent, fuel, and energy carrier.
Colourless, odourless gaseous chemical element. Lightest and most abundant element in the universe. Present in water and in all organic compounds. Chemically reacts with most elements. Discovered by Henry Cavendish in 1776.
The name derives from the Greek hydro for "water" and genes for "forming" because it burned in air to form water. Hydrogen was discovered by the English physicist Henry Cavendish in 1766.
Scientists had been producing hydrogen for years before it was recognized as an element. Written records indicate that Robert Boyle produced hydrogen gas as early as 1671 while experimenting with iron and acids. Hydrogen was first recognized as a distinct element by Henry Cavendish in 1766. Composed of a single proton and a single electron, hydrogen is the simplest and most abundant element in the universe. It is estimated that 90% of the visible universe is composed of hydrogen.
Hydrogen is the raw fuel that most stars 'burn' to produce energy. The same process, known as fusion, is being studied as a possible power source for use on earth. The sun's supply of hydrogen is expected to last another 5 billion years.
From the Greek word hydro (water), and genes (forming). Hydrogen was recognized as a distinct substance by Henry Cavendish in 1776. Diagram of a simple hydrogen atom.
Hydrogen is the most abundant of all elements in the universe. The heavier elements were originally made from hydrogen atoms or from other elements that were originally made from hydrogen atoms.
Pure hydrogen at room temperature is a colorless, odorless, tasteless gas. It has no luster or visible texture and is much less dense than air. Liquid hydrogen is also colorless, forming only at very low temperatures near −253 °C under normal pressure.
Most hydrogen is used in chemical industry rather than burned as a fuel. It is essential for ammonia production by the Haber-Bosch process, petroleum refining, methanol manufacture, and hydrogenation of oils and other chemicals. It is also used in fuel cells, rocket propellants, metal processing, protective atmospheres, and laboratory work. Everyday life encounters hydrogen mainly through water, fuels, plastics, foods, and organic molecules.
Hydrogen is a commercially important element. Large amounts of hydrogen are combined with nitrogen from the air to produce ammonia (NH3) through a process called the Haber process. Hydrogen is also added to fats and oils, such as peanut oil, through a process called hydrogenation. Liquid hydrogen is used in the study of superconductors and, when combined with liquid oxygen, makes an excellent rocket fuel.
Hydrogen combines with other elements to form numerous compounds. Some of the common ones are: water (H2O), ammonia (NH3), methane (CH4), table sugar (C12H22O11), hydrogen peroxide (H2O2) and hydrochloric acid (HCl).
Hydrogen has three common isotopes. The simplest isotope, called protium, is just ordinary hydrogen. The second, a stable isotope called deuterium, was discovered in 1932. The third isotope, tritium, was discovered in 1934.
Great quantities of hydrogen are required commercially for nitrogen fixation using the Haber ammonia process, and for the hydrogenation of fats and oils. It is also used in large quantities in methanol production, in hydrodealkylation, hydrocracking, and hydrodesulfurization. Other uses include rocket fuel, welding, producing hydrochloric acid, reducing metallic ores, and filling balloons.
The lifting power of 1 cubic foot of hydrogen gas is about 0.07 lb at °C, 760 mm pressure.
The hydrogen fuel cell is a developing technology that will allow great amounts of electrical power to be obtained using a source of hydrogen gas.
Consideration is being given to an entire economy based on solar- and nuclear-generated hydrogen. Public acceptance, high capital investment, and the high cost of hydrogen with respect to today's fuels are but a few of the problems facing such an economy. Located in remote regions, power plants would electrolyze seawater; the hydrogen produced would travel to distant cities by pipelines. Pollution-free hydrogen could replace natural gas, gasoline, etc., and could serve as a reducing agent in metallurgy, chemical processing, refining, etc. It could also be used to convert trash into methane and ethylene.
Isotopes in Earth/Planetary Science
Molecules, atoms, and ions of the stable isotopes of hydrogen possess slightly different physical and chemical properties and they are commonly fractionated during physical, chemical, and biological processes, giving rise to variations in isotopic abundances and in atomic weights (Fig. IUPAC.1.1). Hydrogen has the largest relative mass difference among its isotopes and consequently exhibits the largest variation in isotopic composition of any element that does not have radioactive or radiogenic isotopes. Ranges in the stable isotopic composition of naturally occurring hydrogen-bearing materials are shown in Fig. IUPAC.1.1. These variations enable hydrogen isotopes to be used as tracers in environmental studies [13] M. W. Wieser, T. B. Coplen. Pure Appl Chem.83, 359 (2011)..
A primary use of stable hydrogen isotopes is in isotope hydrology. Although the evolution of the stable hydrogen and oxygen isotopic composition of precipitation begins with the evaporation of water from the oceans, their local and global relationship arises primarily from equilibrium isotopic fractionation of heavier (2H and 18O) and lighter (1H and 16O) isotopes of hydrogen and oxygen during condensation as a tropospheric vapor mass follows a trajectory to higher latitudes and over continents [14] W. Dansgaard. Tellus16, 436 (1964)., [15] I. D. Clark, P. Fritz. Environmental Isotopes in Hydrogeology, p. 328, Lewis Publishers, New York (1997).. As a consequence, the hydrogen isotopic composition of precipitation, rivers, and tap waters varies with elevation, season, and distance from the ocean-continent boundary. Figure 4.1.2 shows the variation in the atomic weight of hydrogen in water from rivers across the United States. These variations in the hydrogen isotopic composition of environmental water are often combined with stable oxygen isotopic compositions and have been used to identify the origin of water samples and to investigate the interaction between groundwater and surface water (e.g. lakes, streams, and rivers) [16] C. Kendall, T. B. Coplen. Hydrol. Processes.15, 1363 (2011)..
Isotopes in Forensic Science and Anthropology
Measurements of relative 2H abundances are used to determine the breeding grounds of many species of migrant songbirds. These species of songbirds only grow their feathers before migration, and they grow them on or close to their breeding grounds. Therefore, the isotopic composition of a bird’s feathers correlates to the isotopic composition of the growing season’s precipitation [18] Z. D. Sharp, V. Atudorei, H. O. Panarello, J. Fernández, C. Douthitt. J. Archaeolog. Sci.30, 1709 (2003)., [19] K. A. Hobson. Oecologia120, 314 (1999)., [20] K. A. Hobson, L. I. Wassenaar. Oecologia.109, 142 (1996)..
Measurements of relative 2H abundances of human hair samples collected at archeological sites are used to determine the geographic region in which a subject lived based on the hydrogen isotopic composition of the water they drank. This is possible because hair stores a daily record of the hydrogen isotopic composition of intake water, which correlates to local meteoric water [18] Z. D. Sharp, V. Atudorei, H. O. Panarello, J. Fernández, C. Douthitt. J. Archaeolog. Sci.30, 1709 (2003)., [21] T. B. Coplen, H. Qi. Forensic Sci. Int.266, 222 (2016)..
Isotopes in Geochronology
3H (tritium), with a half-life of 12.31 years, decays to 3He. The relative variations in n(3He)/n(3H) ratios can be interpreted in terms of elapsed time for dating purposes. The dates of groundwater recharge (water moving downward from the surface), where large amounts of 3H were received from precipitation following thermonuclear bomb test periods, come from the elapsed time since a water mass became isolated from the atmosphere in the time range from the mid-1950s to the present [15] I. D. Clark, P. Fritz. Environmental Isotopes in Hydrogeology, p. 328, Lewis Publishers, New York (1997)..
Isotopes in Industry
3H is used for self-luminous exit signs in aircraft and commercial buildings. It is found in luminous dials, gauges, wristwatches, and luminous paints [22] United States Nuclear Regulatory Commission. NRC: Fact Sheet on Tritium Exit Signs, (2013), November 12; http://www.nrc.gov/reading-rm/doc-collections/fact-sheets/fs-tritium.html.. 2H, in the form of heavy water, is used in CANDU (CANada Deuterium Uranium) nuclear reactors as a moderator and coolant [23] CANDU Owners Group Inc. CANDU Reactors, CANDU Owners Group Inc (2013), July 30; http://www.candu.org/candu_reactors.html..
Isotopes in Medicine
2H is used for the isotopic labeling of drugs and nutrients to trace their uptake and metabolism in the human body [24] S. P. O’Grady, A. R. Wende, C. H. Remien, L. O. Valenzuela, L. E. Enright, L. A. Chesson, E. D. Abel, T. E. Cerling, J. R. Ehleringer. PLoS One5, e11699 (2010). https://doi.org/10.1371/journal.pone.0011699., [25] M. van Lieshout, C. E. West, R. B. van Breemen. Am. J. Clin. Nutr.77, 12 (2003).. 2H, in the form of heavy water, is used to study human metabolism. For example, 2H is used in combination with 18O (double labeled water) to measure energy expenditure [26] D. A. Schoeller, E. Ravussin, Y. Schutz, K. J. Acheson, P. Baertschi, E. Jequier. Am. J. Physiol. Regul. Integr. Comp. Physiol.250, R823 (1986)..
Water (H₂O) is the most familiar hydrogen compound and the main reservoir of hydrogen at Earth’s surface. Methane (CH₄) is a major fuel and carbon feedstock. Ammonia (NH₃) is central to fertilizers and nitrogen chemistry. Hydrogen chloride (HCl) forms hydrochloric acid in water. Hydrogen peroxide (H₂O₂) is used as an oxidizer and disinfectant. Metal hydrides store or transfer hydrogen in some chemical and technical systems.
Although pure hydrogen is a gas, we find very little of it in our atmosphere. Hydrogen gas is so light that, uncombined, hydrogen will gain enough velocity from collisions with other gases that they will quickly be ejected from the atmosphere. On earth, hydrogen occurs chiefly in combination with oxygen in water, but it is also present in organic matter such as living plants, petroleum, coal, etc. It is present as the free element in the atmosphere, but only less than 1 ppm by volume. The lightest of all gases, hydrogen combines with other elements sometimes explosively to form compounds.
Quite apart from isotopes, it has been shown that under ordinary conditions hydrogen gas is a mixture of two kinds of molecules, known as ortho- and para-hydrogen, which differ from one another by the spins of their electrons and nuclei.
Normal hydrogen at room temperature contains 25% of the para form and 75% of the ortho form. The ortho form cannot be prepared in the pure state. Since the two forms differ in energy, the physical properties also differ. The melting and boiling points of parahydrogen are about 0.1°C lower than those of normal hydrogen.
See more information at the Hydrogen compound page.
Hydrogen is not toxic and is not radioactive, but it is highly flammable. Mixtures with air ignite over a broad concentration range, and the flame can be nearly invisible in daylight. Leaks disperse upward quickly but can accumulate under ceilings or in confined spaces. Compressed and liquid hydrogen add pressure, cryogenic, and embrittlement hazards. Oxygen displacement is possible in poorly ventilated areas.
Free hydrogen occurs naturally in small amounts from geological reactions, biological activity, and atmospheric chemistry, but it does not persist long near the surface. It is not known to bioaccumulate. Environmental effects depend strongly on how it is produced: steam methane reforming releases carbon dioxide unless captured, while electrolysis depends on the electricity source. Leaked hydrogen can affect atmospheric chemistry indirectly.
Hydrogen is produced at large scale, mainly from natural gas by steam methane reforming and from coal gasification in some regions; electrolysis is smaller but growing where low-carbon electricity is available. Major demand comes from ammonia, refining, methanol, and emerging fuel-cell and synthetic-fuel uses. Costs depend on energy prices, carbon policy, electrolyzer costs, transport, storage, and purity requirements. Because hydrogen is difficult to liquefy and has low volumetric energy density, infrastructure often shapes markets as much as production. Recycling is limited, but industrial off-gases are sometimes recovered and purified.
Hydrogen is estimated to make up more than 90% of all the atoms three quarters of the mass of the universe! This element is found in the stars, and plays an important part in powering the universe through both the proton-proton reaction and carbon-nitrogen cycle. Stellar hydrogen fusion processes release massive amounts of energy by combining hydrogens to form helium.
Production of hydrogen in the U.S. alone amounts to about 3 billion cubic feet per year. Hydrogen is prepared by
▸ steam on heated carbon,
▸ decomposition of certain hydrocarbons with heat,
▸ reaction of sodium or potassium hydroxide on aluminum
▸ electrolysis of water, or
▸ displacement from acids by certain metals.
Liquid hydrogen is important in cryogenics and in the study of superconductivity, as its melting point is only 20 degrees above absolute zero.
Tritium is readily produced in nuclear reactors and is used in the production of the hydrogen bomb.
Hydrogen is the primary component of Jupiter and the other gas giant planets. At some depth in the planet's interior the pressure is so great that solid molecular hydrogen is converted to solid metallic hydrogen.
In 1973, a group of Russian experimenters may have produced metallic hydrogen at a pressure of 2.8 Mbar. At the transition the density changed from 1.08 to 1.3 g/cm3. Earlier, in 1972, at Livermore, California, a group also reported on a similar experiment in which they observed a pressure-volume point centered at 2 Mbar. Predictions say that metallic hydrogen may be metastable; others have predicted it would be a superconductor at room temperature.
Most hydrogen formed in the first minutes after the Big Bang as protons combined with electrons later to make neutral atoms. It is the most abundant element in the universe and the main fuel of stars, where fusion converts hydrogen into helium. Hydrogen dominates gas giants, interstellar clouds, and much of the raw material from which new stars and planetary systems form.
- A hydrogen atom has no neutron in its most common isotope, protium.
- Liquid hydrogen is one of the coldest industrial liquids in regular use.
- Hydrogen gas is so light that Earth’s gravity cannot retain much of it over geological time.
- The Sun consumes hundreds of millions of tonnes of hydrogen each second through fusion.
- Hydrogen can behave like a metal only under extreme pressures, a state studied in giant planets and high-pressure laboratories.
चित्र
गुण
भौतिक
- परमाणु त्रिज्या (आनुभविक)
- 25 pm सभी तत्वों की परमाणु त्रिज्या (आनुभविक) की तुलना करें →
- सहसंयोजक त्रिज्या
- 31 pm सभी तत्वों की सहसंयोजक त्रिज्या की तुलना करें →
- वान डर वाल्स त्रिज्या
- 120 pm सभी तत्वों की वान डर वाल्स त्रिज्या की तुलना करें →
- घनत्व
- 0.08988 kg/m³ सभी तत्वों की घनत्व की तुलना करें →
- मोलर आयतन
- 0.0141 L/mol
- STP पर प्रावस्था
- गैस सभी तत्वों की STP पर प्रावस्था की तुलना करें →
- गलनांक
- -259.34 °C सभी तत्वों की गलनांक की तुलना करें →
- क्वथनांक
- -252.87 °C सभी तत्वों की क्वथनांक की तुलना करें →
- तापीय चालकता
- 0.181 W/(m·K) सभी तत्वों की तापीय चालकता की तुलना करें →
- विशिष्ट ऊष्मा धारिता
- 14.304 J/(g·K) सभी तत्वों की विशिष्ट ऊष्मा धारिता की तुलना करें →
- मोलर ऊष्मा धारिता
- 28.836 J/(mol·K) सभी तत्वों की मोलर ऊष्मा धारिता की तुलना करें →
- क्रिस्टल संरचना
- षट्कोणीय सघन संकुलित सभी तत्वों की क्रिस्टल संरचना की तुलना करें →
रासायनिक
- विद्युतऋणात्मकता (पॉलिंग)
- 2.2 सभी तत्वों की विद्युतऋणात्मकता (पॉलिंग) की तुलना करें →
- विद्युतऋणात्मकता (ऐलन)
- 2.3
- इलेक्ट्रॉन बंधुता
- 0.75419 eV
- आयनन ऊर्जा (प्रथम)
- 13.598435 eV सभी तत्वों की आयनन ऊर्जा (प्रथम) की तुलना करें →
- ऑक्सीकरण अवस्थाएँ
- −1, +1 सभी तत्वों की ऑक्सीकरण अवस्थाएँ की तुलना करें →
- संयोजकता इलेक्ट्रॉन
- 1 सभी तत्वों की संयोजकता इलेक्ट्रॉन की तुलना करें →
- इलेक्ट्रॉन विन्यास
- 1s1
ऊष्मागतिक
- त्रिक बिंदु (तापमान)
- -259.3467 °C
- त्रिक बिंदु (दाब)
- 7041 Pa
- क्रांतिक बिंदु (तापमान)
- -240.212 °C
- क्रांतिक बिंदु (दाब)
- 1.2858e+6 Pa
- गलन ऊष्मा
- 0.00121262 eV सभी तत्वों की गलन ऊष्मा की तुलना करें →
- वाष्पन ऊष्मा
- 0.00936933 eV सभी तत्वों की वाष्पन ऊष्मा की तुलना करें →
- परमाणुकरण ऊष्मा
- 2.259398 eV
- परमाणुकरण एन्थैल्पी
- 2.259398 eV
नाभिकीय
- प्रोटॉन
- 1 सभी तत्वों की प्रोटॉन की तुलना करें →
- न्यूट्रॉन
- 0 सभी तत्वों की न्यूट्रॉन की तुलना करें →
- ज्ञात समस्थानिक
- 7 सभी तत्वों की ज्ञात समस्थानिक की तुलना करें →
- स्थिर समस्थानिक
- 2 सभी तत्वों की स्थिर समस्थानिक की तुलना करें →
- सबसे स्थिर समस्थानिक
- H-1
- खोज का वर्ष
- 1766
प्रचुरता
- प्रचुरता (भूपर्पटी)
- 1400 mg/kg सभी तत्वों की प्रचुरता (भूपर्पटी) की तुलना करें →
- प्रचुरता (महासागर)
- 1.08 × 105 mg/L सभी तत्वों की प्रचुरता (महासागर) की तुलना करें →
क्रिस्टल संरचना
- जालक स्थिरांक a
- 375 pm
इलेक्ट्रॉनिक संरचना
- प्रति कोश इलेक्ट्रॉन
- 1 सभी तत्वों की प्रति कोश इलेक्ट्रॉन की तुलना करें →
पहचानकर्ता
- CAS संख्या
- 1333-74-0 सभी तत्वों की CAS संख्या की तुलना करें →
- टर्म प्रतीक
- 2S1/2
- InChI
- InChI=1S/H
- InChI कुंजी
- YZCKVEUIGOORGS-UHFFFAOYSA-N
इलेक्ट्रॉन विन्यास मापित
H: 1s¹1s¹1s¹परमाणु मॉडल
समस्थानिक न्यूट्रॉन की संख्या, द्रव्यमान और स्थिरता बदलते हैं — उदासीन परमाणु का इलेक्ट्रॉन विन्यास नहीं।
सांकेतिक परमाणु मॉडल, वास्तविक अनुपात में नहीं।
परमाणु पहचान-चिह्न
उत्सर्जन / अवशोषण स्पेक्ट्रम
समस्थानिक वितरण
| द्रव्यमान संख्या | परमाणु द्रव्यमान (u) | प्राकृतिक प्रचुरता | अर्धायु |
|---|---|---|---|
| 1 स्थिर | 1.00782503223 ± 0.00000000009 | 99.9885% | स्थिर |
| 2 स्थिर | 2.01410177812 ± 0.00000000012 | 0.0115% | स्थिर |
प्रावस्था / अवस्था
कारण: क्वथनांक (-252.87 °C) से 277.9 °C अधिक
सांकेतिक, वास्तविक अनुपात में नहीं
प्रावस्था संक्रमण बिंदु
संक्रमण ऊर्जाएँ
गलनांक पर 1 mol को पिघलाने के लिए आवश्यक ऊर्जा
क्वथनांक पर 1 mol को वाष्पित करने के लिए आवश्यक ऊर्जा
घनत्व
मानक परिस्थितियों में
वर्तमान T पर आदर्श गैस नियम से अनुमानित
उन्नत
परमाणु स्पेक्ट्रम
उपलब्ध स्पेक्ट्रमी रेखा डेटा ?
| आयन | आवेश | कुल रेखाएँ | संक्रमण प्रायिकताएँ | स्तर पदनाम |
|---|---|---|---|---|
| D I समस्थानिक | 0 | 364 | 161 | 341 |
| H I | 0 | 568 | 441 | 535 |
| T I समस्थानिक | 0 | 11 | 11 | 11 |
उपलब्ध ऊर्जा स्तर डेटा ?
| आयन | आवेश | स्तर |
|---|---|---|
| D I समस्थानिक | 0 | 78 |
| H I | 0 | 106 |
| T I समस्थानिक | 0 | 10 |
यौगिक
समस्थानिक (2)
The ordinary isotope of hydrogen, H, is known as Protium, the other two isotopes are Deuterium (a proton and a neutron) and Tritium (a protron and two neutrons). Hydrogen is the only element whose isotopes have been given different names. Deuterium and Tritium are both used as fuel in nuclear fusion reactors. One atom of Deuterium is found in about 6000 ordinary hydrogen atoms.
| द्रव्यमान संख्या | परमाणु द्रव्यमान (u) | प्राकृतिक प्रचुरता | अर्धायु | क्षय का प्रकार | |
|---|---|---|---|---|---|
| 1 स्थिर | 1.00782503223 ± 0.00000000009 | 99.9885% ± 0.0070% | स्थिर | stable | |
| 2 स्थिर | 2.01410177812 ± 0.00000000012 | 0.0115% ± 0.0070% | स्थिर | stable |
स्पेक्ट्रमी रेखाएँ
| तरंगदैर्घ्य (nm) | तीव्रता | आयनन अवस्था | प्रकार | संक्रमण | सटीकता | स्रोत | |
|---|---|---|---|---|---|---|---|
| 383.5355892 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 9d 2D | मापित | NIST | |
| 383.5356424 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 9s 2S | मापित | NIST | |
| 383.53587 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 383.5361082 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 9p 2P* | मापित | NIST | |
| 383.5361616 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 9s 2S | मापित | NIST | |
| 383.5361673 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 9p 2P* | मापित | NIST | |
| 383.53839 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 383.53909 nm | 30000 | H I | emission | 2 → 9 | मापित | NIST | |
| 383.5409535 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 9d 2D | मापित | NIST | |
| 383.54096 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 383.5409732 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 9d 2D | मापित | NIST | |
| 383.5410263 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 9s 2S | मापित | NIST | |
| 388.9019815 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 8d 2D | मापित | NIST | |
| 388.9020595 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 8s 2S | मापित | NIST | |
| 388.90227 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 388.9024865 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 8d 2D | मापित | NIST | |
| 388.9025152 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 8p 2P* | मापित | NIST | |
| 388.9025154 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 8d 2D | मापित | NIST | |
| 388.9025933 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 8s 2S | मापित | NIST | |
| 388.9026017 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 8p 2P* | मापित | NIST | |
| 388.90486 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 388.90557 nm | 70000 | H I | emission | 2 → 8 | मापित | NIST | |
| 388.9074883 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 8d 2D | मापित | NIST | |
| 388.90749 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 388.9075172 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 8d 2D | मापित | NIST | |
| 388.9075951 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 8s 2S | मापित | NIST | |
| 397.0041763 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 7d 2D | मापित | NIST | |
| 397.0042976 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 7s 2S | मापित | NIST | |
| 397.00448 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 397.0047325 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 7p 2P* | मापित | NIST | |
| 397.0048539 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 7s 2S | मापित | NIST | |
| 397.004867 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 7p 2P* | मापित | NIST | |
| 397.00719 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 397.00788 nm | 30000 | H I | emission | 2 → 7 | मापित | NIST | |
| 397.0099002 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 7d 2D | मापित | NIST | |
| 397.00991 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 397.009945 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 7d 2D | मापित | NIST | |
| 397.0100663 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 7s 2S | मापित | NIST | |
| 410.1702284 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 6d 2D | मापित | NIST | |
| 410.1704339 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 6s 2S | मापित | NIST | |
| 410.17056 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 410.1707462 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 6d 2D | मापित | NIST | |
| 410.1708218 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 6p 2P* | मापित | NIST | |
| 410.1710277 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 6s 2S | मापित | NIST | |
| 410.1710499 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 6p 2P* | मापित | NIST | |
| 410.17346 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 410.17415 nm | 70000 | H I | emission | 2 → 6 | मापित | NIST | |
| 410.17631 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 6d 2D | मापित | NIST | |
| 410.17632 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 410.176386 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 6d 2D | मापित | NIST | |
| 410.1765915 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 6s 2S | मापित | NIST | |
| 434.0426937 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 5d 2D | मापित | NIST | |
| 434.04309 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 434.0430904 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 5s 2S | मापित | NIST | |
| 434.0433568 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 5p 2P* | मापित | NIST | |
| 434.0437554 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 5s 2S | मापित | NIST | |
| 434.0437982 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 5p 2P* | मापित | NIST | |
| 434.04634 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 434.0471 nm | 90000 | H I | emission | 2 → 5 | मापित | NIST | |
| 434.0494419 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 5d 2D | मापित | NIST | |
| 434.04947 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 434.0495889 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 5d 2D | मापित | NIST | |
| 434.0499857 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 5s 2S | मापित | NIST | |
| 486.1278624 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 4d 2D | मापित | NIST | |
| 486.1283363 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 4d 2D | मापित | NIST | |
| 486.12841 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 486.1286949 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 4p 2P* | मापित | NIST | |
| 486.128837 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 4s 2S | मापित | NIST | |
| 486.1296711 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 4s 2S | मापित | NIST | |
| 486.1297761 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 4p 2P* | मापित | NIST | |
| 486.1325 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 486.1333 nm | 180000 | H I | emission | 2 → 4 | मापित | NIST | |
| 486.1361516 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 4d 2D | मापित | NIST | |
| 486.13622 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 486.1365118 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 4d 2D | मापित | NIST | |
| 486.1374864 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 4s 2S | मापित | NIST | |
| 656.27097 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 3d 2D | मापित | NIST | |
| 656.2714 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 656.2722 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 656.272483 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 3p 2P* | मापित | NIST | |
| 656.275181 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 3s 2S | मापित | NIST | |
| 656.276701 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 3s 2S | मापित | NIST | |
| 656.277 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 656.277153 nm | उपलब्ध नहीं | H I | emission | 2s 2S → 3p 2P* | मापित | NIST | |
| 656.2795 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 656.2819 nm | 500000 | H I | emission | 2 → 3 | मापित | NIST | |
| 656.285177 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 3d 2D | मापित | NIST | |
| 656.28533 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 656.2854 nm | उपलब्ध नहीं | H I | emission | उपलब्ध नहीं | मापित | NIST | |
| 656.286734 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 3d 2D | मापित | NIST | |
| 656.290944 nm | उपलब्ध नहीं | H I | emission | 2p 2P* → 3s 2S | मापित | NIST |
विस्तृत गुण
सहसंयोजक त्रिज्याएँ (विस्तृत)
- सहसंयोजक त्रिज्या (प्यूक्को)
- 32 pm
वान डर वाल्स त्रिज्याएँ
- Bondi
- 120 pm
- Alvarez
- 120 pm
- UFF
- 288.6 pm
- MM3
- 162 pm
- Dreiding
- 319.5 pm
- Rowland–Taylor
- 110 pm
परमाणु और धात्विक त्रिज्याएँ
- परमाणु त्रिज्या (राह्म)
- 154 pm
- धात्विक त्रिज्या (C12)
- 78 pm
संख्यांकन मापक्रम
- Mendeleev
- 105
- Pettifor
- 103
- Glawe
- 103
विद्युतऋणात्मकता मापक्रम
- Ghosh
- 0
- Miedema
- 5
- Gunnarsson–Lundqvist
- 6
- Robles–Bartolotti
- 5
ध्रुवणीयता और परिक्षेपण
- द्विध्रुव ध्रुवणीयता
- 4.5071 a.u.
- द्विध्रुव ध्रुवणीयता (अनिश्चितता)
- 0 a.u.
- C₆
- 6.499 Ha·Bohr6
- C₆ (Gould–Bučko)
- 6.51 Ha·Bohr6
मीडेमा प्राचल
- मीडेमा मोलर आयतन
- 1.7 cm3/mol
- मीडेमा इलेक्ट्रॉन घनत्व
- 3
प्रावस्था संक्रमण और अपररूप
| गलनांक | 13.99 K |
| क्वथनांक | 20.27 K |
| क्रांतिक बिंदु (तापमान) | 32.94 K |
| क्रांतिक बिंदु (दाब) | 1.29 MPa |
| त्रिक बिंदु (तापमान) | 13.8 K |
| त्रिक बिंदु (दाब) | 7.04 kPa |
ऑक्सीकरण अवस्था की श्रेणियाँ
उन्नत संदर्भ डेटा
परिरक्षण स्थिरांक (1)
| n | कक्षक | σ |
|---|---|---|
| 1 | s | 0 |
क्रिस्टल त्रिज्याओं का विवरण (2)
| आवेश | CN | प्रचक्रण | rcrystal (pm) | उत्पत्ति |
|---|---|---|---|---|
| 1 | I | -24 | ||
| 1 | II | -4 |
समस्थानिक क्षय के प्रकार (6)
| समस्थानिक | मोड | तीव्रता |
|---|---|---|
| 3 | B- | 100% |
| 4 | n | 100% |
| 5 | 2n | 100% |
| 6 | n | — |
| 6 | 3n | — |
| 7 | 2n | — |
एक्स-रे प्रकीर्णन गुणक (501)
| ऊर्जा (eV) | f₁ | f₂ |
|---|---|---|
| 10 | — | 0 |
| 10.1617 | — | 0 |
| 10.3261 | — | 0 |
| 10.4931 | — | 0 |
| 10.6628 | — | 0 |
| 10.8353 | — | 0 |
| 11.0106 | — | 0 |
| 11.1886 | — | 0 |
| 11.3696 | — | 0 |
| 11.5535 | — | 0 |
अतिरिक्त डेटा
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
1.40×103 milligrams per kilogram
संदर्भ (1)
- [5] Hydrogen https://education.jlab.org/itselemental/ele001.html
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
1.08×105 milligrams per liter
संदर्भ (1)
- [5] Hydrogen https://education.jlab.org/itselemental/ele001.html
Sources
Sources of this element.
Hydrogen is estimated to make up more than 90% of all the atoms three quarters of the mass of the universe! This element is found in the stars, and plays an important part in powering the universe through both the proton-proton reaction and carbon-nitrogen cycle. Stellar hydrogen fusion processes release massive amounts of energy by combining hydrogens to form helium.
Production of hydrogen in the U.S. alone amounts to about 3 billion cubic feet per year. Hydrogen is prepared by
▸ steam on heated carbon,
▸ decomposition of certain hydrocarbons with heat,
▸ reaction of sodium or potassium hydroxide on aluminum
▸ electrolysis of water, or
▸ displacement from acids by certain metals.
Liquid hydrogen is important in cryogenics and in the study of superconductivity, as its melting point is only 20 degrees above absolute zero.
Tritium is readily produced in nuclear reactors and is used in the production of the hydrogen bomb.
Hydrogen is the primary component of Jupiter and the other gas giant planets. At some depth in the planet's interior the pressure is so great that solid molecular hydrogen is converted to solid metallic hydrogen.
In 1973, a group of Russian experimenters may have produced metallic hydrogen at a pressure of 2.8 Mbar. At the transition the density changed from 1.08 to 1.3 g/cm3. Earlier, in 1972, at Livermore, California, a group also reported on a similar experiment in which they observed a pressure-volume point centered at 2 Mbar. Predictions say that metallic hydrogen may be metastable; others have predicted it would be a superconductor at room temperature.
संदर्भ (1)
- [6] Hydrogen https://periodic.lanl.gov/1.shtml
Isotopes in Forensic Science and Anthropology
Information on the use of this element's isotopes in forensic science and anthropology.
Measurements of relative 2H abundances are used to determine the breeding grounds of many species of migrant songbirds. These species of songbirds only grow their feathers before migration, and they grow them on or close to their breeding grounds. Therefore, the isotopic composition of a bird’s feathers correlates to the isotopic composition of the growing season’s precipitation [18] Z. D. Sharp, V. Atudorei, H. O. Panarello, J. Fernández, C. Douthitt. J. Archaeolog. Sci.30, 1709 (2003)., [19] K. A. Hobson. Oecologia120, 314 (1999)., [20] K. A. Hobson, L. I. Wassenaar. Oecologia.109, 142 (1996)..
Measurements of relative 2H abundances of human hair samples collected at archeological sites are used to determine the geographic region in which a subject lived based on the hydrogen isotopic composition of the water they drank. This is possible because hair stores a daily record of the hydrogen isotopic composition of intake water, which correlates to local meteoric water [18] Z. D. Sharp, V. Atudorei, H. O. Panarello, J. Fernández, C. Douthitt. J. Archaeolog. Sci.30, 1709 (2003)., [21] T. B. Coplen, H. Qi. Forensic Sci. Int.266, 222 (2016)..
संदर्भ (5)
- [18] Z. D. Sharp, V. Atudorei, H. O. Panarello, J. Fernández, C. Douthitt. J. Archaeolog. Sci.30, 1709 (2003).
- [19] K. A. Hobson. Oecologia120, 314 (1999).
- [20] K. A. Hobson, L. I. Wassenaar. Oecologia.109, 142 (1996).
- [21] T. B. Coplen, H. Qi. Forensic Sci. Int.266, 222 (2016).
- [4] IUPAC Periodic Table of the Elements and Isotopes (IPTEI) https://doi.org/10.1515/pac-2015-0703
संदर्भ
(9)
Data deposited in or computed by PubChem
The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.
Element data are cited from the Atomic weights of the elements (an IUPAC Technical Report). The IUPAC periodic table of elements can be found at https://iupac.org/what-we-do/periodic-table-of-elements/. Additional information can be found within IUPAC publication doi:10.1515/pac-2015-0703 Copyright © 2020 International Union of Pure and Applied Chemistry.
The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.
Thomas Jefferson National Accelerator Facility (Jefferson Lab) is one of 17 national laboratories funded by the U.S. Department of Energy. The lab's primary mission is to conduct basic research of the atom's nucleus using the lab's unique particle accelerator, known as the Continuous Electron Beam Accelerator Facility (CEBAF). For more information visit https://www.jlab.org/
The periodic table at the LANL (Los Alamos National Laboratory) contains basic element information together with the history, source, properties, use, handling and more. The provenance data may be found from the link under the source name.
The periodic table contains NIST's critically-evaluated data on atomic properties of the elements. The provenance data that include data for atomic spectroscopy, X-ray and gamma ray, radiation dosimetry, nuclear physics, and condensed matter physics may be found from the link under the source name. Ref: https://www.nist.gov/pml/atomic-spectra-database
This section provides all form of data related to element Hydrogen.
The element property data was retrieved from publications.