Hydrogen (H)
nonmetalGas
প্রমিত পারমাণবিক ওজন
1.008 u [১.০০৭৮৪, ১.০০৮১১]ইলেকট্রন বিন্যাস
1s1গলনাঙ্ক
-259.34 °Cস্ফুটনাঙ্ক
-252.87 °Cঘনত্ব
0.08988 kg/m³জারণ অবস্থা
−1, +1তড়িৎঋণাত্মকতা (পাউলিং)
2.2আয়নীকরণ শক্তি (প্রথম)
13.598435 eVআবিষ্কারের বছর
1766পারমাণবিক ব্যাসার্ধ
25 pmবিস্তারিত
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 The heavier elements were originally made from hydrogen atoms or from other elements that were originally made from hydrogen atoms.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.
ছবি
ধর্ম
ভৌত
- পারমাণবিক ব্যাসার্ধ (পরীক্ষালব্ধ)
- 25 pm সব মৌলের পারমাণবিক ব্যাসার্ধ (পরীক্ষালব্ধ) তুলনা করুন →
- সমযোজী ব্যাসার্ধ
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- 120 pm সব মৌলের ভ্যান ডার ওয়ালস ব্যাসার্ধ তুলনা করুন →
- ঘনত্ব
- 0.08988 kg/m³ সব মৌলের ঘনত্ব তুলনা করুন →
- মোলার আয়তন
- 0.0141 L/mol
- STP-তে দশা
- গ্যাস সব মৌলের STP-তে দশা তুলনা করুন →
- গলনাঙ্ক
- -259.34 °C সব মৌলের গলনাঙ্ক তুলনা করুন →
- স্ফুটনাঙ্ক
- -252.87 °C সব মৌলের স্ফুটনাঙ্ক তুলনা করুন →
- তাপ পরিবাহিতা
- 0.181 W/(m·K) সব মৌলের তাপ পরিবাহিতা তুলনা করুন →
- আপেক্ষিক তাপধারণ ক্ষমতা
- 14.304 J/(g·K) সব মৌলের আপেক্ষিক তাপধারণ ক্ষমতা তুলনা করুন →
- মোলার তাপধারণ ক্ষমতা
- 28.836 J/(mol·K) সব মৌলের মোলার তাপধারণ ক্ষমতা তুলনা করুন →
- স্ফটিক গঠন
- ষড়ভুজীয় ঘনসন্নিবিষ্ট সব মৌলের স্ফটিক গঠন তুলনা করুন →
রাসায়নিক
- তড়িৎঋণাত্মকতা (পাউলিং)
- 2.2 সব মৌলের তড়িৎঋণাত্মকতা (পাউলিং) তুলনা করুন →
- তড়িৎঋণাত্মকতা (অ্যালেন)
- 2.3
- ইলেকট্রন আসক্তি
- 0.75419 eV
- আয়নীকরণ শক্তি (প্রথম)
- 13.598435 eV সব মৌলের আয়নীকরণ শক্তি (প্রথম) তুলনা করুন →
- জারণ অবস্থা
- −1, +1 সব মৌলের জারণ অবস্থা তুলনা করুন →
- যোজ্যতা ইলেকট্রন
- 1 সব মৌলের যোজ্যতা ইলেকট্রন তুলনা করুন →
- ইলেকট্রন বিন্যাস
- 1s1
তাপগতীয়
- ত্রৈধ বিন্দু (তাপমাত্রা)
- -259.3467 °C
- ত্রৈধ বিন্দু (চাপ)
- 7041 Pa
- সংকট বিন্দু (তাপমাত্রা)
- -240.212 °C
- সংকট বিন্দু (চাপ)
- 1.2858e+6 Pa
- গলন তাপ
- 0.00121262 eV সব মৌলের গলন তাপ তুলনা করুন →
- বাষ্পীভবন তাপ
- 0.00936933 eV সব মৌলের বাষ্পীভবন তাপ তুলনা করুন →
- পরমাণুকরণ তাপ
- 2.259398 eV
- পরমাণুকরণ এনথালপি
- 2.259398 eV
নিউক্লীয়
- প্রোটন
- 1 সব মৌলের প্রোটন তুলনা করুন →
- নিউট্রন
- 0 সব মৌলের নিউট্রন তুলনা করুন →
- পরিচিত আইসোটোপ
- 7 সব মৌলের পরিচিত আইসোটোপ তুলনা করুন →
- স্থিতিশীল আইসোটোপ
- 2 সব মৌলের স্থিতিশীল আইসোটোপ তুলনা করুন →
- সবচেয়ে স্থিতিশীল আইসোটোপ
- H-1
- আবিষ্কারের বছর
- 1766
প্রাচুর্য
- প্রাচুর্য (ভূত্বক)
- 1400 mg/kg সব মৌলের প্রাচুর্য (ভূত্বক) তুলনা করুন →
- প্রাচুর্য (মহাসাগর)
- 1.08 × 105 mg/L সব মৌলের প্রাচুর্য (মহাসাগর) তুলনা করুন →
স্ফটিক গঠন
- জালক ধ্রুবক a
- 375 pm
ইলেকট্রনীয় গঠন
- প্রতি শক্তিস্তরে ইলেকট্রন
- 1 সব মৌলের প্রতি শক্তিস্তরে ইলেকট্রন তুলনা করুন →
শনাক্তকারী
- CAS নম্বর
- 1333-74-0 সব মৌলের CAS নম্বর তুলনা করুন →
- টার্ম প্রতীক
- 2S1/2
- InChI
- InChI=1S/H
- InChI Key
- YZCKVEUIGOORGS-UHFFFAOYSA-N
ইলেকট্রন বিন্যাস পরিমাপকৃত
H: 1s¹1s¹1s¹পারমাণবিক মডেল
আইসোটোপভেদে নিউট্রনের সংখ্যা, ভর ও স্থিতিশীলতা পরিবর্তিত হয় — নিরপেক্ষ পরমাণুর ইলেকট্রন বিন্যাস নয়।
পারমাণবিক মডেলের রূপরেখা, প্রকৃত অনুপাতে নয়।
পারমাণবিক স্বতন্ত্র পরিচয়চিহ্ন
নিঃসরণ / শোষণ বর্ণালি
আইসোটোপের বণ্টন
| ভরসংখ্যা | পারমাণবিক ভর (u) | প্রাকৃতিক প্রাচুর্য | অর্ধায়ু |
|---|---|---|---|
| 1 স্থিতিশীল | ১.০০৭৮২৫০৩২২৩ ± ০.০০০০০০০০০০৯ | 99.9885% | স্থিতিশীল |
| 2 স্থিতিশীল | ২.০১৪১০১৭৭৮১২ ± ০.০০০০০০০০০১২ | 0.0115% | স্থিতিশীল |
দশা / অবস্থা
কারণ: স্ফুটনাঙ্কের (-252.87 °C) চেয়ে 277.9 °C বেশি
রূপরেখামূলক, প্রকৃত অনুপাতে নয়
দশান্তর বিন্দু
দশান্তর শক্তি
গলনাঙ্কে 1 mol গলাতে প্রয়োজনীয় শক্তি
স্ফুটনাঙ্কে 1 mol বাষ্পীভূত করতে প্রয়োজনীয় শক্তি
ঘনত্ব
প্রমিত শর্তে
বর্তমান T-তে আদর্শ গ্যাস সূত্রের মাধ্যমে আনুমানিক নির্ণীত
উন্নত
পারমাণবিক বর্ণালি
সংরক্ষিত বর্ণালিরেখার তথ্য ?
| আয়ন | আধান | মোট রেখা | অবস্থান্তরের সম্ভাবনা | স্তরের নির্দেশক |
|---|---|---|---|---|
| D I আইসোটোপ | 0 | 364 | 161 | 341 |
| H I | 0 | 568 | 441 | 535 |
| T I আইসোটোপ | 0 | 11 | 11 | 11 |
সংরক্ষিত শক্তিস্তর তথ্য ?
| আয়ন | আধান | স্তর |
|---|---|---|
| D I আইসোটোপ | 0 | 78 |
| H I | 0 | 106 |
| T I আইসোটোপ | 0 | 10 |
যৌগ
আইসোটোপ (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.
| ভরসংখ্যা | পারমাণবিক ভর (u) | প্রাকৃতিক প্রাচুর্য | অর্ধায়ু | ক্ষয়প্রণালি | |
|---|---|---|---|---|---|
| 1 স্থিতিশীল | ১.০০৭৮২৫০৩২২৩ ± ০.০০০০০০০০০০৯ | 99.9885% ± 0.0070% | স্থিতিশীল | stable | |
| 2 স্থিতিশীল | ২.০১৪১০১৭৭৮১২ ± ০.০০০০০০০০০১২ | 0.0115% ± 0.0070% | স্থিতিশীল | stable |
বর্ণালিরেখা
| তরঙ্গদৈর্ঘ্য (nm) | তীব্রতা | আয়নীকরণ পর্যায় | ধরন | অবস্থান্তর | নির্ভুলতা | উৎস | |
|---|---|---|---|---|---|---|---|
| 383.5355892 nm | তথ্য নেই | H I | emission | 2p 2P* → 9d 2D | পরিমাপকৃত | NIST | |
| 383.5356424 nm | তথ্য নেই | H I | emission | 2p 2P* → 9s 2S | পরিমাপকৃত | NIST | |
| 383.53587 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 383.5361082 nm | তথ্য নেই | H I | emission | 2s 2S → 9p 2P* | পরিমাপকৃত | NIST | |
| 383.5361616 nm | তথ্য নেই | H I | emission | 2s 2S → 9s 2S | পরিমাপকৃত | NIST | |
| 383.5361673 nm | তথ্য নেই | H I | emission | 2s 2S → 9p 2P* | পরিমাপকৃত | NIST | |
| 383.53839 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 383.53909 nm | 30000 | H I | emission | 2 → 9 | পরিমাপকৃত | NIST | |
| 383.5409535 nm | তথ্য নেই | H I | emission | 2p 2P* → 9d 2D | পরিমাপকৃত | NIST | |
| 383.54096 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 383.5409732 nm | তথ্য নেই | H I | emission | 2p 2P* → 9d 2D | পরিমাপকৃত | NIST | |
| 383.5410263 nm | তথ্য নেই | H I | emission | 2p 2P* → 9s 2S | পরিমাপকৃত | NIST | |
| 388.9019815 nm | তথ্য নেই | H I | emission | 2p 2P* → 8d 2D | পরিমাপকৃত | NIST | |
| 388.9020595 nm | তথ্য নেই | H I | emission | 2p 2P* → 8s 2S | পরিমাপকৃত | NIST | |
| 388.90227 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 388.9024865 nm | তথ্য নেই | H I | emission | 2s 2S → 8d 2D | পরিমাপকৃত | NIST | |
| 388.9025152 nm | তথ্য নেই | H I | emission | 2s 2S → 8p 2P* | পরিমাপকৃত | NIST | |
| 388.9025154 nm | তথ্য নেই | H I | emission | 2s 2S → 8d 2D | পরিমাপকৃত | NIST | |
| 388.9025933 nm | তথ্য নেই | H I | emission | 2s 2S → 8s 2S | পরিমাপকৃত | NIST | |
| 388.9026017 nm | তথ্য নেই | H I | emission | 2s 2S → 8p 2P* | পরিমাপকৃত | NIST | |
| 388.90486 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 388.90557 nm | 70000 | H I | emission | 2 → 8 | পরিমাপকৃত | NIST | |
| 388.9074883 nm | তথ্য নেই | H I | emission | 2p 2P* → 8d 2D | পরিমাপকৃত | NIST | |
| 388.90749 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 388.9075172 nm | তথ্য নেই | H I | emission | 2p 2P* → 8d 2D | পরিমাপকৃত | NIST | |
| 388.9075951 nm | তথ্য নেই | H I | emission | 2p 2P* → 8s 2S | পরিমাপকৃত | NIST | |
| 397.0041763 nm | তথ্য নেই | H I | emission | 2p 2P* → 7d 2D | পরিমাপকৃত | NIST | |
| 397.0042976 nm | তথ্য নেই | H I | emission | 2p 2P* → 7s 2S | পরিমাপকৃত | NIST | |
| 397.00448 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 397.0047325 nm | তথ্য নেই | H I | emission | 2s 2S → 7p 2P* | পরিমাপকৃত | NIST | |
| 397.0048539 nm | তথ্য নেই | H I | emission | 2s 2S → 7s 2S | পরিমাপকৃত | NIST | |
| 397.004867 nm | তথ্য নেই | H I | emission | 2s 2S → 7p 2P* | পরিমাপকৃত | NIST | |
| 397.00719 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 397.00788 nm | 30000 | H I | emission | 2 → 7 | পরিমাপকৃত | NIST | |
| 397.0099002 nm | তথ্য নেই | H I | emission | 2p 2P* → 7d 2D | পরিমাপকৃত | NIST | |
| 397.00991 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 397.009945 nm | তথ্য নেই | H I | emission | 2p 2P* → 7d 2D | পরিমাপকৃত | NIST | |
| 397.0100663 nm | তথ্য নেই | H I | emission | 2p 2P* → 7s 2S | পরিমাপকৃত | NIST | |
| 410.1702284 nm | তথ্য নেই | H I | emission | 2p 2P* → 6d 2D | পরিমাপকৃত | NIST | |
| 410.1704339 nm | তথ্য নেই | H I | emission | 2p 2P* → 6s 2S | পরিমাপকৃত | NIST | |
| 410.17056 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 410.1707462 nm | তথ্য নেই | H I | emission | 2s 2S → 6d 2D | পরিমাপকৃত | NIST | |
| 410.1708218 nm | তথ্য নেই | H I | emission | 2s 2S → 6p 2P* | পরিমাপকৃত | NIST | |
| 410.1710277 nm | তথ্য নেই | H I | emission | 2s 2S → 6s 2S | পরিমাপকৃত | NIST | |
| 410.1710499 nm | তথ্য নেই | H I | emission | 2s 2S → 6p 2P* | পরিমাপকৃত | NIST | |
| 410.17346 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 410.17415 nm | 70000 | H I | emission | 2 → 6 | পরিমাপকৃত | NIST | |
| 410.17631 nm | তথ্য নেই | H I | emission | 2p 2P* → 6d 2D | পরিমাপকৃত | NIST | |
| 410.17632 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 410.176386 nm | তথ্য নেই | H I | emission | 2p 2P* → 6d 2D | পরিমাপকৃত | NIST | |
| 410.1765915 nm | তথ্য নেই | H I | emission | 2p 2P* → 6s 2S | পরিমাপকৃত | NIST | |
| 434.0426937 nm | তথ্য নেই | H I | emission | 2p 2P* → 5d 2D | পরিমাপকৃত | NIST | |
| 434.04309 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 434.0430904 nm | তথ্য নেই | H I | emission | 2p 2P* → 5s 2S | পরিমাপকৃত | NIST | |
| 434.0433568 nm | তথ্য নেই | H I | emission | 2s 2S → 5p 2P* | পরিমাপকৃত | NIST | |
| 434.0437554 nm | তথ্য নেই | H I | emission | 2s 2S → 5s 2S | পরিমাপকৃত | NIST | |
| 434.0437982 nm | তথ্য নেই | H I | emission | 2s 2S → 5p 2P* | পরিমাপকৃত | NIST | |
| 434.04634 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 434.0471 nm | 90000 | H I | emission | 2 → 5 | পরিমাপকৃত | NIST | |
| 434.0494419 nm | তথ্য নেই | H I | emission | 2p 2P* → 5d 2D | পরিমাপকৃত | NIST | |
| 434.04947 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 434.0495889 nm | তথ্য নেই | H I | emission | 2p 2P* → 5d 2D | পরিমাপকৃত | NIST | |
| 434.0499857 nm | তথ্য নেই | H I | emission | 2p 2P* → 5s 2S | পরিমাপকৃত | NIST | |
| 486.1278624 nm | তথ্য নেই | H I | emission | 2p 2P* → 4d 2D | পরিমাপকৃত | NIST | |
| 486.1283363 nm | তথ্য নেই | H I | emission | 2s 2S → 4d 2D | পরিমাপকৃত | NIST | |
| 486.12841 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 486.1286949 nm | তথ্য নেই | H I | emission | 2s 2S → 4p 2P* | পরিমাপকৃত | NIST | |
| 486.128837 nm | তথ্য নেই | H I | emission | 2p 2P* → 4s 2S | পরিমাপকৃত | NIST | |
| 486.1296711 nm | তথ্য নেই | H I | emission | 2s 2S → 4s 2S | পরিমাপকৃত | NIST | |
| 486.1297761 nm | তথ্য নেই | H I | emission | 2s 2S → 4p 2P* | পরিমাপকৃত | NIST | |
| 486.1325 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 486.1333 nm | 180000 | H I | emission | 2 → 4 | পরিমাপকৃত | NIST | |
| 486.1361516 nm | তথ্য নেই | H I | emission | 2p 2P* → 4d 2D | পরিমাপকৃত | NIST | |
| 486.13622 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 486.1365118 nm | তথ্য নেই | H I | emission | 2p 2P* → 4d 2D | পরিমাপকৃত | NIST | |
| 486.1374864 nm | তথ্য নেই | H I | emission | 2p 2P* → 4s 2S | পরিমাপকৃত | NIST | |
| 656.27097 nm | তথ্য নেই | H I | emission | 2p 2P* → 3d 2D | পরিমাপকৃত | NIST | |
| 656.2714 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 656.2722 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 656.272483 nm | তথ্য নেই | H I | emission | 2s 2S → 3p 2P* | পরিমাপকৃত | NIST | |
| 656.275181 nm | তথ্য নেই | H I | emission | 2p 2P* → 3s 2S | পরিমাপকৃত | NIST | |
| 656.276701 nm | তথ্য নেই | H I | emission | 2s 2S → 3s 2S | পরিমাপকৃত | NIST | |
| 656.277 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 656.277153 nm | তথ্য নেই | H I | emission | 2s 2S → 3p 2P* | পরিমাপকৃত | NIST | |
| 656.2795 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 656.2819 nm | 500000 | H I | emission | 2 → 3 | পরিমাপকৃত | NIST | |
| 656.285177 nm | তথ্য নেই | H I | emission | 2p 2P* → 3d 2D | পরিমাপকৃত | NIST | |
| 656.28533 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 656.2854 nm | তথ্য নেই | H I | emission | তথ্য নেই | পরিমাপকৃত | NIST | |
| 656.286734 nm | তথ্য নেই | H I | emission | 2p 2P* → 3d 2D | পরিমাপকৃত | NIST | |
| 656.290944 nm | তথ্য নেই | H I | emission | 2p 2P* → 3s 2S | পরিমাপকৃত | NIST |
বিস্তৃত ধর্ম
সমযোজী ব্যাসার্ধ (বিস্তৃত)
- সমযোজী ব্যাসার্ধ (পিউক্কো)
- 32 pm
ভ্যান ডার ওয়ালস ব্যাসার্ধ
- Bondi
- 120 pm
- Alvarez
- 120 pm
- UFF
- 288.6 pm
- MM3
- 162 pm
- Dreiding
- 319.5 pm
- Rowland–Taylor
- 110 pm
পারমাণবিক ও ধাতব ব্যাসার্ধ
- পারমাণবিক ব্যাসার্ধ (রাম)
- 154 pm
- ধাতব ব্যাসার্ধ (C12)
- 78 pm
সংখ্যায়ন স্কেল
- Mendeleev
- 105
- Pettifor
- 103
- Glawe
- 103
তড়িৎঋণাত্মকতার স্কেল
- Ghosh
- 0
- Miedema
- 5
- Gunnarsson–Lundqvist
- 6
- Robles–Bartolotti
- 5
মেরুকরণযোগ্যতা ও বিচ্ছুরণ
- দ্বিমেরু মেরুকরণযোগ্যতা
- 4.5071 a.u.
- দ্বিমেরু মেরুকরণযোগ্যতা (অনিশ্চয়তা)
- 0 a.u.
- C₆
- 6.499 Ha·Bohr6
- C₆ (Gould–Bučko)
- 6.51 Ha·Bohr6
মিডেমা পরামিতি
- মিডেমা মোলার আয়তন
- 1.7 cm3/mol
- মিডেমা ইলেকট্রন ঘনত্ব
- 3
দশান্তর ও রূপভেদ
| গলনাঙ্ক | 13.99 K |
| স্ফুটনাঙ্ক | 20.27 K |
| সংকট বিন্দু (তাপমাত্রা) | 32.94 K |
| সংকট বিন্দু (চাপ) | 1.29 MPa |
| ত্রৈধ বিন্দু (তাপমাত্রা) | 13.8 K |
| ত্রৈধ বিন্দু (চাপ) | 7.04 kPa |
জারণ অবস্থার শ্রেণি
উন্নত তথ্যসূত্রের উপাত্ত
আচ্ছাদন ধ্রুবক (1)
| n | অরবিটাল | σ |
|---|---|---|
| 1 | s | 0 |
স্ফটিক ব্যাসার্ধের বিস্তারিত (2)
| আধান | CN | স্পিন | rcrystal (pm) | উৎস |
|---|---|---|---|---|
| 1 | I | -24 | ||
| 1 | II | -4 |
আইসোটোপের ক্ষয়প্রণালি (6)
| আইসোটোপ | মোড | তীব্রতা |
|---|---|---|
| 3 | B- | 100% |
| 4 | n | 100% |
| 5 | 2n | 100% |
| 6 | n | — |
| 6 | 3n | — |
| 7 | 2n | — |
এক্স-রে বিক্ষেপণ গুণক (501)
| শক্তি (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 |
অতিরিক্ত তথ্য
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
1.40×103 milligrams per kilogram
তথ্যসূত্র (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
তথ্যসূত্র (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.
তথ্যসূত্র (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)..
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- [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
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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.
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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.