Manganese (Mn)
transition-metalSolid
मानक परमाणु भार
54.938044 uइलेक्ट्रॉन विन्यास
[Ar] 4s2 3d5गलनांक
1245.85 °Cक्वथनांक
2060.85 °Cघनत्व
7300 kg/m³ऑक्सीकरण अवस्थाएँ
−3, −1, 0, +1, +2, +3, +4, +5, +6, +7विद्युतऋणात्मकता (पॉलिंग)
1.55आयनन ऊर्जा (प्रथम)
7.434038 eVखोज का वर्ष
1774परमाणु त्रिज्या
140 pmविवरण
Manganese is a hard, brittle first-row transition metal and an essential alloying element in steelmaking. It occurs in nature mainly as oxides, carbonates, and silicates rather than as the free metal. Its chemistry is notable for accessible oxidation states from +2 to +7, with strong colors and redox behavior. Small biological amounts are essential, especially in enzymes, but concentrated manganese compounds and dusts can be hazardous.
It is gray-white, resembling iron, but is harder and very brittle. The metal is reactive chemically and decomposes slowly in cold water. Manganese is used to form many important alloys. Manganese improves rolling and forging qualities in steel, along with adding strength, stiffness, wear resistance, hardness.
With aluminum and antimony, and especially with small amounts of copper, it forms highly ferromagnetic alloys.
Manganese metal is ferromagnetic only after special treatment. The pure metal exists in four allotropic forms. The alpha form is stable at ordinary temperature; gamma manganese, which changes to alpha at ordinary temperatures, is said to be flexible, soft, easily cut, and capable of being bent.
The name derives from the Latin magnes for "magnet" since pyrolusite (MnO2) has magnetic properties. It was discovered by the Swedish pharmacist and chemist Carl-Wilhelm Scheele in 1774. In the same year, the Swedish chemist Johan Gottlieb Gahn first isolated the metal.
Proposed to be an element by Carl Wilhelm Scheele in 1774, manganese was discovered by Johan Gottlieb Gahn, a Swedish chemist, by heating the mineral pyrolusite (MnO2) in the presence of charcoal later that year. Today, most manganese is still obtained from pyrolusite, although it is usually burned in a furnace with powdered aluminum or is treated with sulfuric acid (H2SO4) to form manganese sulfate (MnSO4), which is then electrolyzed.
From the Latin word magnes, magnet, from magnetic properties of pyrolusite. Recognized by Carl Wilhelm Scheele, Torbern Olof Bergman, and others as an element and isolated by Gahn in 1774 by reduction of the dioxide with carbon.
Pure manganese is a silvery-gray metal with a faint pinkish cast when freshly prepared. It tarnishes in air and is hard and brittle rather than malleable. Several solid allotropes are known, and the stable form at room temperature has a complex crystal structure.
Most manganese is used in iron and steel production, where it removes sulfur and oxygen and improves hardness, strength, and wear resistance. Ferromanganese and silicomanganese are standard alloy additions. Manganese is also used in some aluminum alloys and in dry-cell and alkaline batteries through manganese dioxide, MnO₂. Potassium permanganate, KMnO₄, has long been used as a strong oxidizing agent in chemical synthesis, water treatment, and analytical chemistry.
Nearly 90% of all of the manganese produced each year is used in the production of steel. Manganese is added to molten steel to remove oxygen and sulfur and is alloyed with steel to make it easier to form and work with and to increase steel's strength and resistance to impact. Railroad tracks, for example, are made with steel that contains as much as 1.2% manganese. Manganese is also used to give glass an amethyst color and is responsible for the color of amethyst gemstones.
Manganese dioxide (MnO2), the most common compound of manganese, makes up about 0.14% of the Earth's crust. It is used in dry cell batteries to prevent the formation of hydrogen, to remove the green color in glass that is caused by the presence of iron contaminants, and as a drying agent in black paints.
The dioxide (pyrolusite) is used as a depolarizer in dry cells and is used to "decolorize" glass that is colored green by impurities of iron. Manganese by itself colors glass an amethyst color and is responsible for the color of true amethyst. The dioxide is also used in the preparation of oxygen and chlorine and in drying black paints. The permanganate is a powerful oxidizing agent and is used in quantitative analysis and in medicine.
Manganese is widely distributed throughout the animal kingdom. It is an important trace element and may be essential for utilization of vitamin B1.
Isotopes in Earth/Planetary Science
Radioactive 54Mn (half-life of 312 days) has been used as a tracer to study migration of heavy metals in effluents (flowing out) from mining waste [109] Australian Government, Australian Nuclear Science and Technology Organisation (Ansto). [Radioisotopes]:/their Role in Society Today/, Australian Government, Australian Nuclear Science and Technology Organisation (Ansto) (2014), Feb. 24; http://www.ansto.gov.au/__data/assets/pdf_file/0018/3564/Radioisotopes.pdf., [110] AUS-e-TUTE for Astute Science Students. Chemistry Tutorial: Summary of Radioactive Particles, Isotopes, Properties and Uses, AUS-e-TUTE for Astute Science Students (2014), Feb. 24; http://www.ausetute.com.au/nuclesum.html..
Isotopes in Geochronology
The radioactive isotope 53Mn is formed by the interaction of protons, produced by cosmic rays, on iron in rocks. The accumulation of 53Mn, having a half-life of 3.7×106 years, at the Earth’s surface enables determination of exposure ages of landforms to cosmic rays and quantification of erosion rates. For example, Schaefer et al. [211] J. M. Schaefer, T. Faestermann, G. F. Herzog, K. Knie, G. Korschinek, J. Masarik, A. Meier, M. Poutivtsev, G. Rugel, C. Schlüchter, F. Serifiddin, G. Winckler. Earth Planet. Sci. Lett.251, 334 (2006). measured 13 samples from nine dolerite (igneous rock containing plagioclase, pyroxene, and olivine) surfaces in the Dry Valleys, Antarctica. They found that the terrestrial 53Mn concentrations correlate well with cosmic-ray-produced 3He and 21Ne concentrations in the same samples (Fig. IUPAC.25.1), which suggests that 53Mn is produced continuously in place and retained over millions of years without loss. Their results suggest that 53Mn concentrations in rocks can be used to monitor Earth-surface processes on time scales exceeding 10×106 years.
Isotopes in Medicine
51Mn, 52Mn and 52mMn (with half-lives of 46 min, 5.6 days, and 21 min, respectively) are radioactive isotopes that emit positrons that are used in positron emission tomography (PET) imaging [212] G. J. Topping, P. Schaffer, C. Hoehr, T. J. Ruth, V. Sossi. Med. Phys.40, 042502 (2013). https://doi.org/10.1118/1.4793756., [213] C. W. Olanow, P. F. Good, H. Shinotoh, K. A. Hewitt, F. Vingerhoets, B. J. Snow, M. F. Beal, D. B. Calne, D. P. Perl. Neurology46, 492 (1996).. The m in the superscript of 52mMn indicates a metastable state of the isotope.
Manganese commonly forms Mn²⁺ compounds, many of which are pale pink and relatively stable in water. Higher oxidation states are important in oxides and oxyanions: manganese dioxide, MnO₂, contains Mn(IV), while permanganate salts such as potassium permanganate, KMnO₄, contain Mn(VII) and are powerful oxidants. Manganese(II) sulfate, MnSO₄, is an important soluble salt. The carbonate rhodochrosite, MnCO₃, and mixed oxide minerals are major natural sources. Manganate, MnO₄²⁻, is green and less stable than permanganate under many conditions.
See more information at the Manganese compound page.
Metallic manganese is not highly toxic as a solid lump, but dust and fumes from mining, welding, smelting, or grinding can be harmful if inhaled. Chronic excessive exposure to manganese can damage the nervous system and produce symptoms resembling parkinsonism. Strong oxidizing compounds such as potassium permanganate, KMnO₄, can burn skin and react dangerously with reducing agents or organic materials. Normal dietary manganese is essential, but concentrated exposure is a separate hazard.
Exposure to manganese dusts, fume, and compounds should not exceed the ceiling value of 5 mg/m3 for even short periods because of the element's toxicity level.
Manganese is widespread in rocks, soils, freshwater, and marine sediments. Its mobility is controlled strongly by oxidation state, pH, and the availability of oxygen; Mn²⁺ is more soluble, while Mn(III) and Mn(IV) oxides tend to form insoluble coatings and nodules. Microorganisms can oxidize and reduce manganese and help drive its cycling. In water systems, excess dissolved manganese can stain plumbing and affect taste before it reaches levels of toxicological concern.
Manganese is produced chiefly from oxide and carbonate ores, then converted into ferromanganese, silicomanganese, electrolytic manganese metal, or manganese chemicals according to use. Steelmaking dominates demand, so consumption follows construction, transport, and machinery production more than specialty chemical markets. High-grade ore supply is geographically concentrated, and beneficiation is often needed. Recycling occurs mainly indirectly through recycled steel rather than recovery of manganese as a separate product. Battery use has grown in importance but remains distinct from the much larger metallurgical market.
Manganese minerals are widely distributed, with oxides, silicates, and carbonates being the most common. Large quantities of manganese nodules are found on the ocean floor and may become a source of manganese. These nodules contain about 24% manganese, together with many other elements in lesser abundance.
Most manganese today is obtained from ores found in Russia, Brazil, Australia, South Africa, Gabon, and India. Pyrolusite and rhodochrosite are among the most common manganese minerals. The metal is obtained by reduction of the oxide with sodium, magnesium, aluminum, or by electrolysis.
Manganese is a moderately abundant iron-peak element formed in stellar nucleosynthesis, especially in processes associated with silicon burning and supernovae. In rocky planets and meteorites it follows geochemical behavior between lithophile and siderophile tendencies, appearing in silicates, oxides, and metal-bearing phases. Its abundance is far below that of iron but high enough for broad planetary distribution.
- Manganese dioxide, MnO₂, is the main depolarizer material in many zinc-carbon and alkaline cells.
- The intense purple color of permanganate comes from Mn(VII), not from a d-electron transition.
- Manganese nodules on the deep ocean floor also contain iron, nickel, copper, and cobalt.
- Hadfield steel contains high manganese and is valued for work-hardening under impact.
- The name is historically linked to magnesia minerals, which were often confused in early mineralogy.
चित्र
गुण
भौतिक
- परमाणु त्रिज्या (आनुभविक)
- 140 pm सभी तत्वों की परमाणु त्रिज्या (आनुभविक) की तुलना करें →
- सहसंयोजक त्रिज्या
- 139 pm सभी तत्वों की सहसंयोजक त्रिज्या की तुलना करें →
- वान डर वाल्स त्रिज्या
- 197 pm सभी तत्वों की वान डर वाल्स त्रिज्या की तुलना करें →
- धात्विक त्रिज्या
- 118 pm सभी तत्वों की धात्विक त्रिज्या की तुलना करें →
- घनत्व
- 7300 kg/m³ सभी तत्वों की घनत्व की तुलना करें →
- मोलर आयतन
- 0.00739 L/mol
- STP पर प्रावस्था
- ठोस सभी तत्वों की STP पर प्रावस्था की तुलना करें →
- गलनांक
- 1245.85 °C सभी तत्वों की गलनांक की तुलना करें →
- क्वथनांक
- 2060.85 °C सभी तत्वों की क्वथनांक की तुलना करें →
- विशिष्ट ऊष्मा धारिता
- 0.479 J/(g·K) सभी तत्वों की विशिष्ट ऊष्मा धारिता की तुलना करें →
- मोलर ऊष्मा धारिता
- 26.32 J/(mol·K) सभी तत्वों की मोलर ऊष्मा धारिता की तुलना करें →
- क्रिस्टल संरचना
- घनीय सभी तत्वों की क्रिस्टल संरचना की तुलना करें →
रासायनिक
- विद्युतऋणात्मकता (पॉलिंग)
- 1.55 सभी तत्वों की विद्युतऋणात्मकता (पॉलिंग) की तुलना करें →
- विद्युतऋणात्मकता (ऐलन)
- 1.75
- इलेक्ट्रॉन बंधुता
- -0.5 eV (ऋणात्मक मान — परमाणु द्वारा अतिरिक्त इलेक्ट्रॉन बांधने की भविष्यवाणी नहीं)
- आयनन ऊर्जा (प्रथम)
- 7.434038 eV सभी तत्वों की आयनन ऊर्जा (प्रथम) की तुलना करें →
- आयनन ऊर्जा (द्वितीय)
- 15.640044 eV सभी तत्वों की आयनन ऊर्जा (द्वितीय) की तुलना करें →
- आयनन ऊर्जा (तृतीय)
- 33.668116 eV सभी तत्वों की आयनन ऊर्जा (तृतीय) की तुलना करें →
- आयनन ऊर्जा (चतुर्थ)
- 51.210176 eV सभी तत्वों की आयनन ऊर्जा (चतुर्थ) की तुलना करें →
- आयनन ऊर्जा (पंचम)
- 72.410249 eV सभी तत्वों की आयनन ऊर्जा (पंचम) की तुलना करें →
- ऑक्सीकरण अवस्थाएँ
- −3, −1, 0, +1, +2, +3, +4, +5, +6, +7 सभी तत्वों की ऑक्सीकरण अवस्थाएँ की तुलना करें →
- संयोजकता इलेक्ट्रॉन
- 7 सभी तत्वों की संयोजकता इलेक्ट्रॉन की तुलना करें →
- इलेक्ट्रॉन विन्यास
- [Ar] 4s2 3d5
ऊष्मागतिक
- क्रांतिक बिंदु (तापमान)
- 4052 °C
- गलन ऊष्मा
- 0.13680883 eV सभी तत्वों की गलन ऊष्मा की तुलना करें →
- वाष्पन ऊष्मा
- 2.331969 eV सभी तत्वों की वाष्पन ऊष्मा की तुलना करें →
- ऊर्ध्वपातन ऊष्मा
- 2.914443 eV
- परमाणुकरण ऊष्मा
- 2.914443 eV
- परमाणुकरण एन्थैल्पी
- 2.936208 eV
नाभिकीय
- प्रोटॉन
- 25 सभी तत्वों की प्रोटॉन की तुलना करें →
- न्यूट्रॉन
- 30 सभी तत्वों की न्यूट्रॉन की तुलना करें →
- ज्ञात समस्थानिक
- 31 सभी तत्वों की ज्ञात समस्थानिक की तुलना करें →
- स्थिर समस्थानिक
- 1 सभी तत्वों की स्थिर समस्थानिक की तुलना करें →
- सबसे स्थिर समस्थानिक
- Mn-55
- खोज का वर्ष
- 1774
प्रचुरता
- प्रचुरता (भूपर्पटी)
- 950 mg/kg सभी तत्वों की प्रचुरता (भूपर्पटी) की तुलना करें →
- प्रचुरता (महासागर)
- 2 × 10−4 mg/L सभी तत्वों की प्रचुरता (महासागर) की तुलना करें →
क्रिस्टल संरचना
- जालक स्थिरांक a
- 889 pm
इलेक्ट्रॉनिक संरचना
- प्रति कोश इलेक्ट्रॉन
- 2, 8, 13, 2 सभी तत्वों की प्रति कोश इलेक्ट्रॉन की तुलना करें →
पहचानकर्ता
- CAS संख्या
- 7439-96-5 सभी तत्वों की CAS संख्या की तुलना करें →
- टर्म प्रतीक
- 6S5/2
- InChI
- InChI=1S/Mn
- InChI कुंजी
- PWHULOQIROXLJO-UHFFFAOYSA-N
इलेक्ट्रॉन विन्यास मापित
Mn: 3d⁵ 4s²[Ar] 3d⁵ 4s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d⁵ 4s²परमाणु 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 |
|---|---|---|---|
| 55 स्थिर | 54.93804391 ± 0.00000048 | 100.0000% | स्थिर |
प्रावस्था / अवस्था
कारण: गलनांक (1245.85 °C) से 1220.8 °C कम
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
ऊर्ध्वपातनांक पर 1 mol के ऊर्ध्वपातन के लिए आवश्यक ऊर्जा
घनत्व
मानक परिस्थितियों में
मानक परिस्थितियों में
उन्नत
परमाणु स्पेक्ट्रम
25 में से 10 दिखाए जा रहे हैं। आयन के आवेश के अनुसार आरोही क्रम में व्यवस्थित।
उपलब्ध स्पेक्ट्रमी रेखा डेटा ?
| आयन | आवेश | कुल रेखाएँ | संक्रमण प्रायिकताएँ | स्तर पदनाम |
|---|---|---|---|---|
| Mn I | 0 | 631 | 499 | 499 |
| Mn II | +1 | 3975 | 844 | 3781 |
| Mn III | +2 | 86 | 0 | 0 |
| Mn IV | +3 | 50 | 0 | 0 |
| Mn V | +4 | 136 | 112 | 112 |
| Mn VI | +5 | 286 | 97 | 284 |
| Mn VII | +6 | 57 | 26 | 57 |
| Mn VIII | +7 | 49 | 3 | 49 |
| Mn IX | +8 | 43 | 9 | 43 |
| Mn X | +9 | 57 | 18 | 57 |
उपलब्ध ऊर्जा स्तर डेटा ?
| आयन | आवेश | स्तर |
|---|---|---|
| Mn I | 0 | 552 |
| Mn II | +1 | 533 |
| Mn III | +2 | 393 |
| Mn IV | +3 | 104 |
| Mn V | +4 | 85 |
| Mn VI | +5 | 116 |
| Mn VII | +6 | 46 |
| Mn VIII | +7 | 32 |
| Mn IX | +8 | 38 |
| Mn X | +9 | 46 |
आयनिक त्रिज्याएँ
15 में से 10 दिखाए जा रहे हैं।
| आवेश | उपसहसंयोजन | प्रचक्रण | त्रिज्या |
|---|---|---|---|
| +2 | 4 | high | 66 pm |
| +2 | 5 | high | 75 pm |
| +2 | 6 | low | 67 pm |
| +2 | 6 | high | 83 pm |
| +2 | 7 | high | 90 pm |
| +2 | 8 | उपलब्ध नहीं | 96 pm |
| +3 | 5 | उपलब्ध नहीं | 57.99999999999999 pm |
| +3 | 6 | low | 57.99999999999999 pm |
| +3 | 6 | high | 64.5 pm |
| +4 | 4 | उपलब्ध नहीं | 39 pm |
यौगिक
समस्थानिक (1)
| द्रव्यमान संख्या | परमाणु द्रव्यमान (u) | प्राकृतिक प्रचुरता | अर्धायु | क्षय का प्रकार | |
|---|---|---|---|---|---|
| 55 स्थिर | 54.93804391 ± 0.00000048 | 100.0000% | स्थिर | stable |
स्पेक्ट्रमी रेखाएँ
694 में से 50 दिखाए जा रहे हैं। डिफ़ॉल्ट रूप से केवल मापित तीव्रता वाली स्पेक्ट्रमी रेखाएँ दिखाई जाती हैं।
| तरंगदैर्घ्य (nm) | तीव्रता | आयनन अवस्था | प्रकार | संक्रमण | सटीकता | स्रोत | |
|---|---|---|---|---|---|---|---|
| 403.0753 nm | 27000 | Mn I | emission | 3d5.4s2 a 6S → 3d5.(6S).4s.4p.(3P*) z 6P* | मापित | NIST | |
| 403.3062 nm | 19000 | Mn I | emission | 3d5.4s2 a 6S → 3d5.(6S).4s.4p.(3P*) z 6P* | मापित | NIST | |
| 403.4483 nm | 11000 | Mn I | emission | 3d5.4s2 a 6S → 3d5.(6S).4s.4p.(3P*) z 6P* | मापित | NIST | |
| 404.1355 nm | 5600 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 380.6711 nm | 3200 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 382.3507 nm | 2100 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 405.5544 nm | 1900 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 401.81 nm | 1500 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 383.4362 nm | 1300 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 404.8743 nm | 1100 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 405.893 nm | 1100 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 408.2939 nm | 1100 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 408.3628 nm | 1100 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 475.4042 nm | 1000 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 8P* → 3d5.4s.(7S).5s e 8S | मापित | NIST | |
| 482.3524 nm | 1000 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 8P* → 3d5.4s.(7S).5s e 8S | मापित | NIST | |
| 478.3427 nm | 940 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 8P* → 3d5.4s.(7S).5s e 8S | मापित | NIST | |
| 445.1586 nm | 800 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4D* | मापित | NIST | |
| 476.2367 nm | 750 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4F* | मापित | NIST | |
| 406.173 nm | 730 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 6P* → 3d5.4s.(5S).5s f 6S | मापित | NIST | |
| 406.3528 nm | 730 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 407.9412 nm | 730 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 380.9592 nm | 700 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 384.1071 nm | 670 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 446.2031 nm | 510 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 6P* → 3d5.4s.(7S).4d e 6D | मापित | NIST | |
| 432.6643 nm | 500 | Mn II | emission | 3d5.(4F).4s a 5F → 3d5.(4G).4p z 5F* | मापित | NIST | |
| 434.3983 nm | 500 | Mn II | emission | 3d5.(4F).4s a 5F → 3d5.(4G).4p z 5F* | मापित | NIST | |
| 476.6418 nm | 500 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4F* | मापित | NIST | |
| 383.3861 nm | 480 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 382.3887 nm | 390 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 423.5295 nm | 370 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p y 4P* | मापित | NIST | |
| 383.9819 nm | 350 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 384.3984 nm | 350 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 441.489 nm | 350 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4D* | मापित | NIST | |
| 476.5846 nm | 300 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4F* | मापित | NIST | |
| 407.0278 nm | 290 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6D* | मापित | NIST | |
| 425.7669 nm | 290 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p y 4P* | मापित | NIST | |
| 426.5923 nm | 290 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p y 4P* | मापित | NIST | |
| 446.4682 nm | 290 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4D* | मापित | NIST | |
| 602.182 nm | 290 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 6P* → 3d5.4s.(7S).5s e 6S | मापित | NIST | |
| 428.1097 nm | 270 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p y 4P* | मापित | NIST | |
| 445.8254 nm | 270 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 6P* → 3d5.4s.(7S).4d e 6D | मापित | NIST | |
| 449.8902 nm | 240 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4D* | मापित | NIST | |
| 450.2213 nm | 240 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4D* | मापित | NIST | |
| 443.6357 nm | 210 | Mn I | emission | 3d6.(5D).4s a 4D → 3d6.(5D).4p z 4D* | मापित | NIST | |
| 445.7549 nm | 210 | Mn I | emission | 3d5.(6S).4s.4p.(3P*) z 6P* → 3d5.4s.(7S).4d e 6D | मापित | NIST | |
| 382.9718 nm | 200 | Mn I | emission | 3d6.(5D).4s a 6D → 3d6.(5D).4p z 6F* | मापित | NIST | |
| 384.4166 nm | 200 | Mn II | emission | 3d5.(2F).4s b 3F → 3d5.(4G).4p z 3G* | मापित | NIST | |
| 420.63677 nm | 200 | Mn II | emission | 3d5.(4F).4s a 5F → 3d5.(4P).4p z 5D* | मापित | NIST | |
| 429.22329 nm | 200 | Mn II | emission | 3d5.(2D).4s c 3D → 3d5.(4G).4p z 5F* | मापित | NIST | |
| 434.83962 nm | 200 | Mn II | emission | 3d5.(4F).4s a 5F → 3d5.(4G).4p z 5F* | मापित | NIST |
विस्तृत गुण
सहसंयोजक त्रिज्याएँ (विस्तृत)
- सहसंयोजक त्रिज्या (प्यूक्को)
- 119 pm
- सहसंयोजक त्रिज्या (प्यूक्को, द्विबंध)
- 105 pm
- सहसंयोजक त्रिज्या (प्यूक्को, त्रिबंध)
- 103 pm
- सहसंयोजक त्रिज्या (ब्रैग)
- 147 pm
वान डर वाल्स त्रिज्याएँ
- Batsanov
- 205 pm
- Alvarez
- 245 pm
- UFF
- 296.1 pm
- MM3
- 224 pm
परमाणु और धात्विक त्रिज्याएँ
- परमाणु त्रिज्या (राह्म)
- 242 pm
- धात्विक त्रिज्या (C12)
- 127 pm
संख्यांकन मापक्रम
- Mendeleev
- 55
- Pettifor
- 60
- Glawe
- 72
विद्युतऋणात्मकता मापक्रम
- Ghosh
- 0
- Miedema
- 4
- Gunnarsson–Lundqvist
- 5
- Robles–Bartolotti
- 3
ध्रुवणीयता और परिक्षेपण
- द्विध्रुव ध्रुवणीयता
- 68 a.u.
- द्विध्रुव ध्रुवणीयता (अनिश्चितता)
- 9 a.u.
- C₆
- 552 Ha·Bohr6
- C₆ (Gould–Bučko)
- 635 Ha·Bohr6
रासायनिक बंधुता
- प्रोटॉन बंधुता
- 797.3 kJ/mol
- गैसीय क्षारकता
- 774.4 kJ/mol
मीडेमा प्राचल
- मीडेमा मोलर आयतन
- 7.35 cm3/mol
- मीडेमा इलेक्ट्रॉन घनत्व
- 4
आपूर्ति जोखिम और अर्थशास्त्र
- उत्पादन संकेंद्रण
- 33
- सापेक्ष आपूर्ति जोखिम
- 6
- भंडार वितरण
- 24
- राजनीतिक स्थिरता (प्रमुख उत्पादक)
- 24
- राजनीतिक स्थिरता (सबसे अधिक भंडार वाला देश)
- 44
प्रावस्था संक्रमण और अपररूप
| गलनांक | 1519.15 K |
| क्वथनांक | 2334.15 K |
| क्रांतिक बिंदु (तापमान) | 4325.15 K |
ऑक्सीकरण अवस्था की श्रेणियाँ
उन्नत संदर्भ डेटा
परिरक्षण स्थिरांक (7)
| n | कक्षक | σ |
|---|---|---|
| 1 | s | 0.6043 |
| 2 | p | 3.916 |
| 2 | s | 7.2062 |
| 3 | d | 14.4718 |
| 3 | p | 12.8908 |
| 3 | s | 11.9821 |
| 4 | s | 19.7168 |
क्रिस्टल त्रिज्याओं का विवरण (15)
| आवेश | CN | प्रचक्रण | rcrystal (pm) | उत्पत्ति |
|---|---|---|---|---|
| 2 | IV | HS | 80 | |
| 2 | V | HS | 89 | calculated, |
| 2 | VI | LS | 81 | estimated, |
| 2 | VI | HS | 97 | from r^3 vs V plots, |
| 2 | VII | HS | 104 | calculated, |
| 2 | VIII | 110 | from r^3 vs V plots, | |
| 3 | V | 72 | ||
| 3 | VI | LS | 72 | from r^3 vs V plots, |
| 3 | VI | HS | 78.5 | from r^3 vs V plots, |
| 4 | IV | 53 | from r^3 vs V plots, |
समस्थानिक क्षय के प्रकार (57)
| समस्थानिक | मोड | तीव्रता |
|---|---|---|
| 43 | p | — |
| 44 | p | — |
| 45 | p | — |
| 46 | B+ | 100% |
| 46 | B+p | 57% |
| 46 | 2p | 18% |
| 46 | B+A | — |
| 47 | B+ | 100% |
| 47 | B+p | 1.7% |
| 48 | B+ | 100% |
एक्स-रे प्रकीर्णन गुणक (504)
| ऊर्जा (eV) | f₁ | f₂ |
|---|---|---|
| 10 | — | 1.8899 |
| 10.1617 | — | 1.92644 |
| 10.3261 | — | 1.96368 |
| 10.4931 | — | 2.00165 |
| 10.6628 | — | 2.04035 |
| 10.8353 | — | 2.0798 |
| 11.0106 | — | 2.12001 |
| 11.1886 | — | 2.161 |
| 11.3696 | — | 2.20278 |
| 11.5535 | — | 2.24537 |
अतिरिक्त डेटा
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
9.50×102 milligrams per kilogram
संदर्भ (1)
- [5] Manganese https://education.jlab.org/itselemental/ele025.html
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
2×10-4 milligrams per liter
संदर्भ (1)
- [5] Manganese https://education.jlab.org/itselemental/ele025.html
Sources
Sources of this element.
Manganese minerals are widely distributed, with oxides, silicates, and carbonates being the most common. Large quantities of manganese nodules are found on the ocean floor and may become a source of manganese. These nodules contain about 24% manganese, together with many other elements in lesser abundance.
Most manganese today is obtained from ores found in Russia, Brazil, Australia, South Africa, Gabon, and India. Pyrolusite and rhodochrosite are among the most common manganese minerals. The metal is obtained by reduction of the oxide with sodium, magnesium, aluminum, or by electrolysis.
संदर्भ (1)
- [6] Manganese https://periodic.lanl.gov/25.shtml
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 Manganese.
The element property data was retrieved from publications.