Palladium (Pd)
transition-metalSolid
प्रमाणित अणुभार
106.42 uइलेक्ट्रॉन संरूपण
[Kr] 4d10द्रवणांक
1554.9 °Cउत्कलनांक
2962.85 °Cघनता
1.2e+4 kg/m³ऑक्सिडीकरण अवस्था
+1, +2, +3, +4, +5विद्युतऋणता (पॉलिंग)
2.2आयनीकरण ऊर्जा (पहिली)
8.336839 eVशोधाचे वर्ष
1803अणुत्रिज्या
140 pmतपशील
Palladium is a silvery platinum-group metal with high catalytic activity and an unusual ability to absorb large amounts of hydrogen into its lattice. It is chemically noble in air at ordinary temperatures, but it forms many complexes and is readily used in surface chemistry. Its technological importance is dominated by vehicle emission control, fine-chemical catalysis, electronics, and hydrogen-related applications.
The element is a silvery-white metal, it does not tarnish in air, and it is the least dense and lowest melting of the platinum group of metals. When annealed, it is soft and ductile; cold-working greatly increases its strength and hardness. Palladium is attacked by nitric and sulfuric acid.
At room temperatures, the metal has the unusual property of absorbing up to 900 times its own volume of hydrogen, possibly forming Pd2H. It is not yet clear if this is a true compound. Hydrogen readily diffuses through heated palladium, providing a means of purifying the gas.
The name derives from the second largest asteroid of the solar system Pallas (named after the goddess of wisdom and arts—Pallas Athene). The element was discovered by the English chemist and physicist William Hyde Wollaston in 1803, one year after the discovery of Pallas by the German astronomer Wilhelm Olbers in 1802. The discovery was originally published anonymously by Wollaston to obtain priority, while not disclosing any details about his preparation.
Palladium was discovered by William Hyde Wollaston, an English chemist, in 1803 while analyzing samples of platinum ore that were obtained from South America. Although it is a rare element, palladium tends to occur along with deposits of platinum, nickel, copper, silver and gold and is recovered as a byproduct of mining these other metals.
Palladium was named after the asteroid Pallas, which was discovered at about the same time. Pallas was the Greek goddess of wisdom.
Pure palladium is a lustrous, silver-white metal. It is soft and ductile when annealed, can be rolled into thin foil, and does not tarnish rapidly in clean air. Finely divided palladium is gray to black and has much higher surface reactivity than the compact metal.
The largest use of palladium is in catalytic converters, especially for oxidation of carbon monoxide and hydrocarbons and reduction reactions in exhaust systems. Palladium catalysts are also central to hydrogenation and carbon–carbon coupling reactions in chemical manufacture. The metal is used in multilayer ceramic capacitors, electrical contacts, dental alloys, some jewelry alloys, hydrogen purification membranes, and laboratory catalysts such as palladium on carbon.
Palladium is used to make springs for watches, surgical instruments, electrical contacts and dental fillings and crowns. Finely divided palladium acts as a catalyst and is used in hydrogenation and dehydrogenation processes. Palladium at room temperature can absorb up to 900 times its own volume of hydrogen. Hydrogen will easily pass through heated palladium, a property that allows for the easy purification of hydrogen. Palladium alloys are used to make jewelry and, when alloyed with gold, forms a material known as white gold.
Palladium dichloride (PdCl2), a palladium compound, can absorb large amounts of carbon monoxide (CO) gas and is used in carbon monoxide detectors.
Finely divided palladium is a good catalyst and is used for hydrogenation and dehydrogenation reactions. It is alloyed and used in jewelry trades.
White gold is an alloy of gold decolorized by the addition of palladium. Like gold, palladium can be beaten into leaf as thin as 1/250,000 in. The metal is used in dentistry, watch making, and in making surgical instruments and electrical contacts.
Isotopes in Earth/Planetary Science
Small palladium nucleosynthetic anomalies in isotopic composition (related to s-process variability) were identified in type IVB iron meteorites [340] B. Mayer, N. Wittig, M. Humayun, I. Leya. Astrophys. J.809, 180 (2015).. These nucleosynthetic isotope anomalies may represent spatial and/or temporal heterogeneity in the early solar nebula or may be due to chemical processing within the solar nebula [327] N. Dauphas, A. M. Davis, B. Marty, L. Reisberg. Earth Planet. Sci. Lett.226, 465 (2004)., [341] A. Trinquier, T. Elliott, D. Ulfbeck, C. Coath, A. N. Krot, M. Bizzarro. Science324, 374 (2009).. Palladium and molybdenum isotopic compositions on selected iron meteorites are correlated (Fig. IUPAC.46.1). One possible conclusion is that “a common presolar carrier must have been thermally processed on which the more volatile (a measure of the tendency of a substance to vaporize) Pd was lost and homogenized in the solar nebula, resulting in the deviation from the s-process” variability [342] B. Mayer, K. R. Bermingham, E. A. Worsham, M. Humayun, R. J. Walker. “Correlated nucleosynthetic anomalies in Mo, Ru, and Pd from iron meteorites”, in 47th Lunar and Planetary Science Conference.. Because these palladium (and other element) anomalies are persistent throughout the measured iron meteorites, the thermal processing must have occurred prior to the formation of the parent body that produced iron meteorites [342] B. Mayer, K. R. Bermingham, E. A. Worsham, M. Humayun, R. J. Walker. “Correlated nucleosynthetic anomalies in Mo, Ru, and Pd from iron meteorites”, in 47th Lunar and Planetary Science Conference..
Isotopes in Geochronology
The isotope-amount ratio n(107Pd)/n(107Ag) is used in geochronology to help date major thermal events in the Solar System. Although 107Ag is naturally occurring, 107Ag is also the daughter product of the beta decay of 107Pd. If both excess 107Ag and 107Pd (with a half-life of 6.5×106 years) are present in a sample of extraterrestrial origin, then the material would have formed sometime after 107Pd decayed. The n(107Pd)/n(107Ag) amount ratio can be measured to help determine when the 107Pd decay process began and how much time has elapsed since the material was formed [344] W. R. Kelly, G. J. Wasserburg. Geophys. Res. Lett.5 1079 (1978)., [345] G. J. Wasserburg, D. A. Papanastassiou. Some Short-Lived Nuclides in the Early Solar-System – A Connection with the Placental ISM, in Essays in Nuclear Astrophysics, C. A. Barnes, D. D. Clayton, and D. N. Schramm. Cambridge University Press, Cambridge, UK (1982)., [346] J. H. Chen, G. J. Wasserburg. Live 107Pd in the Early Solar System and Implications on Planetary Evolution, in Earth Processes: Reading the Isotopic Code, Geophysical Monograph 95, A. Basu and S. Hart. Amer. Geophys. U., Washington (1996)., [347] J. H. Chen, G. J. Wasserburg. Geochim. Cosmochim. Acta54, 1729 (1990)., [348] A. P. Dicken. Radiogenic Isotope Geology, Cambridge University Press, New York (1995)..
Isotopes in Medicine
Seeds of the radioactive isotope 103Pd are internally placed in the body to fight prostate and other cancers locally. 103Pd has a half-life of 16.99 days and releases energy at about 80 X-rays and 186 Auger electrons per 100 decays of 103Pd. Therefore, this makes this isotope an ideal candidate for internal radiotherapy for the treatment of cancers [349] M. Hussain, S. Sudar, M. N. Aslam, H. A. Shah, R. Ahmad, A. A. Malik, S. M. Qaim. Appl. Radiat. Isot.67, 1842 (2009)..
The radioisotope 109Pd (with a half-life of 13.5 h) can be used as a form of cancer therapy. For example, 109Pd-labeled porphyrins or porphyrin-like substances are used as diagnostic and therapeutic techniques to help locate and address areas of tumorous growth. Porphyrins accumulate in tumors of the body and when radiolabeled porphyrins are introduced to the body, the X-rays and energy released can help determine the location and even treat the cancerous tumors [350] T. Das, S. Chakraborty, H. D. Sarma, S. Banerjee. Radiochim. Acta96, 427 (2008)..
Isotopes Used as a Source of Radioactive Isotope(s)
104Pd is the major target used for cyclotron production of the medically important radioactive isotope 103Pd via the reaction 104Pd (p, p n) 103Pd [349] M. Hussain, S. Sudar, M. N. Aslam, H. A. Shah, R. Ahmad, A. A. Malik, S. M. Qaim. Appl. Radiat. Isot.67, 1842 (2009)..
Palladium most often shows oxidation states +2 and 0, with +4 important in some fluorides and complex salts. Palladium(II) chloride, PdCl₂, is a common starting material for coordination compounds and catalysts. Tetrakis(triphenylphosphine)palladium(0), Pd[P(C₆H₅)₃]₄, is a widely used homogeneous catalyst precursor. Palladium(II) acetate, Pd(CH₃COO)₂, and palladium on carbon are frequent sources of active palladium species in organic synthesis.
See more information at the Palladium compound page.
Compact palladium metal is not highly reactive and presents low acute toxicity, but dusts and finely divided catalysts can be irritating and may ignite adsorbed hydrogen or organic material under unfavorable conditions. Soluble palladium salts and organopalladium compounds can cause skin sensitization and other toxic effects. Spent catalysts may contain hazardous residues from the processes in which they were used.
Palladium occurs naturally at low concentrations, mainly with other platinum-group elements in sulfide and chromite-associated ores. Environmental releases are increased by abrasion and loss from automotive catalysts, creating fine particles in road dust and nearby soils. Palladium is generally sparingly soluble in many natural waters, but complexing ligands such as chloride and organic matter can increase mobility.
Palladium is obtained chiefly as a by-product of nickel, copper, and platinum-group metal mining and refining, so supply cannot respond as independently as demand for a primary metal. Major demand comes from emission-control catalysts, with electronics, chemical catalysts, dentistry, and jewelry making smaller contributions. Recycling from spent automotive catalysts is an important secondary source. Substitution with platinum or rhodium is possible in some catalyst systems but depends on performance, regulation, and relative availability.
Discovered in 1803 by Wollaston, Palladium is found with platinum and other metals of the platinum group in placer deposits of Russia, South America, North America, Ethiopia, and Australia. It is also found associated with the nickel-copper deposits of South Africa and Ontario. Palladium's separation from the platinum metals depends upon the type of ore in which it is found.
Palladium is a heavy element produced mainly by neutron-capture processes in earlier generations of stars. It is much less abundant cosmically than iron or nickel but is present in meteorites and planetary materials with other siderophile and chalcophile elements. On Earth it was partly concentrated into the core during differentiation, leaving crustal concentrations low.
- Palladium can absorb hydrogen to form non-stoichiometric palladium hydride without becoming a simple fixed-ratio salt.
- The element was named after the asteroid Pallas, which had been discovered shortly before palladium.
- Palladium-gold alloys are used to make white gold in some jewelry.
- Carbon monoxide binds strongly to palladium surfaces, a key feature of exhaust catalysis.
- Palladium leaf can be made, but it is less familiar than gold leaf because the metal is far rarer and costlier.
प्रतिमा
गुणधर्म
भौतिक
- अणुत्रिज्या (अनुभवाधारित)
- 140 pm सर्व घटकांच्या अणुत्रिज्या (अनुभवाधारित) ची तुलना करा →
- सहसंयुजी त्रिज्या
- 139 pm सर्व घटकांच्या सहसंयुजी त्रिज्या ची तुलना करा →
- व्हॅन डर वाल्स त्रिज्या
- 202 pm सर्व घटकांच्या व्हॅन डर वाल्स त्रिज्या ची तुलना करा →
- धात्विक त्रिज्या
- 128 pm सर्व घटकांच्या धात्विक त्रिज्या ची तुलना करा →
- घनता
- 1.2 × 104 kg/m³ सर्व घटकांच्या घनता ची तुलना करा →
- मोलर आयतन
- 0.0089 L/mol
- STP येथे अवस्था
- घन सर्व घटकांच्या STP येथे अवस्था ची तुलना करा →
- द्रवणांक
- 1554.9 °C सर्व घटकांच्या द्रवणांक ची तुलना करा →
- उत्कलनांक
- 2962.85 °C सर्व घटकांच्या उत्कलनांक ची तुलना करा →
- उष्णता चालकता
- 71.8 W/(m·K) सर्व घटकांच्या उष्णता चालकता ची तुलना करा →
- विशिष्ट उष्माधारकता
- 0.246 J/(g·K) सर्व घटकांच्या विशिष्ट उष्माधारकता ची तुलना करा →
- मोलर उष्माधारकता
- 25.98 J/(mol·K) सर्व घटकांच्या मोलर उष्माधारकता ची तुलना करा →
- स्फटिक संरचना
- पृष्ठकेंद्रित घनीय सर्व घटकांच्या स्फटिक संरचना ची तुलना करा →
रासायनिक
- विद्युतऋणता (पॉलिंग)
- 2.2 सर्व घटकांच्या विद्युतऋणता (पॉलिंग) ची तुलना करा →
- विद्युतऋणता (ॲलन)
- 1.58
- इलेक्ट्रॉन आसक्ती
- 0.557 eV
- आयनीकरण ऊर्जा (पहिली)
- 8.336839 eV सर्व घटकांच्या आयनीकरण ऊर्जा (पहिली) ची तुलना करा →
- आयनीकरण ऊर्जा (दुसरी)
- 19.430067 eV सर्व घटकांच्या आयनीकरण ऊर्जा (दुसरी) ची तुलना करा →
- आयनीकरण ऊर्जा (तिसरी)
- 32.930113 eV सर्व घटकांच्या आयनीकरण ऊर्जा (तिसरी) ची तुलना करा →
- आयनीकरण ऊर्जा (चौथी)
- 46.000158 eV सर्व घटकांच्या आयनीकरण ऊर्जा (चौथी) ची तुलना करा →
- आयनीकरण ऊर्जा (पाचवी)
- 61.00021 eV सर्व घटकांच्या आयनीकरण ऊर्जा (पाचवी) ची तुलना करा →
- ऑक्सिडीकरण अवस्था
- +1, +2, +3, +4, +5 सर्व घटकांच्या ऑक्सिडीकरण अवस्था ची तुलना करा →
- संयुजा इलेक्ट्रॉन
- 10 सर्व घटकांच्या संयुजा इलेक्ट्रॉन ची तुलना करा →
- इलेक्ट्रॉन संरूपण
- [Kr] 4d10
उष्मागतिक
- द्रवण उष्मा
- 0.17349847 eV सर्व घटकांच्या द्रवण उष्मा ची तुलना करा →
- बाष्पीभवन उष्मा
- 3.700057 eV सर्व घटकांच्या बाष्पीभवन उष्मा ची तुलना करा →
- संप्लवन उष्मा
- 3.907343 eV
- अणूकरण उष्मा
- 3.907343 eV
- अणूकरण एन्थाल्पी
- 3.903197 eV
केंद्रकीय
- प्रोटॉन
- 46 सर्व घटकांच्या प्रोटॉन ची तुलना करा →
- न्यूट्रॉन
- 60 सर्व घटकांच्या न्यूट्रॉन ची तुलना करा →
- ज्ञात समस्थानिके
- 42 सर्व घटकांच्या ज्ञात समस्थानिके ची तुलना करा →
- स्थिर समस्थानिके
- 4 सर्व घटकांच्या स्थिर समस्थानिके ची तुलना करा →
- सर्वाधिक स्थिर समस्थानिक
- Pd-106
- शोधाचे वर्ष
- 1803
विपुलता
- विपुलता (पृथ्वीचे कवच)
- 0.015 mg/kg सर्व घटकांच्या विपुलता (पृथ्वीचे कवच) ची तुलना करा →
स्फटिक संरचना
- जालक स्थिरांक a
- 389 pm
इलेक्ट्रॉन संरचना
- प्रत्येक कवचातील इलेक्ट्रॉन
- 2, 8, 18, 18 सर्व घटकांच्या प्रत्येक कवचातील इलेक्ट्रॉन ची तुलना करा →
ओळखचिन्हे
- CAS क्रमांक
- 7440-05-3 सर्व घटकांच्या CAS क्रमांक ची तुलना करा →
- टर्म चिन्ह
- 1S0
- InChI
- InChI=1S/Pd
- InChI की
- KDLHZDBZIXYQEI-UHFFFAOYSA-N
इलेक्ट्रॉन संरूपण मोजलेले
Pd: 4d¹⁰[Kr] 4d¹⁰1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰अणुप्रतिमान
समस्थानिकांमुळे न्यूट्रॉन संख्या, वस्तुमान आणि स्थैर्य बदलते — विद्युतदृष्ट्या उदासीन अणूचे इलेक्ट्रॉन संरूपण बदलत नाही.
योजनात्मक अणुप्रतिमान, प्रमाणानुसार नाही.
अणूची विशिष्ट ओळख
उत्सर्जन / शोषण वर्णपट
समस्थानिक वितरण
| वस्तुमानांक | अणुवस्तुमान (u) | नैसर्गिक विपुलता | अर्धायुष्य |
|---|---|---|---|
| 104 स्थिर | १०३.९०४०३०५ ± ०.०००००१४ | 11.1400% | स्थिर |
| 105 स्थिर | १०४.९०५०७९६ ± ०.०००००१२ | 22.3300% | स्थिर |
| 106 स्थिर | १०५.९०३४८०४ ± ०.०००००१२ | 27.3300% | स्थिर |
| 108 स्थिर | १०७.९०३८९१६ ± ०.०००००१२ | 26.4600% | स्थिर |
अवस्था / स्थिती
कारण: द्रवणांकापेक्षा (1554.9 °C) 1529.9 °C कमी
योजनात्मक, प्रमाणानुसार नाही
अवस्थांतर बिंदू
अवस्थांतर ऊर्जा
द्रवणांकावर 1 mol वितळवण्यासाठी आवश्यक ऊर्जा
उत्कलनांकावर 1 mol चे बाष्पीभवन करण्यासाठी आवश्यक ऊर्जा
संप्लवनांकावर 1 mol चे संप्लवन करण्यासाठी आवश्यक ऊर्जा
घनता
प्रमाणित परिस्थितीत
प्रमाणित परिस्थितीत
अणुवर्णपट
46 पैकी 10 दाखवले आहेत. आयनाच्या विद्युतभारानुसार चढत्या क्रमाने मांडलेले.
वर्णरेषांचा संग्रह ?
| आयन | विद्युतभार | एकूण वर्णरेषा | संक्रमण संभाव्यता | पातळ्यांची नामांकने |
|---|---|---|---|---|
| Pd I | 0 | 76 | 8 | 75 |
| Pd II | +1 | 62 | 10 | 62 |
| Pd III | +2 | 75 | 0 | 0 |
ऊर्जा पातळ्यांचा संग्रह ?
| आयन | विद्युतभार | पातळ्या |
|---|---|---|
| Pd I | 0 | 145 |
| Pd II | +1 | 186 |
| Pd III | +2 | 177 |
| Pd IV | +3 | 2 |
| Pd V | +4 | 2 |
| Pd VI | +5 | 2 |
| Pd VII | +6 | 2 |
| Pd VIII | +7 | 2 |
| Pd IX | +8 | 2 |
| Pd X | +9 | 2 |
आयनिक त्रिज्या
| विद्युतभार | समन्वय | प्रचक्रण | त्रिज्या |
|---|---|---|---|
| +1 | 2 | उपलब्ध नाही | 59 pm |
| +2 | 4 | उपलब्ध नाही | 64 pm |
| +2 | 6 | उपलब्ध नाही | 86 pm |
| +3 | 6 | उपलब्ध नाही | 76 pm |
| +4 | 6 | उपलब्ध नाही | 61.5 pm |
संयुगे
समस्थानिके (4)
| वस्तुमानांक | अणुवस्तुमान (u) | नैसर्गिक विपुलता | अर्धायुष्य | क्षय प्रकार | |
|---|---|---|---|---|---|
| 104 स्थिर | १०३.९०४०३०५ ± ०.०००००१४ | 11.1400% ± 0.0800% | स्थिर | stable | |
| 105 स्थिर | १०४.९०५०७९६ ± ०.०००००१२ | 22.3300% ± 0.0800% | स्थिर | stable | |
| 106 स्थिर | १०५.९०३४८०४ ± ०.०००००१२ | 27.3300% ± 0.0300% | स्थिर | stable | |
| 108 स्थिर | १०७.९०३८९१६ ± ०.०००००१२ | 26.4600% ± 0.0900% | स्थिर | stable |
वर्णरेषा
| तरंगलांबी (nm) | तीव्रता | आयनीकरण टप्पा | प्रकार | संक्रमण | अचूकता | स्रोत | |
|---|---|---|---|---|---|---|---|
| 383.2286 nm | 1500 | Pd I | emission | 4d9.(2D<3/2>).5s 2[3/2] → 4d9.(2D<5/2>).5p 2[3/2]* | मोजलेले | NIST | |
| 389.41982 nm | 2200 | Pd I | emission | 4d9.(2D<3/2>).5s 2[3/2] → 4d9.(2D<5/2>).5p 2[5/2]* | मोजलेले | NIST | |
| 395.86229 nm | 1500 | Pd I | emission | 4d9.(2D<3/2>).5s 2[3/2] → 4d9.(2D<5/2>).5p 2[5/2]* | मोजलेले | NIST | |
| 408.73428 nm | 290 | Pd I | emission | 4d9.(2D<3/2>).5s 2[3/2] → 4d9.(2D<5/2>).5p 2[3/2]* | मोजलेले | NIST | |
| 416.98387 nm | 90 | Pd I | emission | 4d9.(2D<3/2>).5s 2[3/2] → 4d9.(2D<5/2>).5p 2[3/2]* | मोजलेले | NIST | |
| 421.29533 nm | 2500 | Pd I | emission | 4d9.(2D<3/2>).5s 2[3/2] → 4d9.(2D<5/2>).5p 2[7/2]* | मोजलेले | NIST | |
| 447.35846 nm | 180 | Pd I | emission | 4d9.(2D<3/2>).5s 2[3/2] → 4d9.(2D<5/2>).5p 2[3/2]* | मोजलेले | NIST | |
| 478.81874 nm | उपलब्ध नाही | Pd I | emission | 4d9.(2D<5/2>).5p 2[3/2]* → 4d9.(2D<5/2>).5d 2[5/2] | मोजलेले | NIST | |
| 481.75067 nm | उपलब्ध नाही | Pd I | emission | 4d9.(2D<5/2>).5p 2[3/2]* → 4d9.(2D<5/2>).5d 2[3/2] | मोजलेले | NIST | |
| 487.54251 nm | 35 | Pd I | emission | 4d9.(2D<5/2>).5p 2[3/2]* → 4d9.(2D<5/2>).5d 2[1/2] | मोजलेले | NIST | |
| 511.08092 nm | 55 | Pd I | emission | 4d9.(2D<5/2>).5p 2[7/2]* → 4d9.(2D<5/2>).5d 2[7/2] | मोजलेले | NIST | |
| 511.70072 nm | 75 | Pd I | emission | 4d9.(2D<3/2>).5p 2[5/2]* → 4d9.(2D<3/2>).5d 2[7/2] | मोजलेले | NIST | |
| 516.38405 nm | 160 | Pd I | emission | 4d9.(2D<5/2>).5p 2[7/2]* → 4d9.(2D<5/2>).5d 2[9/2] | मोजलेले | NIST | |
| 523.48612 nm | 55 | Pd I | emission | 4d9.(2D<5/2>).5p 2[7/2]* → 4d9.(2D<5/2>).5d 2[7/2] | मोजलेले | NIST | |
| 529.56266 nm | 120 | Pd I | emission | 4d9.(2D<5/2>).5p 2[7/2]* → 4d9.(2D<5/2>).5d 2[9/2] | मोजलेले | NIST | |
| 531.25867 nm | 18 | Pd I | emission | 4d9.(2D<5/2>).5p 2[3/2]* → 4d9.(2D<5/2>).5d 2[5/2] | मोजलेले | NIST | |
| 534.51048 nm | 15 | Pd I | emission | 4d9.(2D<3/2>).5p 2[5/2]* → 4d9.(2D<3/2>).5d 2[5/2] | मोजलेले | NIST | |
| 539.52204 nm | 35 | Pd I | emission | 4d9.(2D<3/2>).5p 2[5/2]* → 4d9.(2D<3/2>).5d 2[7/2] | मोजलेले | NIST | |
| 554.28067 nm | 55 | Pd I | emission | 4d9.(2D<5/2>).5p 2[5/2]* → 4d9.(2D<5/2>).5d 2[7/2] | मोजलेले | NIST | |
| 554.70204 nm | 35 | Pd I | emission | 4d9.(2D<5/2>).5p 2[5/2]* → 4d9.(2D<5/2>).5d 2[5/2] | मोजलेले | NIST | |
| 561.94631 nm | 27 | Pd I | emission | 4d9.(2D<3/2>).5p 2[3/2]* → 4d9.(2D<3/2>).5d 2[5/2] | मोजलेले | NIST | |
| 564.27039 nm | 15 | Pd I | emission | 4d9.(2D<3/2>).5p 2[1/2]* → 4d9.(2D<3/2>).5d 2[3/2] | मोजलेले | NIST | |
| 565.54366 nm | 14 | Pd I | emission | 4d9.(2D<3/2>).5p 2[3/2]* → 4d9.(2D<3/2>).5d 2[5/2] | मोजलेले | NIST | |
| 567.00702 nm | 75 | Pd I | emission | 4d9.(2D<5/2>).5p 2[5/2]* → 4d9.(2D<5/2>).5d 2[7/2] | मोजलेले | NIST | |
| 569.0128 nm | 11 | Pd I | emission | 4d9.(2D<3/2>).5p 2[1/2]* → 4d9.(2D<3/2>).5d 2[3/2] | मोजलेले | NIST | |
| 569.50921 nm | उपलब्ध नाही | Pd I | emission | 4d9.(2D<5/2>).5p 2[5/2]* → 4d9.(2D<5/2>).5d 2[5/2] | मोजलेले | NIST | |
| 573.66175 nm | 18 | Pd I | emission | 4d9.(2D<5/2>).5p 2[5/2]* → 4d9.(2D<5/2>).5d 2[3/2] | मोजलेले | NIST | |
| 677.45174 nm | 23 | Pd I | emission | 4d8.5s2 3F → 4d9.(2D<3/2>).5p 2[5/2]* | मोजलेले | NIST | |
| 678.44893 nm | 65 | Pd I | emission | 4d9.(2D<5/2>).5p 2[3/2]* → 4d9.(2D<5/2>).6s 2[5/2] | मोजलेले | NIST | |
| 683.3446 nm | उपलब्ध नाही | Pd I | emission | 4d9.(2D<3/2>).5p 2[3/2]* → 4d9.(2D<5/2>).5d 2[5/2] | मोजलेले | NIST | |
| 701.6446 nm | 11 | Pd I | emission | 4d9.(2D<3/2>).5p 2[1/2]* → 4d9.(2D<3/2>).6s 2[3/2] | मोजलेले | NIST | |
| 731.0053 nm | उपलब्ध नाही | Pd I | emission | 4d9.(2D<3/2>).5p 2[5/2]* → 4d9.(2D<3/2>).6s 2[3/2] | मोजलेले | NIST | |
| 736.8096 nm | 75 | Pd I | emission | 4d9.(2D<5/2>).5p 2[7/2]* → 4d9.(2D<5/2>).6s 2[5/2] | मोजलेले | NIST | |
| 739.19 nm | 27 | Pd I | emission | 4d9.(2D<3/2>).5p 2[5/2]* → 4d9.(2D<3/2>).6s 2[3/2] | मोजलेले | NIST | |
| 748.6909 nm | 16 | Pd I | emission | 4d9.(2D<5/2>).5p 2[7/2]* → 4d9.(2D<5/2>).6s 2[5/2] | मोजलेले | NIST |
विस्तारित गुणधर्म
सहसंयुजी त्रिज्या (विस्तारित)
- सहसंयुजी त्रिज्या (प्युक्को)
- 120 pm
- सहसंयुजी त्रिज्या (प्युक्को, दुहेरी बंध)
- 117 pm
- सहसंयुजी त्रिज्या (प्युक्को, तिहेरी बंध)
- 112 pm
व्हॅन डर वाल्स त्रिज्या
- Batsanov
- 205 pm
- Alvarez
- 215 pm
- UFF
- 289.9 pm
- MM3
- 237 pm
अणुत्रिज्या आणि धात्विक त्रिज्या
- अणुत्रिज्या (राह्म)
- 215 pm
- धात्विक त्रिज्या (C12)
- 137 pm
क्रमांकन मापनपट्ट्या
- Mendeleev
- 68
- Pettifor
- 69
- Glawe
- 65
विद्युतऋणता मापनपट्ट्या
- Ghosh
- 0
- Miedema
- 5
- Gunnarsson–Lundqvist
- 3
- Robles–Bartolotti
- 2
ध्रुवणक्षमता आणि अपस्करण
- द्विध्रुव ध्रुवणक्षमता
- 26.14 a.u.
- द्विध्रुव ध्रुवणक्षमता (अनिश्चितता)
- 0.1 a.u.
- C₆ (Gould–Bučko)
- 628 Ha·Bohr6
रासायनिक आसक्ती
- प्रोटॉन आसक्ती
- 696 kJ/mol
- वायूची क्षारकता
- 673.4 kJ/mol
मिडेमा प्राचल
- मिडेमा मोलर आयतन
- 8.9 cm3/mol
- मिडेमा इलेक्ट्रॉन घनता
- 5
पुरवठा जोखीम आणि अर्थकारण
- उत्पादनाचे केंद्रीकरण
- 60
- सापेक्ष पुरवठा जोखीम
- 8
- साठ्यांचे वितरण
- 95
- राजकीय स्थैर्य (प्रमुख उत्पादक)
- 44
- राजकीय स्थैर्य (सर्वाधिक साठे असलेला देश)
- 44
अवस्थांतरे आणि अपरूपे
| द्रवणांक | 1827.95 K |
| उत्कलनांक | 3236.15 K |
ऑक्सिडीकरण अवस्थांचे वर्ग
प्रगत संदर्भ माहिती
परिरक्षण स्थिरांक (9)
| n | कक्षिका | σ |
|---|---|---|
| 1 | s | 0.9411 |
| 2 | p | 4.07 |
| 2 | s | 12.1172 |
| 3 | d | 14.5489 |
| 3 | p | 16.9804 |
| 3 | s | 16.7788 |
| 4 | d | 32.3824 |
| 4 | p | 28.2768 |
| 4 | s | 27.014 |
स्फटिक त्रिज्यांचा तपशील (5)
| विद्युतभार | CN | प्रचक्रण | rcrystal (pm) | उत्पत्ती |
|---|---|---|---|---|
| 1 | II | 73 | ||
| 2 | IVSQ | 78 | ||
| 2 | VI | 100 | ||
| 3 | VI | 90 | ||
| 4 | VI | 75.5 | from r^3 vs V plots, |
समस्थानिक क्षय प्रकार (62)
| समस्थानिक | मोड | तीव्रता |
|---|---|---|
| 90 | B+ | — |
| 90 | B+p | — |
| 90 | 2p | — |
| 91 | B+ | 100% |
| 91 | B+p | 3.1% |
| 92 | B+ | 100% |
| 92 | B+p | 1.6% |
| 93 | B+ | 100% |
| 93 | B+p | 7.4% |
| 94 | B+ | 100% |
क्ष-किरण प्रकीर्णन गुणक (507)
| ऊर्जा (eV) | f₁ | f₂ |
|---|---|---|
| 10 | — | 1.15058 |
| 10.1617 | — | 1.2095 |
| 10.3261 | — | 1.27144 |
| 10.4931 | — | 1.33655 |
| 10.6628 | — | 1.40499 |
| 10.8353 | — | 1.47694 |
| 11.0106 | — | 1.54695 |
| 11.1886 | — | 1.61473 |
| 11.3696 | — | 1.68548 |
| 11.5535 | — | 1.75934 |
अतिरिक्त माहिती
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
1.5×10-2 milligrams per kilogram
संदर्भ (1)
- [5] Palladium https://education.jlab.org/itselemental/ele046.html
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
Not Applicable
संदर्भ (1)
- [5] Palladium https://education.jlab.org/itselemental/ele046.html
Sources
Sources of this element.
Discovered in 1803 by Wollaston, Palladium is found with platinum and other metals of the platinum group in placer deposits of Russia, South America, North America, Ethiopia, and Australia. It is also found associated with the nickel-copper deposits of South Africa and Ontario. Palladium's separation from the platinum metals depends upon the type of ore in which it is found.
संदर्भ (1)
- [6] Palladium https://periodic.lanl.gov/46.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 Palladium.
The element property data was retrieved from publications.