Dysprosium (Dy)
lanthanideSolid
प्रमाणित अणुभार
162.5 uइलेक्ट्रॉन संरूपण
[Xe] 6s2 4f10द्रवणांक
1411.85 °Cउत्कलनांक
2566.85 °Cघनता
8550 kg/m³ऑक्सिडीकरण अवस्था
0, +1, +2, +3, +4विद्युतऋणता (पॉलिंग)
1.22आयनीकरण ऊर्जा (पहिली)
5.939061 eVशोधाचे वर्ष
1878अणुत्रिज्या
175 pmतपशील
Dysprosium is a heavy lanthanide metal with atomic number 66. In compounds it is overwhelmingly trivalent, forming pale salts whose chemistry resembles that of neighboring rare earths. Its technological importance comes from an unusually large magnetic moment and strong magnetic anisotropy, especially when incorporated into high-performance permanent magnets. Natural dysprosium is a mixture of stable isotopes and is obtained with other rare earth elements rather than as a native metal.
The element has a metallic, bright silver luster. It is relatively stable in air at room temperature, and is readily attacked and dissolved by dilute and concentrated mineral acids, to evolve hydrogen. The metal is soft enough to be cut with a knife and can be machined without sparking if overheating is avoided. Small amounts of impurities can greatly affect its physical properties.
The name derives from the Greek dysprositos for "hard to get at", owing to the difficulty in separating this rare earth element from a holmium mineral in which it was found. It was discovered by the Swiss chemist Marc Delafontaine in the mineral samarskite in 1878 and called philippia. Philippia was subsequently thought to be a mixture of terbium and yttrium. It was later rediscovered in a holmium sample by the French chemist Paul-Emile Lecoq de Boisbaudran in 1886, who was then credited with the discovery. Dysprosium was first isolated by the French chemist Georges Urbain in 1906.
Dysprosium was discovered by Paul-Émile Lecoq de Boisbaudran, a French chemist, in 1886 as an impurity in erbia, the oxide of erbium. The metal was isolated by Georges Urbain, another French chemist, in 1906. Pure samples of dysprosium were first produced in the 1950s. Today, dysprosium is primarily obtained through an ion exchange process from monazite sand ((Ce, La, Th, Nd, Y)PO4), a material rich in rare earth elements.
From the Greek word dysprositos, meaning hard to get at. Dysprosium was discovered in 1886 by Lecoq de Boisbaudran, but not isolated. Neither the oxide nor the metal was available in relatively pure form until 1950, when the development of ion-exchange separation and metallographic reduction techniques were created by Spedding and associates. Dysprosium occurs along with other so-called rare-earth or lanthanide elements in a variety of minerals such as xenotime, fergusonite, gadolinite, euxenite, polycrase, and blomstrandine. The most important sources, however, are from monaziate and bastnasite. Dysprosium can be prepared by reduction of the trifluoride with calcium.
Pure dysprosium is a bright, silvery metal when freshly cut, but it slowly tarnishes in air. It is relatively soft and can be machined, though the metal is reactive enough that clean surfaces require protection. At ordinary temperature it is paramagnetic; it develops more ordered magnetic states only at low temperatures.
The largest practical use of dysprosium is as an additive to neodymium-iron-boron permanent magnets, where it improves resistance to demagnetization at elevated temperature. This is important in traction motors, wind-turbine generators, and compact actuators, although manufacturers try to minimize the amount used because supply is constrained. Dysprosium is also used in Terfenol-D magnetostrictive alloy, in some specialty lighting and laser materials, and as neutron-absorbing material in selected nuclear-technology applications.
There are no commercial applications for dysprosium. Since it easily absorbs neutrons and has a high melting point, dysprosium might be alloyed with steel for use in nuclear reactors. When combined with vanadium and other rare earth elements, dysprosium is used as a laser material.
Dysprosium oxide (Dy2O3), also known as dysprosia, is combined with nickel and added to a special cement used to cool nuclear reactor rods. Other dysprosium compounds include: dysprosium fluoride (DyF3), dysprosium iodide (DyI3) and dysprosium sulfate (Dy2(SO4)3).
While we have not found many applications for dysprosium, its thermal neutron absorption cross-section and high melting point suggest metallurgical uses in nuclear control applications and for alloying with special stainless steels. A dysprosium oxide-nickel cement has found use in cooling nuclear reactor rods. This cement absorbs neutrons readily without swelling or contracting under prolonged neutron bombardment. In combination with vanadium and other rare earths, dysprosium has been used in making laser materials. Dysprosium-cadmium chalcogenides, as sources of infrared radiation, have been used for studying chemical reactions.
Isotopes in Industry
The isotopes of dysprosium are highly magnetic and have been the subject of physics research involving interactions of isotopes and the structure of lattice supersolids (spatially ordered material with superfluid properties, i.e. zero viscosity). The Magneto-Optical Trapping (MOT) chamber is used for slowing atoms (isotopes) to study the physics of neutral atoms by using a laser light to cool atoms (“Doppler cooling”) and magnetic quadrupole fields to slow and “trap” the neutral atoms (Fig. IUPAC.66.1) [462] S. H. Youn, M. Lu, U. Ray, B. L. Lev. Am. Phys. Soc. Phys. Rev. A.82, 043425 (2010). https://doi.org/10.1103/PhysRevA.82.043425., [463] C. M. Elliott. First Dysprosium MOT, Physics Illinois-University of Illinois at Urbana-Champaign (2017), Feb. 28; http://engineering.illinois.edu/news/article/2009-07-31-first-dysprosium-mot..
164Dy has a large neutron absorption cross section, so dysprosium is used for control rods [464] V. E. Ceron, J. G. Hirsch. Phys. Lett. B471, 1 (1999).. 161Dy has been a key isotope for studying the Mössbauer Effect, which is the resonance and absorption of gamma ray emissions on nearby atoms in a solid state [465] R. L. Cohen. Phys. Rev.137, 1809 (1965)..
Isotopes in Medicine
165Dy (with a half-life of 140 min) is commonly used in arthritis therapy (radiosynovectomy). Rheumatic inflammation of the membranes of joints is often treated by the injection of 165Dy-ferric oxide directly into the joint space of the knee. Leakage from the joint has been shown to be minimal [467] C. B. Sledge, J. D. Zuckerman, M. R. Zalutsky, R. W. Atcher, S. Shortkroff, D. R. Lionberger, H. A. Rose, B. J. Hurson, P. A. Lankenner, R. J. Anderson, W. A. Bloomer. Arthritis Rheum.29, 153 (1986)..
Isotopes Used as a Source of Radioactive Isotope(s)
164Dy is used to produce 166Dy (with a half-life of 3.4 days) via double neutron capture [468] D. Ma, A. R. Ketring, G. J. Ehrhardt, W. Jia. J. Radioanal. Nucl. Chem.206, 119 (1996)., [469] S. Mirzadeh, R. E. Schenter, A. P. Callahan, F. F. Knapp. Production Capabilities in U.S. Nuclear Reactors for Medical Radioisotopes, Tm-12010, Oak Ridge National Laboratory Oak Ridge, Tenn (1992)., [470] S. Lahiri, K. J. Volkers, B. Wierczinski. Appl. Radiat. Isot.61, 1157 (2004).. 166Dy, which decays to 166Ho, is used in cancer and arthritis therapy [468] D. Ma, A. R. Ketring, G. J. Ehrhardt, W. Jia. J. Radioanal. Nucl. Chem.206, 119 (1996)., [471] G. Ferro-Flores, O. Hernandez-Oviedo, C. Arteaga de Murphy, J. I. Tendilla, F. Monroy-Guzman, M. Pedraza-Lopez, K. Aldama-Alvarado. Appl. Radiat. Isot.61, 1227 (2004)..
Dysprosium chemistry is dominated by the +3 oxidation state, represented by dysprosium(III) oxide, Dy₂O₃, dysprosium(III) chloride, DyCl₃, and many hydrated salts. The Dy³⁺ ion is strongly paramagnetic because of its 4f electrons, which are shielded enough to give sharp optical transitions in some host crystals. Dysprosium(II) compounds are uncommon and require strongly reducing conditions; +4 chemistry is not a normal feature of dysprosium. Many minerals contain dysprosium only as a minor component substituting for other heavy rare earth ions.
See more information at the Dysprosium compound page.
Dysprosium metal dust and filings can burn, and the metal reacts slowly with moisture to form hydrogen, H₂, and hydroxides or oxides. Soluble dysprosium salts should be handled as toxicologically uncertain rare-earth compounds rather than as harmless materials; ingestion or inhalation of dust is undesirable. Natural dysprosium is not significantly radioactive, but activated dysprosium isotopes can present radiation hazards in nuclear settings.
Dysprosium occurs dispersed in minerals such as xenotime and ion-adsorption clays, where it substitutes for other trivalent rare earth elements. Weathering and processing can mobilize rare-earth ions, but dysprosium generally has low solubility in neutral to alkaline waters because it forms insoluble phosphates, carbonates, and hydroxides. It has no known biological function. Environmental concern is usually tied to mining, acid leaching, and waste management rather than to natural background concentrations.
Dysprosium is produced as a separated rare earth from mixed ores and concentrates, not from dedicated dysprosium minerals. The main industrial challenge is separation from chemically similar lanthanides by solvent extraction or ion-exchange processes. Demand is strongly linked to high-temperature permanent magnets, while supply is limited by the availability of heavy rare-earth feedstocks. Recycling from magnets is technically possible and increasingly important, but collection, separation, and alloy complexity limit recovery. Substitution strategies include reducing dysprosium content, using grain-boundary diffusion, or redesigning motors to need less coercivity.
Usually found with erbium, holmium and other rare earths in some minerals such as monazite sand, which is often 50% rare earth by weight.
Dysprosium is a rare cosmic element. Its stable isotopes are produced mainly by slow and rapid neutron-capture processes in evolved stars and explosive stellar environments, then incorporated into interstellar dust and later planetary materials. In the Solar System it is concentrated with other refractory rare earths in silicate and phosphate phases rather than in metallic cores or volatile reservoirs.
- The name dysprosium comes from a Greek word meaning “hard to get at,” reflecting its difficult separation from other lan
- Dysprosium has one of the highest thermal-neutron absorption cross sections among stable elements.
- A small dysprosium addition can greatly raise the coercivity of Nd₂Fe₁₄B-based magnets.
- The isotope ¹⁶⁴Dy is the most abundant naturally occurring dysprosium isotope.
- Dysprosium metal can be cut with ordinary tools, but fresh surfaces tarnish readily.
प्रतिमा
गुणधर्म
भौतिक
- अणुत्रिज्या (अनुभवाधारित)
- 175 pm सर्व घटकांच्या अणुत्रिज्या (अनुभवाधारित) ची तुलना करा →
- सहसंयुजी त्रिज्या
- 192 pm सर्व घटकांच्या सहसंयुजी त्रिज्या ची तुलना करा →
- व्हॅन डर वाल्स त्रिज्या
- 229 pm सर्व घटकांच्या व्हॅन डर वाल्स त्रिज्या ची तुलना करा →
- घनता
- 8550 kg/m³ सर्व घटकांच्या घनता ची तुलना करा →
- मोलर आयतन
- 0.019 L/mol
- STP येथे अवस्था
- घन सर्व घटकांच्या STP येथे अवस्था ची तुलना करा →
- द्रवणांक
- 1411.85 °C सर्व घटकांच्या द्रवणांक ची तुलना करा →
- उत्कलनांक
- 2566.85 °C सर्व घटकांच्या उत्कलनांक ची तुलना करा →
- उष्णता चालकता
- 10.7 W/(m·K) सर्व घटकांच्या उष्णता चालकता ची तुलना करा →
- विशिष्ट उष्माधारकता
- 0.173 J/(g·K) सर्व घटकांच्या विशिष्ट उष्माधारकता ची तुलना करा →
- मोलर उष्माधारकता
- 28.16 J/(mol·K) सर्व घटकांच्या मोलर उष्माधारकता ची तुलना करा →
- स्फटिक संरचना
- षट्कोणी निकट-संकुलित सर्व घटकांच्या स्फटिक संरचना ची तुलना करा →
रासायनिक
- विद्युतऋणता (पॉलिंग)
- 1.22 सर्व घटकांच्या विद्युतऋणता (पॉलिंग) ची तुलना करा →
- इलेक्ट्रॉन आसक्ती
- 0.352 eV
- आयनीकरण ऊर्जा (पहिली)
- 5.939061 eV सर्व घटकांच्या आयनीकरण ऊर्जा (पहिली) ची तुलना करा →
- आयनीकरण ऊर्जा (दुसरी)
- 11.64704 eV सर्व घटकांच्या आयनीकरण ऊर्जा (दुसरी) ची तुलना करा →
- आयनीकरण ऊर्जा (तिसरी)
- 22.890079 eV सर्व घटकांच्या आयनीकरण ऊर्जा (तिसरी) ची तुलना करा →
- आयनीकरण ऊर्जा (चौथी)
- 41.230142 eV सर्व घटकांच्या आयनीकरण ऊर्जा (चौथी) ची तुलना करा →
- आयनीकरण ऊर्जा (पाचवी)
- 62.100214 eV सर्व घटकांच्या आयनीकरण ऊर्जा (पाचवी) ची तुलना करा →
- ऑक्सिडीकरण अवस्था
- 0, +1, +2, +3, +4 सर्व घटकांच्या ऑक्सिडीकरण अवस्था ची तुलना करा →
- संयुजा इलेक्ट्रॉन
- 3 सर्व घटकांच्या संयुजा इलेक्ट्रॉन ची तुलना करा →
- इलेक्ट्रॉन संरूपण
- [Xe] 6s2 4f10
उष्मागतिक
- द्रवण उष्मा
- 0.11504379 eV सर्व घटकांच्या द्रवण उष्मा ची तुलना करा →
- बाष्पीभवन उष्मा
- 2.38379 eV सर्व घटकांच्या बाष्पीभवन उष्मा ची तुलना करा →
- संप्लवन उष्मा
- 3.016013 eV
- अणूकरण उष्मा
- 3.016013 eV
- अणूकरण एन्थाल्पी
- 3.009794 eV
केंद्रकीय
- प्रोटॉन
- 66 सर्व घटकांच्या प्रोटॉन ची तुलना करा →
- न्यूट्रॉन
- 98 सर्व घटकांच्या न्यूट्रॉन ची तुलना करा →
- ज्ञात समस्थानिके
- 39 सर्व घटकांच्या ज्ञात समस्थानिके ची तुलना करा →
- स्थिर समस्थानिके
- 6 सर्व घटकांच्या स्थिर समस्थानिके ची तुलना करा →
- सर्वाधिक स्थिर समस्थानिक
- Dy-164
- शोधाचे वर्ष
- 1878
विपुलता
- विपुलता (पृथ्वीचे कवच)
- 5.2 mg/kg सर्व घटकांच्या विपुलता (पृथ्वीचे कवच) ची तुलना करा →
- विपुलता (महासागर)
- 9.1 × 10−7 mg/L सर्व घटकांच्या विपुलता (महासागर) ची तुलना करा →
स्फटिक संरचना
- जालक स्थिरांक a
- 359 pm
इलेक्ट्रॉन संरचना
- प्रत्येक कवचातील इलेक्ट्रॉन
- 2, 8, 18, 28, 8, 2 सर्व घटकांच्या प्रत्येक कवचातील इलेक्ट्रॉन ची तुलना करा →
ओळखचिन्हे
- CAS क्रमांक
- 7429-91-6 सर्व घटकांच्या CAS क्रमांक ची तुलना करा →
- टर्म चिन्ह
- 5I8
- InChI
- InChI=1S/Dy
- InChI की
- KBQHZAAAGSGFKK-UHFFFAOYSA-N
इलेक्ट्रॉन संरूपण मोजलेले
Dy: 4f¹⁰ 6s²[Xe] 4f¹⁰ 6s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹⁰ 6s²अणुप्रतिमान
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 |
|---|---|---|---|
| 158 स्थिर | १५७.९२४४१५९ ± ०.०००००३१ | 0.0950% | स्थिर |
| 160 स्थिर | १५९.९२५२०४६ ± ०.०००००२ | 2.3290% | स्थिर |
| 161 स्थिर | १६०.९२६९४०५ ± ०.०००००२ | 18.8890% | स्थिर |
| 162 स्थिर | १६१.९२६८०५६ ± ०.०००००२ | 25.4750% | स्थिर |
| 163 स्थिर | १६२.९२८७३८३ ± ०.०००००२ | 24.8960% | स्थिर |
| 164 स्थिर | १६३.९२९१८१९ ± ०.०००००२ | 28.2600% | स्थिर |
अवस्था / स्थिती
कारण: द्रवणांकापेक्षा (1411.85 °C) 1386.8 °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
66 पैकी 10 दाखवले आहेत. आयनाच्या विद्युतभारानुसार चढत्या क्रमाने मांडलेले.
वर्णरेषांचा संग्रह ?
| आयन | विद्युतभार | एकूण वर्णरेषा | संक्रमण संभाव्यता | पातळ्यांची नामांकने |
|---|---|---|---|---|
| Dy I | 0 | 230 | 73 | 73 |
| Dy II | +1 | 421 | 17 | 17 |
ऊर्जा पातळ्यांचा संग्रह ?
| आयन | विद्युतभार | पातळ्या |
|---|---|---|
| Dy I | 0 | 740 |
| Dy II | +1 | 576 |
| Dy III | +2 | 2 |
| Dy IV | +3 | 13 |
| Dy V | +4 | 2 |
| Dy VI | +5 | 2 |
| Dy VII | +6 | 2 |
| Dy VIII | +7 | 2 |
| Dy IX | +8 | 2 |
| Dy X | +9 | 2 |
आयनिक त्रिज्या
| विद्युतभार | समन्वय | प्रचक्रण | त्रिज्या |
|---|---|---|---|
| +2 | 6 | उपलब्ध नाही | 107 pm |
| +2 | 7 | उपलब्ध नाही | 112.99999999999999 pm |
| +2 | 8 | उपलब्ध नाही | 119 pm |
| +3 | 6 | उपलब्ध नाही | 91.2 pm |
| +3 | 7 | उपलब्ध नाही | 97 pm |
| +3 | 8 | उपलब्ध नाही | 102.69999999999999 pm |
| +3 | 9 | उपलब्ध नाही | 108.3 pm |
संयुगे
समस्थानिके (6)
| वस्तुमानांक | अणुवस्तुमान (u) | नैसर्गिक विपुलता | अर्धायुष्य | क्षय प्रकार | |
|---|---|---|---|---|---|
| 158 स्थिर | १५७.९२४४१५९ ± ०.०००००३१ | 0.0950% ± 0.0030% | स्थिर | stable | |
| 160 स्थिर | १५९.९२५२०४६ ± ०.०००००२ | 2.3290% ± 0.0180% | स्थिर | stable | |
| 161 स्थिर | १६०.९२६९४०५ ± ०.०००००२ | 18.8890% ± 0.0420% | स्थिर | stable | |
| 162 स्थिर | १६१.९२६८०५६ ± ०.०००००२ | 25.4750% ± 0.0360% | स्थिर | stable | |
| 163 स्थिर | १६२.९२८७३८३ ± ०.०००००२ | 24.8960% ± 0.0420% | स्थिर | stable | |
| 164 स्थिर | १६३.९२९१८१९ ± ०.०००००२ | 28.2600% ± 0.0540% | स्थिर | stable |
विस्तारित गुणधर्म
सहसंयुजी त्रिज्या (विस्तारित)
- सहसंयुजी त्रिज्या (प्युक्को)
- 167 pm
- सहसंयुजी त्रिज्या (प्युक्को, दुहेरी बंध)
- 133 pm
व्हॅन डर वाल्स त्रिज्या
- Alvarez
- 287 pm
- UFF
- 342.8 pm
- MM3
- 290 pm
अणुत्रिज्या आणि धात्विक त्रिज्या
- अणुत्रिज्या (राह्म)
- 275 pm
क्रमांकन मापनपट्ट्या
- Mendeleev
- 31
- Pettifor
- 25
- Glawe
- 24
विद्युतऋणता मापनपट्ट्या
- Ghosh
- 0
- Miedema
- 3
- Gunnarsson–Lundqvist
- 5
- Robles–Bartolotti
- 4
ध्रुवणक्षमता आणि अपस्करण
- द्विध्रुव ध्रुवणक्षमता
- 163 a.u.
- द्विध्रुव ध्रुवणक्षमता (अनिश्चितता)
- 15 a.u.
- C₆ (Gould–Bučko)
- 2430 Ha·Bohr6
मिडेमा प्राचल
- मिडेमा मोलर आयतन
- 19 cm3/mol
- मिडेमा इलेक्ट्रॉन घनता
- 2
पुरवठा जोखीम आणि अर्थकारण
- उत्पादनाचे केंद्रीकरण
- 97
- सापेक्ष पुरवठा जोखीम
- 10
- साठ्यांचे वितरण
- 50
- राजकीय स्थैर्य (प्रमुख उत्पादक)
- 24
- राजकीय स्थैर्य (सर्वाधिक साठे असलेला देश)
- 24
अवस्थांतरे आणि अपरूपे
| द्रवणांक | 1685.15 K |
| उत्कलनांक | 2840.15 K |
ऑक्सिडीकरण अवस्थांचे वर्ग
प्रगत संदर्भ माहिती
परिरक्षण स्थिरांक (13)
| n | कक्षिका | σ |
|---|---|---|
| 1 | s | 1.2914 |
| 2 | p | 4.3204 |
| 2 | s | 17.2906 |
| 3 | d | 13.6701 |
| 3 | p | 20.1195 |
| 3 | s | 20.6067 |
| 4 | d | 34.982 |
| 4 | f | 39.464 |
| 4 | p | 32.174 |
| 4 | s | 31.408 |
स्फटिक त्रिज्यांचा तपशील (7)
| विद्युतभार | CN | प्रचक्रण | rcrystal (pm) | उत्पत्ती |
|---|---|---|---|---|
| 2 | VI | 121 | ||
| 2 | VII | 127 | ||
| 2 | VIII | 133 | ||
| 3 | VI | 105.2 | from r^3 vs V plots, | |
| 3 | VII | 111 | ||
| 3 | VIII | 116.7 | from r^3 vs V plots, | |
| 3 | IX | 122.3 | from r^3 vs V plots, |
समस्थानिक क्षय प्रकार (56)
| समस्थानिक | मोड | तीव्रता |
|---|---|---|
| 138 | B+ | — |
| 138 | B+p | — |
| 139 | B+ | 100% |
| 139 | B+p | 11% |
| 140 | B+ | — |
| 140 | B+p | — |
| 141 | B+ | 100% |
| 141 | B+p | — |
| 142 | B+ | 100% |
| 142 | e+ | 90% |
क्ष-किरण प्रकीर्णन गुणक (514)
| ऊर्जा (eV) | f₁ | f₂ |
|---|---|---|
| 10 | — | 0.15635 |
| 10.1617 | — | 0.1621 |
| 10.3261 | — | 0.16806 |
| 10.4931 | — | 0.17425 |
| 10.6628 | — | 0.18066 |
| 10.8353 | — | 0.18731 |
| 11.0106 | — | 0.19421 |
| 11.1886 | — | 0.20135 |
| 11.3696 | — | 0.20876 |
| 11.5535 | — | 0.21654 |
अतिरिक्त माहिती
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
5.2 milligrams per kilogram
संदर्भ (1)
- [5] Dysprosium https://education.jlab.org/itselemental/ele066.html
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
9.1×10-7 milligrams per liter
संदर्भ (1)
- [5] Dysprosium https://education.jlab.org/itselemental/ele066.html
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 Dysprosium.
The element property data was retrieved from publications.