Dysprosium (Dy)
lanthanideSolid
मानक परमाणु भार
162.5 uइलेक्ट्रॉन विन्यास
[Xe] 6s2 4f10गलनांक
1411.85 °Cक्वथनांक
2566.85 °Cघनत्व
8550 kg/m³ऑक्सीकरण अवस्थाएँ
0, +1, +2, +3, +4विद्युतऋणात्मकता (पॉलिंग)
1.22आयनन ऊर्जा (प्रथम)
5.939061 eVखोज का वर्ष
1878परमाणु त्रिज्या
175 pmविवरण
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.
चित्र
गुण
भौतिक
- परमाणु त्रिज्या (आनुभविक)
- 175 pm सभी तत्वों की परमाणु त्रिज्या (आनुभविक) की तुलना करें →
- सहसंयोजक त्रिज्या
- 192 pm सभी तत्वों की सहसंयोजक त्रिज्या की तुलना करें →
- वान डर वाल्स त्रिज्या
- 229 pm सभी तत्वों की वान डर वाल्स त्रिज्या की तुलना करें →
- घनत्व
- 8550 kg/m³ सभी तत्वों की घनत्व की तुलना करें →
- मोलर आयतन
- 0.019 L/mol
- STP पर प्रावस्था
- ठोस सभी तत्वों की STP पर प्रावस्था की तुलना करें →
- गलनांक
- 1411.85 °C सभी तत्वों की गलनांक की तुलना करें →
- क्वथनांक
- 2566.85 °C सभी तत्वों की क्वथनांक की तुलना करें →
- तापीय चालकता
- 10.7 W/(m·K) सभी तत्वों की तापीय चालकता की तुलना करें →
- विशिष्ट ऊष्मा धारिता
- 0.173 J/(g·K) सभी तत्वों की विशिष्ट ऊष्मा धारिता की तुलना करें →
- मोलर ऊष्मा धारिता
- 28.16 J/(mol·K) सभी तत्वों की मोलर ऊष्मा धारिता की तुलना करें →
- क्रिस्टल संरचना
- षट्कोणीय सघन संकुलित सभी तत्वों की क्रिस्टल संरचना की तुलना करें →
रासायनिक
- विद्युतऋणात्मकता (पॉलिंग)
- 1.22 सभी तत्वों की विद्युतऋणात्मकता (पॉलिंग) की तुलना करें →
- इलेक्ट्रॉन बंधुता
- 0.352 eV
- आयनन ऊर्जा (प्रथम)
- 5.939061 eV सभी तत्वों की आयनन ऊर्जा (प्रथम) की तुलना करें →
- आयनन ऊर्जा (द्वितीय)
- 11.64704 eV सभी तत्वों की आयनन ऊर्जा (द्वितीय) की तुलना करें →
- आयनन ऊर्जा (तृतीय)
- 22.890079 eV सभी तत्वों की आयनन ऊर्जा (तृतीय) की तुलना करें →
- आयनन ऊर्जा (चतुर्थ)
- 41.230142 eV सभी तत्वों की आयनन ऊर्जा (चतुर्थ) की तुलना करें →
- आयनन ऊर्जा (पंचम)
- 62.100214 eV सभी तत्वों की आयनन ऊर्जा (पंचम) की तुलना करें →
- ऑक्सीकरण अवस्थाएँ
- 0, +1, +2, +3, +4 सभी तत्वों की ऑक्सीकरण अवस्थाएँ की तुलना करें →
- संयोजकता इलेक्ट्रॉन
- 3 सभी तत्वों की संयोजकता इलेक्ट्रॉन की तुलना करें →
- इलेक्ट्रॉन विन्यास
- [Xe] 6s2 4f10
ऊष्मागतिक
- गलन ऊष्मा
- 0.11504379 eV सभी तत्वों की गलन ऊष्मा की तुलना करें →
- वाष्पन ऊष्मा
- 2.38379 eV सभी तत्वों की वाष्पन ऊष्मा की तुलना करें →
- ऊर्ध्वपातन ऊष्मा
- 3.016013 eV
- परमाणुकरण ऊष्मा
- 3.016013 eV
- परमाणुकरण एन्थैल्पी
- 3.009794 eV
नाभिकीय
- प्रोटॉन
- 66 सभी तत्वों की प्रोटॉन की तुलना करें →
- न्यूट्रॉन
- 98 सभी तत्वों की न्यूट्रॉन की तुलना करें →
- ज्ञात समस्थानिक
- 39 सभी तत्वों की ज्ञात समस्थानिक की तुलना करें →
- स्थिर समस्थानिक
- 6 सभी तत्वों की स्थिर समस्थानिक की तुलना करें →
- सबसे स्थिर समस्थानिक
- Dy-164
- खोज का वर्ष
- 1878
प्रचुरता
- प्रचुरता (भूपर्पटी)
- 5.2 mg/kg सभी तत्वों की प्रचुरता (भूपर्पटी) की तुलना करें →
- प्रचुरता (महासागर)
- 9.1 × 10−7 mg/L सभी तत्वों की प्रचुरता (महासागर) की तुलना करें →
क्रिस्टल संरचना
- जालक स्थिरांक a
- 359 pm
इलेक्ट्रॉनिक संरचना
- प्रति कोश इलेक्ट्रॉन
- 2, 8, 18, 28, 8, 2 सभी तत्वों की प्रति कोश इलेक्ट्रॉन की तुलना करें →
पहचानकर्ता
- CAS संख्या
- 7429-91-6 सभी तत्वों की CAS संख्या की तुलना करें →
- टर्म प्रतीक
- 5I8
- InChI
- InChI=1S/Dy
- InChI कुंजी
- KBQHZAAAGSGFKK-UHFFFAOYSA-N
इलेक्ट्रॉन विन्यास मापित
Dy: 4f¹⁰ 6s²[Xe] 4f¹⁰ 6s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹⁰ 6s²परमाणु 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 |
|---|---|---|---|
| 158 स्थिर | 157.9244159 ± 0.0000031 | 0.0950% | स्थिर |
| 160 स्थिर | 159.9252046 ± 0.000002 | 2.3290% | स्थिर |
| 161 स्थिर | 160.9269405 ± 0.000002 | 18.8890% | स्थिर |
| 162 स्थिर | 161.9268056 ± 0.000002 | 25.4750% | स्थिर |
| 163 स्थिर | 162.9287383 ± 0.000002 | 24.8960% | स्थिर |
| 164 स्थिर | 163.9291819 ± 0.000002 | 28.2600% | स्थिर |
प्रावस्था / अवस्था
कारण: गलनांक (1411.85 °C) से 1386.8 °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
परमाणु स्पेक्ट्रम
66 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 |
|---|---|---|---|---|
| Dy I | 0 | 230 | 73 | 73 |
| Dy II | +1 | 421 | 17 | 17 |
उपलब्ध ऊर्जा स्तर डेटा ?
| आयन | आवेश | स्तर |
|---|---|---|
| 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 त्रिज्याएँ
| आवेश | उपसहसंयोजन | प्रचक्रण | त्रिज्या |
|---|---|---|---|
| +2 | 6 | उपलब्ध नहीं | 107 pm |
| +2 | 7 | उपलब्ध नहीं | 112.99999999999999 pm |
| +2 | 8 | उपलब्ध नहीं | 119 pm |
| +3 | 6 | उपलब्ध नहीं | 91.2 pm |
| +3 | 7 | उपलब्ध नहीं | 97 pm |
| +3 | 8 | उपलब्ध नहीं | 102.69999999999999 pm |
| +3 | 9 | उपलब्ध नहीं | 108.3 pm |
यौगिक
समस्थानिक (6)
| द्रव्यमान संख्या | परमाणु द्रव्यमान (u) | प्राकृतिक प्रचुरता | अर्धायु | क्षय का प्रकार | |
|---|---|---|---|---|---|
| 158 स्थिर | 157.9244159 ± 0.0000031 | 0.0950% ± 0.0030% | स्थिर | stable | |
| 160 स्थिर | 159.9252046 ± 0.000002 | 2.3290% ± 0.0180% | स्थिर | stable | |
| 161 स्थिर | 160.9269405 ± 0.000002 | 18.8890% ± 0.0420% | स्थिर | stable | |
| 162 स्थिर | 161.9268056 ± 0.000002 | 25.4750% ± 0.0360% | स्थिर | stable | |
| 163 स्थिर | 162.9287383 ± 0.000002 | 24.8960% ± 0.0420% | स्थिर | stable | |
| 164 स्थिर | 163.9291819 ± 0.000002 | 28.2600% ± 0.0540% | स्थिर | stable |
विस्तृत गुण
सहसंयोजक त्रिज्याएँ (विस्तृत)
- सहसंयोजक त्रिज्या (प्यूक्को)
- 167 pm
- सहसंयोजक त्रिज्या (प्यूक्को, द्विबंध)
- 133 pm
वान डर वाल्स त्रिज्याएँ
- Alvarez
- 287 pm
- UFF
- 342.8 pm
- MM3
- 290 pm
परमाणु और धात्विक त्रिज्याएँ
- परमाणु त्रिज्या (राह्म)
- 275 pm
संख्यांकन मापक्रम
- Mendeleev
- 31
- Pettifor
- 25
- Glawe
- 24
विद्युतऋणात्मकता मापक्रम
- Ghosh
- 0
- Miedema
- 3
- Gunnarsson–Lundqvist
- 5
- Robles–Bartolotti
- 4
ध्रुवणीयता और परिक्षेपण
- द्विध्रुव ध्रुवणीयता
- 163 a.u.
- द्विध्रुव ध्रुवणीयता (अनिश्चितता)
- 15 a.u.
- C₆ (Gould–Bučko)
- 2430 Ha·Bohr6
मीडेमा प्राचल
- मीडेमा मोलर आयतन
- 19 cm3/mol
- मीडेमा इलेक्ट्रॉन घनत्व
- 2
आपूर्ति जोखिम और अर्थशास्त्र
- उत्पादन संकेंद्रण
- 97
- सापेक्ष आपूर्ति जोखिम
- 10
- भंडार वितरण
- 50
- राजनीतिक स्थिरता (प्रमुख उत्पादक)
- 24
- राजनीतिक स्थिरता (सबसे अधिक भंडार वाला देश)
- 24
प्रावस्था संक्रमण और अपररूप
| गलनांक | 1685.15 K |
| क्वथनांक | 2840.15 K |
ऑक्सीकरण अवस्था की श्रेणियाँ
उन्नत संदर्भ डेटा
परिरक्षण स्थिरांक (13)
| n | कक्षक | 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 |
क्रिस्टल त्रिज्याओं का विवरण (7)
| आवेश | CN | प्रचक्रण | rcrystal (pm) | उत्पत्ति |
|---|---|---|---|---|
| 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 के 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% |
एक्स-रे 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 डेटा
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.