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*It is used in yttrium-[[iron]]-[[garnet]] (YIG) and yttrium-[[lanthanum]]-[[fluoride]] (YLF) [[solid state laser]]s found in [[microwave]] equipment (which are in turn found in a variety of medical and dental settings).
*It is used in yttrium-[[iron]]-[[garnet]] (YIG) and yttrium-[[lanthanum]]-[[fluoride]] (YLF) [[solid state laser]]s found in [[microwave]] equipment (which are in turn found in a variety of medical and dental settings).
*It is used as a yellow or red [[glass]] coloring.
*It is used as a black or red [[glass]] coloring.
*Holmium-containing glass has been used as a calibration standard for UV/visible spectrophotometers
*Holmium-containing glass has been used as a calibration standard for UV/visible spectrophotometers
*Holmium is one of the colorants used for [[cubic zirconia]] for use in jewelry, providing a [[Dichroism|dichroic color]] in peach or yellow, depending on the lighting source.
*Holmium is one of the colorants used for [[cubic zirconia]] for use in jewelry, providing a [[Dichroism|dichroic color]] in peach or yellow, depending on the lighting source.
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| volume = 56
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| year = 2002
| year = 1996
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Revision as of 15:49, 9 January 2009

Holmium, 67Ho
Holmium
Pronunciation/ˈhlmiəm/ (HOHL-mee-əm)
Appearancesilvery white
Standard atomic weight Ar°(Ho)
Holmium in the periodic table
Hydrogen Helium
Lithium Beryllium Boron Carbon Nitrogen Oxygen Fluorine Neon
Sodium Magnesium Aluminium Silicon Phosphorus Sulfur Chlorine Argon
Potassium Calcium Scandium Titanium Vanadium Chromium Manganese Iron Cobalt Nickel Copper Zinc Gallium Germanium Arsenic Selenium Bromine Krypton
Rubidium Strontium Yttrium Zirconium Niobium Molybdenum Technetium Ruthenium Rhodium Palladium Silver Cadmium Indium Tin Antimony Tellurium Iodine Xenon
Caesium Barium Lanthanum Cerium Praseodymium Neodymium Promethium Samarium Europium Gadolinium Terbium Dysprosium Holmium Erbium Thulium Ytterbium Lutetium Hafnium Tantalum Tungsten Rhenium Osmium Iridium Platinum Gold Mercury (element) Thallium Lead Bismuth Polonium Astatine Radon
Francium Radium Actinium Thorium Protactinium Uranium Neptunium Plutonium Americium Curium Berkelium Californium Einsteinium Fermium Mendelevium Nobelium Lawrencium Rutherfordium Dubnium Seaborgium Bohrium Hassium Meitnerium Darmstadtium Roentgenium Copernicium Nihonium Flerovium Moscovium Livermorium Tennessine Oganesson


Ho

Es
dysprosiumholmiumerbium
Atomic number (Z)67
Groupf-block groups (no number)
Periodperiod 6
Block  f-block
Electron configuration[Xe] 4f11 6s2
Electrons per shell2, 8, 18, 29, 8, 2
Physical properties
Phase at STPsolid
Melting point1734 K ​(1461 °C, ​2662 °F)
Boiling point2873 K ​(2600 °C, ​4712 °F)
Density (at 20° C)8.795 g/cm3[3]
when liquid (at m.p.)8.34 g/cm3
Heat of fusion17.0 kJ/mol
Heat of vaporization251 kJ/mol
Molar heat capacity27.15 J/(mol·K)
Vapor pressure
P (Pa) 1 10 100 1 k 10 k 100 k
at T (K) 1432 1584 (1775) (2040) (2410) (2964)
Atomic properties
Oxidation statescommon: +3
0,[4] +1,? +2?
ElectronegativityPauling scale: 1.23
Ionization energies
  • 1st: 581.0 kJ/mol
  • 2nd: 1140 kJ/mol
  • 3rd: 2204 kJ/mol
Atomic radiusempirical: 176 pm
Covalent radius192±7 pm
Color lines in a spectral range
Spectral lines of holmium
Other properties
Natural occurrenceprimordial
Crystal structurehexagonal close-packed (hcp) (hP2)
Lattice constants
Hexagonal close packed crystal structure for holmium
a = 357.80 pm
c = 561.77 pm (at 20 °C)[3]
Thermal expansionpoly: 11.2 µm/(m⋅K) (at r.t.)
Thermal conductivity16.2 W/(m⋅K)
Electrical resistivitypoly: 814 nΩ⋅m (at r.t.)
Magnetic orderingparamagnetic
Young's modulus64.8 GPa
Shear modulus26.3 GPa
Bulk modulus40.2 GPa
Speed of sound thin rod2760 m/s (at 20 °C)
Poisson ratio0.231
Vickers hardness410–600 MPa
Brinell hardness500–1250 MPa
CAS Number7440-60-0
History
DiscoveryPer Theodor Cleve, Jacques-Louis Soret and Marc Delafontaine (1878)
Isotopes of holmium
Main isotopes[5] Decay
abun­dance half-life (t1/2) mode pro­duct
163Ho synth 4570 y ε 163Dy
164Ho synth 28.8 min ε 164Dy
β 164Er
165Ho 100% stable
166Ho synth 26.812 h β 166Er
166m1Ho synth 1132.6 y β 166Er
167Ho synth 3.1 h β 167Er
 Category: Holmium
| references

Holmium (Template:PronEng) is a chemical element with the symbol Ho and atomic number 67. Part of the lanthanide series, holmium is a relatively soft and malleable silvery-white metallic element, which is stable in dry air at room temperature. A rare earth metal, it is found in the minerals monazite and gadolinite.

Characteristics

A trivalent metallic rare earth element, holmium has the highest magnetic moment (10.6µB) of any naturally-occurring element and possesses other unusual magnetic properties. When combined with yttrium, it forms highly magnetic compounds.

Holmium is a relatively soft and malleable element that is fairly corrosion-resistant and stable in dry air at standard temperature and pressure. In moist air and at higher temperatures, however, it quickly oxidizes, forming a yellowish oxide. In pure form, holmium possesses a metallic, bright silvery luster. Holmium oxide has some fairly dramatic color changes depending on the lighting conditions. In daylight, it is a tannish yellow color. Under trichromatic light, it is a fiery orange red, almost indistinguishable from the way erbium oxide looks under this same lighting. This has to do with the sharp emission bands of the phosphors, and the absorption bands of both oxides.

Applications

Because of its magnetic properties, holmium has been used to create the strongest artificially-generated magnetic fields when placed within high-strength magnets as a magnetic pole piece (also called a magnetic flux concentrator). Since it can absorb nuclear fission-bred neutrons, the element is also used in nuclear control rods. Other commercial applications of the element abound:

  • It is used in yttrium-iron-garnet (YIG) and yttrium-lanthanum-fluoride (YLF) solid state lasers found in microwave equipment (which are in turn found in a variety of medical and dental settings).
  • It is used as a black or red glass coloring.
  • Holmium-containing glass has been used as a calibration standard for UV/visible spectrophotometers
  • Holmium is one of the colorants used for cubic zirconia for use in jewelry, providing a dichroic color in peach or yellow, depending on the lighting source.
  • Holmium may be used as the active ion in some solid state lasers.
  • The radioactive but long-lived Ho-166m1 (see "Isotopes" below) is used in calibration of gamma ray spectrometers.[6]

History

Holmium (Holmia, Latin name for Stockholm) was discovered by Marc Delafontaine and Jacques-Louis Soret in 1878 who noticed the aberrant spectrographic absorption bands of the then-unknown element (they called it "Element X").[7][8] Later in 1878, Per Teodor Cleve independently discovered the element while he was working on erbia earth (erbium oxide).[9][10]

Using the method developed by Carl Gustaf Mosander, Cleve first removed all of the known contaminants from erbia. The result of that effort was two new materials, one brown and one green. He named the brown substance holmia (after the Latin name for Cleve's home town, Stockholm) and the green one thulia. Holmia was later found to be the holmium oxide and thulia was thulium oxide.

Holmium (as the oxide) would not be obtained reasonably pure until the 20th century, and would not become commercially available in high purity until the late 1950s.[citation needed] The Lindsay Chemical Division of American Potash and Chemical Corporation was one of the first producers, using the newly-developed ion-exchange technology to purify holmium as isolated from monazite, in which it was present in trace amounts.[citation needed] In 1960, one pound of 99% holmium oxide was priced at US $105, and the 99.9% grade cost US $125, which were the same prices as were charged for the comparable oxides of gadolinium, dysprosium, and erbium.[citation needed] One of the early applications was in the form of a glass called a "holmium oxide plate" which was used (by 1965) as a calibration standard for UV/visible spectroscopy. [citation needed]

Occurrence

Like all other rare earths, holmium is not naturally found as a free element. It does occur combined with other elements in the minerals gadolinite, monazite, and in other rare-earth minerals. It is commercially extracted via ion-exchange from monazite sand (0.05% holmium) but is still difficult to separate from other rare earths. The element has been isolated through the reduction of its anhydrous chloride or fluoride with metallic calcium. Its estimated abundance in the Earth's crust is 1.3 milligrams per kilogram. Holmium obeys the Oddo-Harkins rule: as an odd-numbered element, it is less abundant than its immediate even numbered neighbors, dysprosium and erbium. However, it is the most abundant of the odd-numbered heavy lanthanides. The principal current source are some of the ion-adsorption clays of southern China. Some of these have a rare-earth composition similar to that found in xenotime or gadolinite. Yttrium makes up about two-thirds of the total by weight; holmium is around 1.5%. The original ores themselves are very lean, maybe only 0.1% total lanthanide, but are easily extracted.

Isotopes

Natural holmium contains one stable isotope, holmium-165. Some synthetic radioactive isotopes are known, the most stable one is holmium-163, with a half life of 4570 years. All other radioisotopes have ground-state half lives not greater than 1.117 days, and most have half lives under 3 hours. However, the metastable 166m1Ho has a half life of around 1200 years because of its high spin. This fact, combined with a high excitation energy resulting in a particularly rich spectrum of decay gamma rays produced when the metastable state de-excites, makes this isotope useful in nuclear physics experiments as a means for calibrating energy responses and intrinsic efficiencies of gamma ray spectrometers.

Precautions

The element, as with other rare earths, appears to have a low degree of acute toxicity. Holmium plays no biological role in humans but may be able to stimulate metabolism.[citation needed]

See also

References

  1. ^ "Standard Atomic Weights: Holmium". CIAAW. 2021.
  2. ^ Prohaska, Thomas; Irrgeher, Johanna; Benefield, Jacqueline; Böhlke, John K.; Chesson, Lesley A.; Coplen, Tyler B.; Ding, Tiping; Dunn, Philip J. H.; Gröning, Manfred; Holden, Norman E.; Meijer, Harro A. J. (2022-05-04). "Standard atomic weights of the elements 2021 (IUPAC Technical Report)". Pure and Applied Chemistry. doi:10.1515/pac-2019-0603. ISSN 1365-3075.
  3. ^ a b Arblaster, John W. (2018). Selected Values of the Crystallographic Properties of Elements. Materials Park, Ohio: ASM International. ISBN 978-1-62708-155-9.
  4. ^ Yttrium and all lanthanides except Ce and Pm have been observed in the oxidation state 0 in bis(1,3,5-tri-t-butylbenzene) complexes, see Cloke, F. Geoffrey N. (1993). "Zero Oxidation State Compounds of Scandium, Yttrium, and the Lanthanides". Chem. Soc. Rev. 22: 17–24. doi:10.1039/CS9932200017. and Arnold, Polly L.; Petrukhina, Marina A.; Bochenkov, Vladimir E.; Shabatina, Tatyana I.; Zagorskii, Vyacheslav V.; Cloke (2003-12-15). "Arene complexation of Sm, Eu, Tm and Yb atoms: a variable temperature spectroscopic investigation". Journal of Organometallic Chemistry. 688 (1–2): 49–55. doi:10.1016/j.jorganchem.2003.08.028.
  5. ^ Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF). Chinese Physics C. 45 (3): 030001. doi:10.1088/1674-1137/abddae.
  6. ^ Ming-Chen Yuan, Jeng-Hung Lee and Wen-Song Hwang (1996). "The absolute counting of 166mHo, 58Co and 88Y". Applied Radiation and Isotopes. 56 (1–2): 44.
  7. ^ Jacques-Louis Soret (1878). "Sur les spectres d'absorption ultra-violets des terres de la gadolinite". Comptes rendus de l'Académie des sciences. 87: 1062.
  8. ^ Jacques-Louis Soret (1879). "Sur le spectre des terres faisant partie du groupe de l'yttria". Comptes rendus de l'Académie des sciences. 89: 521.
  9. ^ Per Teodor Cleve (1879). "Sur deux nouveaux éléments dans l'erbine". Comptes rendus de l'Académie des sciences. 89: 478.
  10. ^ Per Teodor Cleve (1879). "Sur l'erbine". Comptes rendus de l'Académie des sciences. 89: 708.