62
Sm
Samarium
Atomic Mass 150.36
Electron Configuration [Xe]6s24f6
Oxidation States +3, +2
Year Discovered 1879

Identifiers

Element Name Samarium
Element Symbol Sm
InChI InChI=1S/Sm
InChIKey KZUNJOHGWZRPMI-UHFFFAOYSA-N

Properties

Atomic Weight

150.36(2)

150.36

150.4

150.36(2)

Electron Configuration

[Xe]6s24f6

Atomic Radius

Van der Waals Atomic Radius : 229 pm (Van der Waals)

Empirical Atomic Radius : 185pm (Empirical)

Covalent Atomic Radius : 198(8) pm (Covalent)

Oxidation States

+3, +2

4, 3, 2, 1 ​(a mildly basic oxide)

Ground Level

7F0

Ionization Energy

5.644 eV

5.643722 ± 0.000021 eV

Electronegativity

Pauling Scale Electronegativity : 1.17(Pauling Scale)

Atomic Spectra

Lines Holdings

Levels Holdings

Physical Description

Solid

Element Classification

Metal

Element Period Number

6

Element Group Number

- Lanthanide

Density

7.52 grams per cubic centimeter

Melting Point

1347 K (1074°C or 1965°F)

1072°C

Boiling Point

2067 K (1794°C or 3261°F)

1900°C

Estimated Crustal Abundance

7.05 milligrams per kilogram

Estimated Oceanic Abundance

4.5×10-7 milligrams per liter

History

The name derives from the mineral samarskite, in which it was found and that had been named for Colonel Samarski, a Russian mine official. Samarium was originally discovered in 1878 by the Swiss chemist Marc Delafontaine, who called it decipium. It was also discovered by the French chemist Paul-Emile Lecoq de Boisbaudran in 1879. In 1881, Delafontaine determined that his decipium could be resolved into two elements, one of which was identical to Boisbaudran's samarium. In 1901, the French chemist Eugène-Anatole Demarçay showed that this samarium earth also contained europium.

Samarium was observed spectroscopically by Jean Charles Galissard de Marignac, a Swiss chemist, in a material known as dydimia in 1853. Paul-Émile Lecoq de Boisbaudran, a French chemist, was the first to isolate samarium from the mineral samarskite ((Y, Ce, U, Fe)3(Nb, Ta, Ti)5O16) in 1879. Today, samarium is primarily obtained through an ion exchange process from monazite sand ((Ce, La, Th, Nd, Y)PO4), a material rich in rare earth elements that can contain as much as 2.8% samarium.

Discovered spectroscopically by its sharp absorption lines in 1879 by Lecoq de Boisbaudran in the mineral samarskite, named in honor of a Russian mine official, Col. Samarski.

Historical Atomic Weights

Year Atomic Weight (uncertainty) [u] Reference
2005 150.36(2) https://doi.org/10.1351/pac200678112051
1979 150.36(3) https://doi.org/10.1351/pac198052102349
1969 150.4(1) https://doi.org/10.1351/pac197021010091
1955 150.35 https://doi.org/10.1021/ja01595a001
1925 150.43 https://doi.org/10.1039/CT9252700913
1909 150.4 https://doi.org/10.1021/ja01931a001
1905 150.3 https://doi.org/10.1021/ja01979a001
1902 150 https://doi.org/10.1007/BF01370337

Historical Isotopic Abundances

Year Isotope Abundance (uncertainty) Reference
2013 144Sm 0.0308(4) https://doi.org/10.1515/pac-2015-0503
2013 147Sm 0.1500(14) https://doi.org/10.1515/pac-2015-0503
2013 148Sm 0.1125(9) https://doi.org/10.1515/pac-2015-0503
2013 149Sm 0.1382(10) https://doi.org/10.1515/pac-2015-0503
2013 150Sm 0.0737(9) https://doi.org/10.1515/pac-2015-0503
2013 152Sm 0.2674(9) https://doi.org/10.1515/pac-2015-0503
2013 154Sm 0.2274(14) https://doi.org/10.1515/pac-2015-0503
1997 144Sm 0.0307(7) https://doi.org/10.1351/pac199870010217
1997 147Sm 0.1499(18) https://doi.org/10.1351/pac199870010217
1997 148Sm 0.1124(10) https://doi.org/10.1351/pac199870010217
1997 149Sm 0.1382(7) https://doi.org/10.1351/pac199870010217
1997 150Sm 0.0738(1) https://doi.org/10.1351/pac199870010217
1997 152Sm 0.2675(16) https://doi.org/10.1351/pac199870010217
1997 154Sm 0.2275(29) https://doi.org/10.1351/pac199870010217
1979 144Sm 0.031(1) https://doi.org/10.1351/pac198052102349
1979 147Sm 0.151(2) https://doi.org/10.1351/pac198052102349
1979 148Sm 0.113(1) https://doi.org/10.1351/pac198052102349
1979 149Sm 0.139(1) https://doi.org/10.1351/pac198052102349
1979 150Sm 0.074(1) https://doi.org/10.1351/pac198052102349
1979 152Sm 0.266(2) https://doi.org/10.1351/pac198052102349
1979 154Sm 0.226(2) https://doi.org/10.1351/pac198052102349
1975 144Sm 0.031 https://doi.org/10.1351/pac197647010075
1975 147Sm 0.151 https://doi.org/10.1351/pac197647010075
1975 148Sm 0.113 https://doi.org/10.1351/pac197647010075
1975 149Sm 0.139 https://doi.org/10.1351/pac197647010075
1975 150Sm 0.074 https://doi.org/10.1351/pac197647010075
1975 152Sm 0.266 https://doi.org/10.1351/pac197647010075
1975 154Sm 0.226 https://doi.org/10.1351/pac197647010075

Description

Samarium has a bright silver luster and is reasonably stable in air. Three crystal modifications of the metal exist, with transformations at 734 and 922°C. The metal ignites in air at about 150°C. The sulfide has excellent high-temperature stability and good thermoelectric efficiencies up to 1100°C.

Users

Samarium is one of the rare earth elements used to make carbon arc lights which are used in the motion picture industry for studio lighting and projector lights. Samarium also makes up about 1% of Misch metal, a material that is used to make flints for lighters.

Samarium forms a compound with cobalt (SmCo5) which is a powerful permanent magnet with the highest resistance to demagnetization of any material known. Samarium oxide (Sm2O3) is added to glass to absorb infrared radiation and acts as a catalyst for the dehydration and dehydrogenation of ethanol (C2H6O).

Samarium, along with other rare earths, is used for carbon-arc lighting for the motion picture industry. SmCo5 has been used in making a new permanent magnet material with the highest resistance to demagnetization of any known material. It is said to have an intrinsic coercive force as high as 2200 kA/m. Samarium oxide has been used in optical glass to absorb the infrared. Samarium is used to dope calcium fluoride crystal for use in optical lasers or lasers. Compounds of the metal act as sensitizers for phosphors excited in the infrared; the oxide exhibits catalytic properties in the dehydration and dehydrogenation of ethyl alcohol. It is used in infrared absorbing glass and as a neutron absorber in nuclear reactors.

Sources

Samarium is found along with other members of the rare-earth elements in many minerals, including monazite and bastnasite, which are commercial sources. It occurs in monazite to the extent of 2.8%. While misch metal containing about 1% of samarium metal, has long been used, samarium has not been isolated in relatively pure form until recently. Ion-exchange and solvent extraction techniques have recently simplified separation of the rare earths from one another; more recently, electrochemical deposition, using an electrolytic solution of lithium citrate and a mercury electrode, is said to be a simple, fast, and highly specific way to separate the rare earths. Samarium metal can be produced by reducing the oxide with lanthanum.

Compounds

See more information at the Samarium compound page.

Element Forms

CID Name Formula SMILES Molecular Weight
23951 samarium Sm [Sm] 150.4
114941 samarium-153 Sm [153Sm] 152.92210
119249 samarium(3+) Sm+3 [Sm+3] 150.4
177480 samarium-154 Sm [154Sm] 153.92222
177554 samarium-145 Sm [145Sm] 144.91342
9877421 samarium-152 Sm [152Sm] 151.91974
25087174 samarium-147 Sm [147Sm] 146.91490
44154635 samarium-146 Sm [146Sm] 145.91305
114939 samarium-151 Sm [151Sm] 150.91994
177498 samarium-150 Sm [150Sm] 149.91728
177673 samarium-156 Sm [156Sm] 155.92554
10197772 samarium-149 Sm [149Sm] 148.91719
25086834 samarium-144 Sm [144Sm] 143.91201
167086 samarium-155 Sm [155Sm] 154.92465
177495 samarium-141 Sm [141Sm] 140.91848
177629 samarium-142 Sm [142Sm] 141.91521
90478796 samarium-152(3+) Sm+3 [152Sm+3] 151.91974
90479421 samarium-153(3+) Sm+3 [153Sm+3] 152.92210
25086833 samarium-148 Sm [148Sm] 147.91483
10103390 samarium-157 Sm [157Sm] 156.92842

Handling And Storage

Little is known of the toxicity of samarium; therefore, it should be handled carefully.

Isotopes

Stable Isotope Count 5
Summary Twenty one isotopes of samarium exist. Natural samarium is a mixture of several isotopes, three of which are unstable with long half-lives.

Isotopes in Earth/Planetary Science

One possible origin for the Moon is from debris ejected by an indirect giant impact of Earth by an astronomical body the size of Mars when the Earth was forming [436]. The kinetic energy liberated is thought to have melted a large part of the Moon forming a lunar magma ocean. Samarium isotope measurement results [437], along with measurements of isotopes of hafnium, tungsten, and neodymium[438], suggest that lunar magma formed about 70×106 years after the Solar System formed and had crystallized by about 215×106 years after formation. 147Sm (with a half-life of 1.06×1011 years) is used to study the formation of potassium, rare earth elements, and phosphorus-rich rocks [439].

[436] R. M. Canup, E. Asphaug. Nature412, 708 (2001).
[437] A. Brandon. Nature450, 1169 (2007).
[438] K. Righter, C. K. Shearer. Geochim. Cosmochim. Acta67, 2497 (2003).
[439] J. Edmunson, L. E. Borg. “The formation age of KREEP based on the 147Sm-143Nd geochemistry of KREEP-rich rocks: duration of lunar magma ocean crystallization and similarity to early mars”, in Workshop on Early Planetary Differentiation.

Isotopes in Geochronology

147Sm is used for determining formation ages of igneous and metamorphic rocks via analysis of the minerals which compose them, such as those shown in Fig. IUPAC.62.1 [440], [441], [442].

Fig. IUPAC.62.1: Cross plot of n(¹⁴³Nd)/n(¹⁴⁴Nd) isotope-amount ratio and n(¹⁴⁷Sm)/n(¹⁴⁴Nd) amount ratio of carbonate and fluorocarbonates at the Bayan Obo rare-earth-element-niobium-iron deposit in Inner Mongolia, China (modified from [442]). ¹⁴³Nd is produced by decay of ¹⁴⁷Sm. Rock containing higher amounts of ¹⁴⁷Sm at time of mineralization will over time produce higher amounts of ¹⁴³Nd (e.g. fluorite samples). Alternatively, rocks containing lower amounts of ¹⁴⁷Sm at time of mineralization will over time produce lower amounts of ¹⁴³Nd (e.g. huanghoite samples). Samples from an older mineralization event will have proportionally more ¹⁴³Nd because of the longer accumulation time for ¹⁴³Nd; thus, the slope of the line through the samples above correlates to the time since mineralization (formation), and such a line is called an isochron.

[440] T. Iizuka, O. Nebel, M. McCulloch. Early Crustal Evolution Deduced from a Combined U-Pb and Sm-Nd Isotopic Study of Mt. Narryer and Jack Hills Monazites, The Australian National University (2014), Feb. 28; http://rses.anu.edu.au/highlights/view.php?article=191.
[441] K. Rankenburg, A. D. Brandon, C. R. Neal. Science312 1369 (2006).
[442] F. F. Hu, H. R. Fan, S. Liu, K. F. Yang, F. Chen. Resour. Geol.59, 407 (2009).

Isotopes in Medicine

The radioisotope 153Sm (with a half-life of 1.9 days) is used in medicine to treat the severe pain associated with cancer that has spread to bones (Fig. IUPAC.62.2) [443], [444], [445].

Fig. IUPAC.62.2: Targeting of bone metastases with ¹⁵³Sm-EDTMP in a prostate cancer patient. ANT indicates the anterior view of the patient; POST indicates the posterior view of the patient; arrow represents uptake in the pubic bone of the patient. (Image Source: Pandit-Taskar, Batraki, and Divgi, 2004) [445].

[443] International Atomic Energy Agency. Optimization of Production and Quality Control of Therapeutic Radionuclides and Radiopharmaceuticals, IAEA-TECDOC-1114, IAEA VIENNA (1999).
[444] C. L. Maini, S. Bergomi, L. Romano, R. Sciuto. Eur. J. Nucl. Med. Mol. Imaging31, S171 (2004).
[445] N. Pandit-Taskar, M. Batraki, C. R. Divgi. J. Nucl. Med.45, 1358 (2004).

Isotopes Used as a Source of Radioactive Isotope(s)

147Sm bombarded with 40Ca produces the radioisotope 182Pb [446].

[446] K. S. Toth, D. M. Moltz, J. M. Nitschke, P. A. Wilmarth, J. D. Robertson. AIP Conference Proc.283, 347 (1991).

Isotope Mass and Abundance

Isotope Atomic Mass (uncertainty) [u] Abundance (uncertainty)
144Sm 143.912 01(1) 0.0308(4) 0.0307(7)
147Sm 146.914 90(1) 0.1500(14) 0.1499(18)
148Sm 147.914 83(1) 0.1125(9) 0.1124(10)
149Sm 148.917 191(9) 0.1382(10) 0.1382(7)
150Sm 149.917 282(9) 0.0737(9) 0.0738(1)
152Sm 151.919 739(8) 0.2674(9) 0.2675(16)
154Sm 153.922 22(1) 0.2274(14) 0.2275(29)

Atomic Mass, Half Life, and Decay

Nuclide Atomic Mass and Uncertainty [u] Half Life and Uncertainty Discovery Year Decay Modes, Intensities and Uncertainties [%]
128Sm 127.957971 ± 0.000537 [Estimated] 500 ms [Estimated] β+ ?; β+p ?
129Sm 128.954557 ± 0.000537 [Estimated] 550 ms ± 100 1999 β+=100%; β+p=?
130Sm 129.948792 ± 0.000429 [Estimated] 1 s [Estimated] 1999 β+ ?
131Sm 130.946022 ± 0.000429 [Estimated] 1.2 s ± 0.2 1986 β+=100%; β+p=?
132Sm 131.940805 ± 0.000322 [Estimated] 4.0 s ± 0.3 1989 β+=100%; β+p ?
133Sm 132.938560 ± 0.00032 [Estimated] 2.89 s ± 0.16 1977 β+=100%; β+p=?
133Smm 132.938560 ± 0.00032 [Estimated] 3.5 s ± 0.4 1993 β+=?; IT ?; β+p ?
134Sm 133.934110 ± 0.00021 [Estimated] 9.5 s ± 0.8 1977 β+=100%
135Sm 134.932520000 ± 0.000166 10.3 s ± 0.5 1977 β+=100%; β+p=0.02±0.1%
136Sm 135.928275553 ± 0.000013416 47 s ± 2 1982 β+=100%
136Smm 135.928275553 ± 0.000013416 15 us ± 1 1994 IT=100%
137Sm 136.927007959 ± 0.000030718 45 s ± 1 1986 β+=100%
137Smm 136.927007959 ± 0.000030718 20 s [Estimated] β+ ?
138Sm 137.923243988 ± 0.000012686 3.1 m ± 0.2 1982 β+=100%
139Sm 138.922296631 ± 0.000011684 2.57 m ± 0.10 1971 β+=100%
139Smm 138.922296631 ± 0.000011684 10.7 s ± 0.6 1973 IT=93.7±0.5%; β+=6.3±0.5%
140Sm 139.918994714 ± 0.000013416 14.82 m ± 0.12 1967 β+=100%
141Sm 140.918481545 ± 0.000009162 10.2 m ± 0.2 1967 β+=100%
141Smm 140.918481545 ± 0.000009162 22.6 m ± 0.2 1967 β+=99.69±0.3%; IT=0.31±0.3%
142Sm 141.915209415 ± 0.000002002 72.49 m ± 0.05 1959 β+=100%; e+<5%
142Smm 141.915209415 ± 0.000002002 170 ns ± 2 1975 IT=100%
142Smn 141.915209415 ± 0.000002002 480 ns ± 60 1979 IT=100%
143Sm 142.914634848 ± 0.000002951 8.75 m ± 0.06 1956 β+=100%; e+=40.0±2%; ε=60.0±2%
143Smm 142.914634848 ± 0.000002951 66 s ± 2 1960 IT≈100%; β+=0.24±0.5%
143Smn 142.914634848 ± 0.000002951 30 ms ± 3 1969 IT=100%
144Sm 143.912006285 ± 0.000001566 Stable 1933 IS=3.08±0.4%; 2β+ ?
144Smm 143.912006285 ± 0.000001566 880 ns ± 25 1972 IT=100%
145Sm 144.913417157 ± 0.000001594 340 d ± 3 1947 ε=100%
145Smm 144.913417157 ± 0.000001594 3.52 us ± 0.16 1993 IT=100%
146Sm 145.913046835 ± 0.000003269 68 My ± 7 1953 α=100%
147Sm 146.914904401 ± 0.000001354 106.6 Gy ± 0.5 1933 IS=15.00±1.4%; α=100%
148Sm 147.914829233 ± 0.000001337 6.3 Py ± 1.3 1933 IS=11.25±0.9%; α=100%
149Sm 148.917191211 ± 0.000001241 Stable >2Py 1933 IS=13.82±1%; α ?
150Sm 149.917281993 ± 0.000001193 Stable 1934 IS=7.37±0.9%
151Sm 150.919938859 ± 0.000001191 94.6 y ± 0.6 1947 β-=100%
151Smm 150.919938859 ± 0.000001191 1.4 us ± 0.1 1973 IT=100%
152Sm 151.919738646 ± 0.00000109 Stable 1933 IS=26.74±0.9%
153Sm 152.922103576 ± 0.0000011 46.2846 h ± 0.0023 1938 β-=100%
153Smm 152.922103576 ± 0.0000011 10.6 ms ± 0.3 1971 IT=100%
154Sm 153.922215756 ± 0.0000014 Stable >2.3Ey 1933 IS=22.74±1.4%; 2β- ?
155Sm 154.924646645 ± 0.000001429 22.18 m ± 0.06 1951 β-=100%
155Smm 154.924646645 ± 0.000001429 2.8 us ± 0.5 2010 IT=100%
155Smn 154.924646645 ± 0.000001429 1.00 us ± 0.08 2010 IT=100%
156Sm 155.925538191 ± 0.000009148 9.4 h ± 0.2 1951 β-=100%
156Smm 155.925538191 ± 0.000009148 185 ns ± 7 1974 IT=100%
157Sm 156.928418598 ± 0.000004759 8.03 m ± 0.07 1973 β-=100%
158Sm 157.929949262 ± 0.000005133 5.30 m ± 0.03 1970 β-=100%
159Sm 158.933217130 ± 0.00000637 11.37 s ± 0.15 1986 β-=100%
159Smm 158.933217130 ± 0.00000637 116 ns ± 8 2009 IT=100%
160Sm 159.935337032 ± 0.0000021 9.6 s ± 0.3 1986 β-=100%
160Smm 159.935337032 ± 0.0000021 120 ns ± 46 2009 IT=100%
160Smn 159.935337032 ± 0.0000021 1.8 us ± 0.4 2016 IT=100%
161Sm 160.939160062 ± 0.000007318 4.8 s ± 0.4 1998 β-=100%
161Smm 160.939160062 ± 0.000007318 2.6 us ± 0.4 2017 IT=100%
162Sm 161.941621687 ± 0.000003782 2.7 s ± 0.3 2005 β-=100%
162Smm 161.941621687 ± 0.000003782 1.78 us ± 0.07 2017 IT=100%
163Sm 162.945679085 ± 0.0000079 1.3 s ± 0.5 2012 β-=100%
164Sm 163.948550061 ± 0.0000044 1.43 s ± 0.24 2012 β-=100%; β-n ?
164Smm 163.948550061 ± 0.0000044 600 ns ± 140 2014 IT=100%
165Sm 164.953290 ± 0.000429 [Estimated] 980 ms ± 210 2012 β-=100%; β-n ?
166Sm 165.956575 ± 0.000429 [Estimated] 800 ms ± 630 2017 β-=100%
167Sm 166.962072 ± 0.000537 [Estimated] 190 ms >550ns [Estimated] 2018 β- ?; β-n ?
168Sm 167.966033 ± 0.000322 [Estimated] 340 ms >550ns [Estimated] 2018 β- ?; β-n ?

Information Sources

  1. 1.  PubChem
  2. 2.  Atomic Mass Data Center (AMDC), International Atomic Energy Agency (IAEA)
  3. 3.  IUPAC Commission on Isotopic Abundances and Atomic Weights (CIAAW)
  4. 4.  Jefferson Lab, U.S. Department of Energy
    LICENSE
    Please see citation and linking information https https://www.jlab.org/privacy-and-security-notice
  5. 5.  Los Alamos National Laboratory, U.S. Department of Energy
  6. 6.  NIST Physical Measurement Laboratory
  7. 7.  IUPAC Periodic Table of the Elements and Isotopes (IPTEI)
    LICENSE
    Copyright (c) 2020 International Union of Pure and Applied Chemistry. The International Union of Pure and Applied Chemistry (IUPAC) contribution within Pubchem is provided under a CC-BY-NC-ND 4.0 license, unless otherwise stated.
    https://creativecommons.org/licenses/by-nc-nd/4.0/
  8. 8.  PubChem Elements
    Samarium

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