38
Sr
Strontium
Atomic Mass 87.62
Electron Configuration [Kr]5s2
Oxidation States +2
Year Discovered 1790

Identifiers

Element Name Strontium
Element Symbol Sr
InChI InChI=1S/Sr
InChIKey CIOAGBVUUVVLOB-UHFFFAOYSA-N

Properties

Atomic Weight

87.62(1)

87.62

87.62

87.62(1)

Electron Configuration

[Kr]5s2

Atomic Radius

Van der Waals Atomic Radius : 249 pm (Van der Waals)

Empirical Atomic Radius : 200pm (Empirical)

Covalent Atomic Radius : 195(10) pm (Covalent)

Oxidation States

+2

2, 1 ​(a strongly basic oxide)

Ground Level

1S0

Ionization Energy

5.695 eV

5.69486745 ± 0.00000012 eV

Electronegativity

Pauling Scale Electronegativity : 0.95(Pauling Scale)

Allen Scale Electronegativity : 0.963(Allen Scale)

Electron Affinity

0eV

-1.51eV

Atomic Spectra

Lines Holdings

Levels Holdings

Physical Description

Solid

Element Classification

Metal

Element Period Number

5

Element Group Number

2 - Alkaline Earth Metal

Density

2.64 grams per cubic centimeter

Melting Point

1050 K (777°C or 1431°F)

777°C

Boiling Point

1655 K (1382°C or 2520°F)

1377°C

Estimated Crustal Abundance

3.70×102 milligrams per kilogram

Estimated Oceanic Abundance

7.9 milligrams per liter

History

The name derives from Strontian, a town in Scotland. The mineral strontianite is found in mines in Strontian. The element was discovered in 1792 by the Scottish chemist and physician Thomas Charles Hope, who observed the brilliant red flame colour of strontium. It was first isolated by the English chemist Humphry Davy in 1808.

Strontium was discovered by Adair Crawford, an Irish chemist, in 1790 while studying the mineral witherite (BaCO3). When he mixed witherite with hydrochloric acid (HCl) he did not get the results he expected. He assumed that his sample of witherite was contaminated with an unknown mineral, a mineral he named strontianite (SrCO3). Strontium was first isolated by Sir Humphry Davy, an English chemist, in 1808 through the electrolysis of a mixture of strontium chloride (SrCl2) and mercuric oxide (HgO). Today, strontium is obtained from two of its most common ores, celestite (SrSO4) and strontianite (SrCO3), by treating them with hydrochloric acid, forming strontium chloride. The strontium chloride, usually mixed with potassium chloride (KCl), is then melted and electrolyzed, forming strontium and chlorine gas (Cl2).

Named after Strontian, a town in Scotland. Isolated by Davey by electrolysis in 1808, however, Adair Crawford recognized a new mineral (strontianite) as differing from other barium minerals in 1790.

Historical Atomic Weights

Year Atomic Weight (uncertainty) [u] Reference
1969 87.62(1) https://doi.org/10.1351/pac197021010091
1961 87.62 https://doi.org/10.1021/ja00881a001
1911 87.63 https://doi.org/10.1021/ja01928a001
1909 87.62 https://doi.org/10.1021/ja01931a001
1902 87.6 https://doi.org/10.1007/BF01370337

Historical Isotopic Abundances

Year Isotope Abundance (uncertainty) Reference
2013 84Sr 0.0056(2) https://doi.org/10.1515/pac-2015-0503
2013 86Sr 0.0986(20) https://doi.org/10.1515/pac-2015-0503
2013 87Sr 0.0700(20) https://doi.org/10.1515/pac-2015-0503
2013 88Sr 0.8258(35) https://doi.org/10.1515/pac-2015-0503
1979 84Sr 0.0056(1) https://doi.org/10.1351/pac198052102349
1979 86Sr 0.0986(1) https://doi.org/10.1351/pac198052102349
1979 87Sr 0.0700(1) https://doi.org/10.1351/pac198052102349
1979 88Sr 0.8258(1) https://doi.org/10.1351/pac198052102349
1975 84Sr 0.005 https://doi.org/10.1351/pac197647010075
1975 86Sr 0.099 https://doi.org/10.1351/pac197647010075
1975 87Sr 0.07 https://doi.org/10.1351/pac197647010075
1975 88Sr 0.826 https://doi.org/10.1351/pac197647010075

Description

Strontium is softer than calcium and decomposes in water more vigorously. It does not absorb nitrogen below 380°C. It should be kept under kerosene to prevent oxidation. Freshly cut strontium has a silvery appearance, but rapidly turns a yellowish color with the formation of the oxide. The finely divided metal ignites spontaneously in air. Volatile strontium salts impart a beautiful crimson color to flames, and these salts are used in pyrotechnics and in the production of flares. Natural strontium is a mixture of four stable isotopes.

Users

Most of the strontium produced today is used in the manufacture of color television picture tubes. It is also used to refine zinc and is combined with iron to make magnets.

Two strontium compounds, strontium carbonate (SrCO3) and strontium nitrate (Sr(NO3)2), burn with a bright, red flame and are used in fireworks and signal flares. Strontium carbonate is also used to make certain kinds of glass and is the base material for making most other strontium compounds.

Strontium-90, a radioactive isotope of strontium, is a common product of nuclear explosions. It has a half-life of about 28.8 years and decays into yttrium-90 through beta decay. Strontium-90 is especially deadly since it has a relatively long half-life, is strongly radioactive and is absorbed by the body, where it accumulates in the skeletal system. The radiation affects the production of new blood cells, which eventually leads to death.

In addition to the medical imaging application described in the image caption above, strontium has found use in producing ferrite magnets and in refining zinc. Strontium titanate is an interesting optical material as it has an extremely high refractive index and an optical dispersion greater than that of diamond. It has been used as a gemstone, but is very soft. It does not occur naturally.

Compounds

Strontium is found chiefly as celestite and strontianite. The metal can be prepared by electrolysis of the fused chloride mixed with potassium chloride, or is made by reducing strontium oxide with aluminum in a vacuum at a temperature at which strontium distills off. Three allotropic forms of the metal exist, with transition points at 235 and 540°C.

See more information at the Strontium compound page.

Element Forms

CID Name Formula SMILES Molecular Weight
5359327 strontium Sr [Sr] 87.62
5486204 strontium-90 Sr [90Sr] 89.90773
104798 strontium(2+) Sr+2 [Sr+2] 87.62
5388880 strontium-89 Sr [89Sr] 88.9074508
3083408 strontium-89(2+) Sr+2 [89Sr+2] 88.9074508
5464271 strontium-85 Sr [85Sr] 84.91293
6335517 strontium-87 Sr [87Sr] 86.90887749
6335835 strontium-86 Sr [86Sr] 85.90926072
6337059 strontium-82 Sr [82Sr] 81.91840
6337617 strontium-88 Sr [88Sr] 87.90561225
56843737 strontium-84 Sr [84Sr] 83.91342
157925 strontium-85(2+) Sr+2 [85Sr+2] 84.91293
6337043 strontium-91 Sr [91Sr] 90.91020
6337062 strontium-92 Sr [92Sr] 91.91104
6337556 strontium-81 Sr [81Sr] 80.92321
6337557 strontium-83 Sr [83Sr] 82.91755
6337582 strontium-80 Sr [80Sr] 79.92452
180072 strontium-90(2+) Sr+2 [90Sr+2] 89.90773
71587231 strontium-87(2+) Sr+2 [87Sr+2] 86.90887749
156022708 strontium-88(2+) Sr+2 [88Sr+2] 87.90561225
10197617 strontium-82(2+) Sr+2 [82Sr+2] 81.91840
76960673 strontium-83(2+) Sr+2 [83Sr+2] 82.91755
76968890 strontium-92(2+) Sr+2 [92Sr+2] 91.91104

Isotopes

Stable Isotope Count 4
Summary Sixteen other unstable isotopes are known to exist. Of greatest importance is 90Sr with a half-life of 29 years. It is a product of nuclear fallout and presents a health problem. This isotope is one of the best long-lived high-energy beta emitters known, and is used in SNAP (Systems for Nuclear Auxilliary Power) devices. These devices hold promise for use in space vehicles, remote weather stations, navigational buoys, etc., and where a lightweight, long-lived, nuclear-electric power source is needed.

Isotopes in Earth/Planetary Science

Stable isotopic fractionation of strontium is small because the relative differences between the masses of strontium stable isotopes are small (mass numbers are 86, 87, and 88 for the most abundant stable isotopes). Also, strontium is not subject to reduction-oxidation reactions in normal terrestrial environments, which would cause isotopic fractionation to be more evident. Nevertheless, current studies are exploring potential applications of stable strontium isotopic fractionation; for example, it has been used as a proxy for temperature during coral growth and for insights into the diets of ancient populations [295], [296].

The relative abundance of natural radiogenic 87Sr in seawater is related to the relative rates of processes that add or remove strontium in the ocean (seafloor spreading, mid-ocean-ridge hydrothermal activity, and continental weathering). Over geologic time, these processes have fluctuated and the isotope-amount ratio n(87Sr)/n(86Sr) has changed systematically. By measuring the n(87Sr)/n(86Sr) ratio in marine fossils of known age, it is possible to identify when such environmental changes occurred. Conversely, it is possible to estimate the ages of marine deposits by comparing measured n(87Sr)/n(86Sr) ratios with the global time chart; this process is known as strontium isotope stratigraphy [297].

[295] A. Rüggeberg, J. Fietzke, V. Liebetrau, A. Eisenhauer, W. C. Dullo, A. Freiwald. Earth Planet. Sci. Lett.269, 570 (2008).
[296] K. J. Knudson, H. M. Williams, J. E. Buikstra, P. D. Tomczak, G. W. Gordon, A. D. Anbar. J. Archaeolog. Sci.37, 2352 (2010).
[297] J. M. McArthur, R. J. Howarth, T. R. Bailey. J. Geol.109, 155 (2001).

Isotopes in Forensic Science and Anthropology

The isotope-amount ratio n(87Sr)/n(86Sr) is highly variable in rocks, minerals, soils, and waters, and it can be transmitted to plants (Fig. IUPAC.38.1), animals, and manufactured materials. Measurements of n(87Sr)/n(86Sr) ratios are used for forensic applications in food authentication (determining where food came from), archaeology, crime-scene investigation, and human migration [298], [299].

Fig. IUPAC.38.1: Variation in strontium isotope-amount ratios of twenty species of exotic wood from thirteen countries (modified from [300]).

[298] B. L. Beard, C. M. Johnson. J. Forensic Sci.45, 1049 (2000).
[299] K. M. Frei, R. Frei. Appl. Geochem.26, 326 (2011).
[300] K. Miller, T. B. Coplen, M. Wieser. “Identification of the geographical origin of exotic wood species using 87Sr/86Sr isotope amount ratios”, in Goldschmidt 22nd Conference, Montreal, Quebec, Canada.

Isotopes in Geochronology

The 87Rb- 87Sr dating technique utilizes the fact that 87Sr is a product of radioactive 87Rb decay (half-life of 4.97×1010 years) and is a useful tool for determining ages of rocks and minerals spanning the age of the Earth (Fig. IUPAC.38.2) [301].

Fig. IUPAC.38.2: Cross plot of n(⁸⁷Sr)/n(⁸⁶Sr) isotope-amount ratio and n(⁸⁷Rb)/n(⁸⁶Sr) amount ratio of sphalerites (zinc sulfide mineral) from the Kipushi base metal deposit, Democratic Republic of Congo (modified from [302]). ⁸⁷Sr is produced by decay of radioactive ⁸⁷Rb. Rock containing higher amounts of ⁸⁷Rb will over time produce higher amounts of ⁸⁷Sr, for example sample KI 1270/128 R. Rock containing lower amounts of ⁸⁷Rb will over time produce smaller amounts of ⁸⁷Sr, for example sample KI 1270/113 R. Assuming all the sphalerites in this figure were formed at the same time, one can determine the age of formation of the sulfides from the slope of the line through the data points, here (451.1 ± 6.0)×10⁶ a, and this line is called an isochron.

[301] G. Faure. Principles of Isotope Geology, 2nd Edition. p. 608. Wiley, New York (1986).
[302] J. Schneider, F. Melcher, M. Brauns. Miner Depos.42, 791 (2007).

Isotope Mass and Abundance

Isotope Atomic Mass (uncertainty) [u] Abundance (uncertainty)
84Sr 83.913 419(8) 0.0056(2)
86Sr 85.909 260 73(4) 0.0986(20)
87Sr 86.908 877 50(3) 0.0700(20)
88Sr 87.905 612 26(4) 0.8258(35)
Isotope Atomic Mass (uncertainty) [u] Abundance (uncertainty)
84Sr 83.9134191(13) 0.0056(1)
86Sr 85.9092606(12) 0.0986(1)
87Sr 86.9088775(12) 0.0700(1)
88Sr 87.9056125(12) 0.8258(1)

Atomic Mass, Half Life, and Decay

Nuclide Atomic Mass and Uncertainty [u] Half Life and Uncertainty Discovery Year Decay Modes, Intensities and Uncertainties [%]
73Sr 72.965700 ± 0.00043 [Estimated] 25.3 ms ± 1.4 1993 β+=100%; β+p=63±0.3%
74Sr 73.956170 ± 0.000107 [Estimated] 27.6 ms ± 2.6 1995 β+=100%; β+p ?
75Sr 74.949952767 ± 0.000236183 85.2 ms ± 2.3 1991 β+=100%; β+p=5.2±0.9%
76Sr 75.941762760 ± 0.000037 7.89 s ± 0.07 1990 β+=100%; β+p=3.4e-3±0.8%
77Sr 76.937945454 ± 0.0000085 9.0 s ± 0.2 1976 β+=100%; β+p=0.08±0.3%
78Sr 77.932179979 ± 0.000008 156.1 s ± 2.7 1982 β+=100%
79Sr 78.929704692 ± 0.000007967 2.25 m ± 0.10 1972 β+=100%
80Sr 79.924517538 ± 0.000003718 106.3 m ± 1.5 1961 β+=100%
81Sr 80.923211393 ± 0.000003358 22.3 m ± 0.4 1952 β+=100%
81Srm 80.923211393 ± 0.000003358 390 ns ± 50 1983 IT=100%
81Srn 80.923211393 ± 0.000003358 6.4 us ± 0.5 1989 IT ?
82Sr 81.918399845 ± 0.000006432 25.35 d ± 0.03 1952 ε=100%
83Sr 82.917554372 ± 0.000007336 32.41 h ± 0.03 1952 β+=100%
83Srm 82.917554372 ± 0.000007336 4.95 s ± 0.12 1972 IT=100%
84Sr 83.913419118 ± 0.000001334 Stable 1936 IS=00.56±0.2%; 2β+ ?
85Sr 84.912932041 ± 0.00000302 64.846 d ± 0.006 1940 ε=100%
85Srm 84.912932041 ± 0.00000302 67.63 m ± 0.04 1940 IT=86.6±0.4%; β+=13.4±0.4%
86Sr 85.90926072473 ± 0.00000000563 Stable 1931 IS=9.86±2%
86Srm 85.90926072473 ± 0.00000000563 455 ns ± 7 1971 IT=100%
87Sr 86.90887749454 ± 0.0000000055 Stable 1931 IS=7.00±2%
87Srm 86.90887749454 ± 0.0000000055 2.805 h ± 0.009 1940 IT=99.70±0.8%; ε=0.30±0.8%
88Sr 87.905612253 ± 0.000000006 Stable 1923 IS=82.58±3.5%
89Sr 88.907450808 ± 0.000000098 50.563 d ± 0.025 1937 β-=100%
90Sr 89.907727870 ± 0.000001555 28.91 y ± 0.03 1948 β-=100%
91Sr 90.910195942 ± 0.000005853 9.65 h ± 0.06 1943 β-=100%
92Sr 91.911038222 ± 0.000003675 2.611 h ± 0.017 1956 β-=100%
93Sr 92.914024314 ± 0.000008109 7.43 m ± 0.03 1959 β-=100%
94Sr 93.915355641 ± 0.000001785 75.3 s ± 0.2 1959 β-=100%
95Sr 94.919358282 ± 0.000006237 23.90 s ± 0.14 1961 β-=100%
96Sr 95.921719045 ± 0.000009089 1.059 s ± 0.008 1971 β-=100%; β-n ?
97Sr 96.926375621 ± 0.000003633 432 ms ± 4 1978 β-=100%; β-n=0.02±0.1%
97Srm 96.926375621 ± 0.000003633 175.2 ns ± 2.1 1990 IT=100%
97Srn 96.926375621 ± 0.000003633 513 ns ± 5 1974 IT=100%
98Sr 97.928692636 ± 0.000003463 653 ms ± 2 1971 β-=100%; β-n=0.23±0.3%
99Sr 98.932883604 ± 0.000005085 269.2 ms ± 1.0 1975 β-=100%; β-n=0.100±1.9%
100Sr 99.935783270 ± 0.000007426 202.1 ms ± 1.7 1978 β-=100%; β-n=1.11±3.4%
100Srm 99.935783270 ± 0.000007426 122 ns ± 9 1995 IT=100%
101Sr 100.940606264 ± 0.000009103 113.7 ms ± 1.7 1983 β-=100%; β-n=2.75±3.5%
102Sr 101.944004679 ± 0.000072 69 ms ± 6 1986 β-=100%; β-n=5.5±1.5%
103Sr 102.949243 ± 0.000215 [Estimated] 53 ms ± 10 1997 β-=100%; β-n ?; β-2n ?
104Sr 103.953022 ± 0.000322 [Estimated] 50.6 ms ± 4.2 1997 β-=100%; β-n ?; β-2n ?
105Sr 104.959001 ± 0.000537 [Estimated] 39 ms ± 5 1997 β-=100%; β-n ?; β-2n ?
106Sr 105.963177 ± 0.000644 [Estimated] 21 ms ± 8 2010 β-=100%; β-n ?; β-2n ?
107Sr 106.969672 ± 0.000751 [Estimated] 25 ms >400ns [Estimated] 2010 β- ?; β-n ?; β-2n ?

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
    Strontium

Shall we send you a message when we have discounts available?

Remind me later

Thank you! Please check your email inbox to confirm.

Oops! Notifications are disabled.