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Isotopes of osmium

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Isotopes of osmium (76Os)
Main isotopes Decay
abun­dance half-life (t1/2) mode pro­duct
Os 0.02% 1.12×10 y α W
Os synth 92.95 d ε Re
Os 1.59% 2.0×10 y α W
Os 1.96% stable
Os 13.2% stable
Os 16.1% stable
Os 26.3% stable
Os synth 14.99 d β Ir
Os 40.8% stable
Os synth 29.83 h β Ir
Os synth 6 y β Ir
Standard atomic weight Ar°(Os)

Osmium (76Os) has seven naturally occurring isotopes, five of which are stable: Os, Os, Os, Os, and (most abundant) Os. The other natural isotopes, Os, and Os, have extremely long half-life (1.12×10 years and 2×10 years, respectively) and for practical purposes can be considered to be stable as well. Os is the daughter of Re (half-life 4.12×10 years) and is most often measured in an Os/Os ratio. This ratio, as well as the Re/Os ratio, have been used extensively in dating terrestrial as well as meteoric rocks. It has also been used to measure the intensity of continental weathering over geologic time and to fix minimum ages for stabilization of the mantle roots of continental cratons. However, the most notable application of Os in dating has been in conjunction with iridium, to analyze the layer of shocked quartz along the Cretaceous–Paleogene boundary that marks the extinction of the dinosaurs 66 million years ago. Isotopically pure Os, were it available, would be the densest stable material on earth at 22.80 grams per cubic centimeter.

There are also 31 artificial radioisotopes, the longest-lived of which is Os with a half-life of six years; all others have half-lives under 93 days. There are also ten known nuclear isomers, the longest-lived of which is Os with a half-life of 13.10 hours. All isotopes and nuclear isomers of osmium are either radioactive or observationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed.

Uses of osmium isotopes

The isotopic ratio of osmium-187 and osmium-188 (Os/Os) can be used as a window into geochemical changes throughout the ocean's history. The average marine Os/Os ratio in oceans is 1.06. This value represents a balance of the continental derived riverine inputs of Os with a Os/Os ratio of ~1.3, and the mantle/extraterrestrial inputs with a Os/Os ratio of ~0.13. Being a descendant of Re, Os can be radiogenically formed by beta decay. This decay has actually pushed the Os/Os ratio of the Bulk silicate earth (Earth minus the core) by 33%. This is what drives the difference in the Os/Os ratio we see between continental materials and mantle material. Crustal rocks have a much higher level of Re, which slowly degrades into Os driving up the ratio. Within the mantle however, the uneven response of Re and Os results in these mantle, and melted materials being depleted in Re, and do not allow for them to accumulate Os like the continental material. The input of both materials in the marine environment results in the observed Os/Os of the oceans and has fluctuated greatly over the history of our planet. These changes in the isotopic values of marine Os can be observed in the marine sediment that is deposited, and eventually lithified in that time period. This allows for researchers to make estimates on weathering fluxes, identifying flood basalt volcanism, and impact events that may have caused some of our largest mass extinctions. The marine sediment Os isotope record has been used to identify and corroborate the impact of the K-T boundary for example. The impact of this ~10 km asteroid massively altered the Os/Os signature of marine sediments at that time. With the average extraterrestrial Os/Os of ~0.13 and the huge amount of Os this impact contributed (equivalent to 600,000 years of present-day riverine inputs) lowered the global marine Os/Os value of ~0.45 to ~0.2.

Os isotope ratios may also be used as a signal of anthropogenic impact. The same Os/Os ratios that are common in geological settings may be used to gauge the addition of anthropogenic Os through things like catalytic converters. While catalytic converters have been shown to drastically reduce the emission of NOx and CO, they are introducing platinum group elements (PGE) such as Os, to the environment. Other sources of anthropogenic Os include combustion of fossil fuels, smelting chromium ore, and smelting of some sulfide ores. In one study, the effect of automobile exhaust on the marine Os system was evaluated. Automobile exhaust Os/Os has been recorded to be ~0.2 (similar to extraterrestrial and mantle derived inputs) which is heavily depleted (3, 7). The effect of anthropogenic Os can be seen best by comparing aquatic Os ratios and local sediments or deeper waters. Impacted surface waters tend to have depleted values compared to deep ocean and sediments beyond the limit of what is expected from cosmic inputs. This increase in effect is thought to be due to the introduction of anthropogenic airborne Os into precipitation.

The long half-life of Os with respect to alpha decay to W has been proposed as a radiometric dating method for osmium-rich rocks or for differentiation of a planetary core.

List of isotopes


Nuclide
Z N Isotopic mass (Da)
Half-life
Decay
mode

Daughter
isotope

Spin and
parity
Natural abundance (mole fraction)
Excitation energy Normal proportion Range of variation
Os 76 84 97+97
−32 μs
α W 0+
Os 1844(18) keV 41+15
−9 μs
α W 8+
Os 76 85 160.98905(43)# 0.64(6) ms α W (7/2–)
Os 76 86 161.98443(32)# 2.1(1) ms α W 0+
Os 76 87 162.98246(32)# 5.7(5) ms α W 7/2–
β ? Re
Os 76 88 163.97807(16) 21(1) ms α (96%) W 0+
β (4%) Re
Os 76 89 164.97665(22)# 71(3) ms α (90%) W (7/2–)
β (10%) Re
Os 76 90 165.972698(19) 213(5) ms α (83%) W 0+
β (17%) Re
Os 76 91 166.971552(87) 839(5) ms α (51%) W 7/2–
β (49%) Re
Os 434.3(11) keV 0.672(7) μs IT Os 13/2+
Os 76 92 167.967799(11) 2.1(1) s β (57%) Re 0+
α (43%) W
Os 76 93 168.967018(28) 3.46(11) s β (86.3%) Re (5/2–)
α (13.7%) W
Os 76 94 169.963579(10) 7.37(18) s β (90.5%) Re 0+
α (9.5%) W
Os 76 95 170.963180(20) 8.3(2) s β (98.20%) Re (5/2−)
α (1.80%) W
Os 76 96 171.960017(14) 19.2(9) s β (98.81%) Re 0+
α (1.19%) W
Os 76 97 172.959808(16) 22.4(9) s β (99.6%) Re 5/2–
α (0.4%) W
Os 76 98 173.957063(11) 44(4) s β (99.98%) Re 0+
α (.024%) W
Os 76 99 174.956945(13) 1.4(1) min β Re (5/2−)
Os 76 100 175.954770(12) 3.6(5) min β Re 0+
Os 76 101 176.954958(16) 3.0(2) min β Re 1/2−
Os 76 102 177.953253(15) 5.0(4) min β Re 0+
Os 76 103 178.953816(17) 6.5(3) min β Re 1/2–
Os 145.41(12) keV ~500 ns IT Os (7/2)–
Os 243.0(8) keV 783(14) ns IT Os (9/2)+
Os 76 104 179.952382(17) 21.5(4) min β Re 0+
Os 76 105 180.953247(27) 105(3) min β Re 1/2−
Os 49.20(14) keV 2.7(1) min β Re 7/2−
Os 156.91(15) keV 262(6) ns IT Os 9/2+
Os 76 106 181.952110(23) 21.84(20) h EC Re 0+
Os 1831.4(3) keV 780(70) μs IT Os 8–
Os 7049.5(4) keV 150(10) ns IT Os 25+
Os 76 107 182.953125(53) 13.0(5) h β Re 9/2+
Os 170.73(7) keV 9.9(3) h β (85%) Re 1/2−
IT (15%) Os
Os 76 108 183.95249292(89) 1.12(23)×10 y α W 0+ 2(2)×10
Os 76 109 184.95404597(89) 92.95(9) d EC Re 1/2−
Os 102.37(11) keV 3.0(4) μs IT Os 7/2−
Os 275.53(12) keV 0.78(5) μs IT Os 11/2+
Os 76 110 185.95383757(82) 2.0(11)×10 y α W 0+ 0.0159(64)
Os 76 111 186.95574957(79) Observationally Stable 1/2− 0.0196(17)
Os 100.45(4) keV 112(6) ns IT Os 7/2−
Os 257.10(7) keV 231(2) μs IT Os 11/2+
Os 76 112 187.95583729(79) Observationally Stable 0+ 0.1324(27)
Os 76 113 188.95814595(72) Observationally Stable 3/2− 0.1615(23)
Os 30.82(2) keV 5.81(10) h IT Os 9/2−
Os 76 114 189.95844544(70) Observationally Stable 0+ 0.2626(20)
Os 1705.7(1) keV 9.86(3) min IT Os 10−
Os 76 115 190.96092811(71) 14.99(2) d β Ir 9/2−
Os 74.382(3) keV 13.10(5) h IT Os 3/2−
Os 76 116 191.9614788(25) Observationally Stable 0+ 0.4078(32)
Os 2015.40(11) keV 5.94(9) s IT Os 10−
β? Ir
Os 4580.3(10) keV 205(7) ns IT Os (20+)
Os 76 117 192.9641496(25) 29.830(18) h β Ir 3/2−
Os 315.6(3) keV 121(28) ns IT Os (9/2−)
Os 76 118 193.9651794(26) 6.0(2) y β Ir 0+
Os 76 119 194.968318(60) 6.5(11) min β Ir (3/2−)
Os 427.8(3) keV 47(3) s IT Os (13/2+)
β? Ir
Os 76 120 195.969643(43) 34.9(2) min β Ir 0+
Os 76 121 196.97308(22)# 93(7) s β Ir 5/2−#
Os 76 122 197.97466(22)# 125(28) s β Ir 0+
Os 76 123 198.97824(22)# 6(3) s β Ir 5/2−#
Os 76 124 199.98009(32)# 7(4) s β Ir 0+
Os 76 125 200.98407(32)# 3# s β? Ir 1/2−#
Os 76 126 201.98655(43)# 2# s β? Ir 0+
Os 76 127 202.99220(43)# 300# ms β? Ir 9/2+#
β n? Ir
This table header & footer:
  1. Os – Excited nuclear isomer.
  2. ( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
  3. # – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
  4. Bold half-life – nearly stable, half-life longer than age of universe.
  5. Modes of decay:
    EC: Electron capture
    IT: Isomeric transition


    p: Proton emission
  6. Bold italics symbol as daughter – Daughter product is nearly stable.
  7. Bold symbol as daughter – Daughter product is stable.
  8. ( ) spin value – Indicates spin with weak assignment arguments.
  9. # – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  10. ^ primordial radionuclide
  11. Theorized to also undergo ββ decay to W
  12. ^ Used in rhenium-osmium dating
  13. Believed to undergo α decay to W with a half-life over 3.2×10 years
  14. Believed to undergo α decay to W with a half-life over 3.3×10 years
  15. Believed to undergo α decay to W with a half-life over 3.3×10 years
  16. Believed to undergo α decay to W with a half-life over 1.2×10 years
  17. Believed to undergo α decay to W or ββ decay to Pt with a half-life over 5.3×10 years

References

  1. ^ 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.
  2. ^ Peters, Stefan T.M.; Münker, Carsten; Becker, Harry; Schulz, Toni (April 2014). "Alpha-decay of Os revealed by radiogenic W in meteorites: Half life determination and viability as geochronometer". Earth and Planetary Science Letters. 391: 69–76. doi:10.1016/j.epsl.2014.01.030.
  3. "Standard Atomic Weights: Osmium". CIAAW. 1991.
  4. 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.
  5. Flegenheimer, Juan (2014). "The mystery of the disappearing isotope". Revista Virtual de Química. 6 (4): 1139–1142. doi:10.5935/1984-6835.20140073.
  6. ^ Peucker-Ehrenbrink, B.; Ravizza, G. (2000). "The marine osmium isotope record". Terra Nova. 12 (5): 205–219. Bibcode:2000TeNov..12..205P. doi:10.1046/j.1365-3121.2000.00295.x. S2CID 12486288.
  7. ^ Esser, Bradley K.; Turekian, Karl K. (1993). "The osmium isotopic composition of the continental crust". Geochimica et Cosmochimica Acta. 57 (13): 3093–3104. Bibcode:1993GeCoA..57.3093E. doi:10.1016/0016-7037(93)90296-9.
  8. Hauri, Erik H. (2002). "Osmium Isotopes and Mantle Convection" (PDF). Philosophical Transactions: Mathematical, Physical and Engineering Sciences. 360 (1800): 2371–2382. Bibcode:2002RSPTA.360.2371H. doi:10.1098/rsta.2002.1073. JSTOR 3558902. PMID 12460472. S2CID 18451805.
  9. Lowery, Christopher; Morgan, Joanna; Gulick, Sean; Bralower, Timothy; Christeson, Gail (2019). "Ocean Drilling Perspectives on Meteorite Impacts". Oceanography. 32: 120–134. doi:10.5670/oceanog.2019.133.
  10. Selby, D.; Creaser, R. A. (2005). "Direct Radiometric Dating of Hydrocarbon Deposits Using Rhenium-Osmium Isotopes". Science. 308 (5726): 1293–1295. Bibcode:2005Sci...308.1293S. doi:10.1126/science.1111081. PMID 15919988. S2CID 41419594.
  11. ^ Chen, C.; Sedwick, P. N.; Sharma, M. (2009). "Anthropogenic osmium in rain and snow reveals global-scale atmospheric contamination". Proceedings of the National Academy of Sciences. 106 (19): 7724–7728. Bibcode:2009PNAS..106.7724C. doi:10.1073/pnas.0811803106. PMC 2683094. PMID 19416862.
  12. Cook, David L.; Kruijer, Thomas S.; Leya, Ingo; Kleine, Thorsten (September 2014). "Cosmogenic W variations in meteorites and re-assessment of a possible Os–W decay system". Geochimica et Cosmochimica Acta. 140: 160–176. doi:10.1016/j.gca.2014.05.013.
  13. Cook, David L.; Smith, Thomas; Leya, Ingo; Hilton, Connor D.; Walker, Richard J.; Schönbächler, Maria (September 2018). "Excess W in IIAB iron meteorites: Identification of cosmogenic, radiogenic, and nucleosynthetic components". Earth Planet Sci Lett. 503: 29–36. doi:10.1016/j.epsl.2018.09.021. PMC 6398611.
  14. Wang, Meng; Huang, W.J.; Kondev, F.G.; Audi, G.; Naimi, S. (2021). "The AME 2020 atomic mass evaluation (II). Tables, graphs and references*". Chinese Physics C. 45 (3): 030003. doi:10.1088/1674-1137/abddaf.
  15. ^ Briscoe, A. D.; Page, R. D.; Uusitalo, J.; et al. (2023). "Decay spectroscopy at the two-proton drip line: Radioactivity of the new nuclides Os and W". Physics Letters B. 47 (138310). doi:10.1016/j.physletb.2023.138310. hdl:10272/23933.
Isotopes of the chemical elements
Group 1 2   3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
Period Hydrogen and
alkali metals
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