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Standard atomic weightAr°(Os) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Osmium (76Os) has seven naturally occurringisotopes, five of which are stable:187Os,188Os,189Os,190Os, and (most abundant)192Os. The other natural isotopes,184Os, and186Os, have extremely longhalf-life (1.12×1013 years and 2×1015 years, respectively) and for practical purposes can be considered to be stable as well.187Os is the daughter of187Re (half-life 4.12×1010 years) and is most often measured in an187Os/188Os ratio. This ratio, as well as the187Re/188Os ratio, have been used extensively in dating terrestrial as well asmeteoricrocks. It has also been used to measure the intensity of continental weathering over geologic time and to fix minimum ages for stabilization of themantle roots of continentalcratons. However, the most notable application of Os in dating has been in conjunction withiridium, to analyze the layer ofshocked quartz along theCretaceous–Paleogene boundary that marks the extinction of thedinosaurs 66 million years ago. Isotopically pure192Os, were it available, would be the densest stable material on earth at 22.80 grams per cubic centimeter.
There are also 31 artificialradioisotopes,[5] the longest-lived of which is194Os with a half-life of six years; all others have half-lives under 93 days. There are also ten knownnuclear isomers, the longest-lived of which is191mOs with a half-life of 13.10 hours. All isotopes and nuclear isomers of osmium are either radioactive orobservationally stable, meaning that they are predicted to be radioactive but no actual decay has been observed.
The isotopic ratio of osmium-187 and osmium-188 (187Os/188Os) can be used as a window into geochemical changes throughout the ocean's history.[6] The average marine187Os/188Os ratio in oceans is 1.06.[6] This value represents a balance of the continental derived riverine inputs of Os with a187Os/188Os ratio of ~1.3, and themantle/extraterrestrial inputs with a187Os/188Os ratio of ~0.13.[6] Being a descendant of187Re,187Os can beradiogenically formed by beta decay.[7] This decay has actually pushed the187Os/188Os ratio of the Bulk silicate earth (Earth minus thecore) by 33%.[8] This is what drives the difference in the187Os/188Os ratio we see between continental materials and mantle material.Crustal rocks have a much higher level of Re, which slowly degrades into187Os driving up the ratio.[7] 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 accumulate187Os like the continental material.[7] The input of both materials in the marine environment results in the observed187Os/188Os 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 themarine sediment that is deposited, and eventuallylithified in that time period.[9] 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.[10] The impact of this ~10 km asteroid massively altered the187Os/188Os signature of marine sediments at that time. With the average extraterrestrial187Os/188Os 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 marine187Os/188Os value of ~0.45 to ~0.2.[6]
Os isotope ratios may also be used as a signal of anthropogenic impact.[11] The same187Os/188Os ratios that are common in geological settings may be used to gauge the addition of anthropogenic Os through things likecatalytic converters.[11] While catalytic converters have been shown to drastically reduce the emission of NOx and CO, they are introducingplatinum group elements (PGE) such as Os, to the environment.[11] Other sources of anthropogenic Os include combustion offossil fuels, smeltingchromium ore, and smelting of somesulfide ores. In one study, the effect of automobile exhaust on the marine Os system was evaluated. Automobile exhaust187Os/188Os 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.[11] This increase in effect is thought to be due to the introduction of anthropogenic airborne Os into precipitation.
The long half-life of184Os with respect to alpha decay to180W has been proposed as aradiometric dating method for osmium-rich rocks or fordifferentiation of a planetary core.[2][12][13]
Nuclide [n 1] | Z | N | Isotopic mass(Da)[14] [n 2][n 3] | Half-life[1] [n 4] | Decay mode[1] [n 5] | Daughter isotope [n 6][n 7] | Spin and parity[1] [n 8][n 9] | Natural abundance(mole fraction) | |||||||||||
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Excitation energy | Normal proportion[1] | Range of variation | |||||||||||||||||
160Os[15] | 76 | 84 | 97+97 −32 μs | α | 156W | 0+ | |||||||||||||
160mOs[15] | 1844(18) keV | 41+15 −9 μs | α | 156W | 8+ | ||||||||||||||
161Os | 76 | 85 | 160.98905(43)# | 0.64(6) ms | α | 157W | (7/2–) | ||||||||||||
162Os | 76 | 86 | 161.98443(32)# | 2.1(1) ms | α | 158W | 0+ | ||||||||||||
163Os | 76 | 87 | 162.98246(32)# | 5.7(5) ms | α | 159W | 7/2– | ||||||||||||
β+ ? | 163Re | ||||||||||||||||||
164Os | 76 | 88 | 163.97807(16) | 21(1) ms | α (96%) | 160W | 0+ | ||||||||||||
β+ (4%) | 164Re | ||||||||||||||||||
165Os | 76 | 89 | 164.97665(22)# | 71(3) ms | α (90%) | 161W | (7/2–) | ||||||||||||
β+ (10%) | 165Re | ||||||||||||||||||
166Os | 76 | 90 | 165.972698(19) | 213(5) ms | α (83%) | 162W | 0+ | ||||||||||||
β+ (17%) | 166Re | ||||||||||||||||||
167Os | 76 | 91 | 166.971552(87) | 839(5) ms | α (51%) | 163W | 7/2– | ||||||||||||
β+ (49%) | 167Re | ||||||||||||||||||
167mOs | 434.3(11) keV | 0.672(7) μs | IT | 167Os | 13/2+ | ||||||||||||||
168Os | 76 | 92 | 167.967799(11) | 2.1(1) s | β+ (57%) | 168Re | 0+ | ||||||||||||
α (43%) | 164W | ||||||||||||||||||
169Os | 76 | 93 | 168.967018(28) | 3.46(11) s | β+ (86.3%) | 169Re | (5/2–) | ||||||||||||
α (13.7%) | 165W | ||||||||||||||||||
170Os | 76 | 94 | 169.963579(10) | 7.37(18) s | β+ (90.5%) | 170Re | 0+ | ||||||||||||
α (9.5%) | 166W | ||||||||||||||||||
171Os | 76 | 95 | 170.963180(20) | 8.3(2) s | β+ (98.20%) | 171Re | (5/2−) | ||||||||||||
α (1.80%) | 167W | ||||||||||||||||||
172Os | 76 | 96 | 171.960017(14) | 19.2(9) s | β+ (98.81%) | 172Re | 0+ | ||||||||||||
α (1.19%) | 168W | ||||||||||||||||||
173Os | 76 | 97 | 172.959808(16) | 22.4(9) s | β+ (99.6%) | 173Re | 5/2– | ||||||||||||
α (0.4%) | 169W | ||||||||||||||||||
174Os | 76 | 98 | 173.957063(11) | 44(4) s | β+ (99.98%) | 174Re | 0+ | ||||||||||||
α (.024%) | 170W | ||||||||||||||||||
175Os | 76 | 99 | 174.956945(13) | 1.4(1) min | β+ | 175Re | (5/2−) | ||||||||||||
176Os | 76 | 100 | 175.954770(12) | 3.6(5) min | β+ | 176Re | 0+ | ||||||||||||
177Os | 76 | 101 | 176.954958(16) | 3.0(2) min | β+ | 177Re | 1/2− | ||||||||||||
178Os | 76 | 102 | 177.953253(15) | 5.0(4) min | β+ | 178Re | 0+ | ||||||||||||
179Os | 76 | 103 | 178.953816(17) | 6.5(3) min | β+ | 179Re | 1/2– | ||||||||||||
179m1Os | 145.41(12) keV | ~500 ns | IT | 179Os | (7/2)– | ||||||||||||||
179m2Os | 243.0(8) keV | 783(14) ns | IT | 179Os | (9/2)+ | ||||||||||||||
180Os | 76 | 104 | 179.952382(17) | 21.5(4) min | β+ | 180Re | 0+ | ||||||||||||
181Os | 76 | 105 | 180.953247(27) | 105(3) min | β+ | 181Re | 1/2− | ||||||||||||
181m1Os | 49.20(14) keV | 2.7(1) min | β+ | 181Re | 7/2− | ||||||||||||||
181m2Os | 156.91(15) keV | 262(6) ns | IT | 181Os | 9/2+ | ||||||||||||||
182Os | 76 | 106 | 181.952110(23) | 21.84(20) h | EC | 182Re | 0+ | ||||||||||||
182m1Os | 1831.4(3) keV | 780(70) μs | IT | 182Os | 8– | ||||||||||||||
182m2Os | 7049.5(4) keV | 150(10) ns | IT | 182Os | 25+ | ||||||||||||||
183Os | 76 | 107 | 182.953125(53) | 13.0(5) h | β+ | 183Re | 9/2+ | ||||||||||||
183mOs | 170.73(7) keV | 9.9(3) h | β+ (85%) | 183Re | 1/2− | ||||||||||||||
IT (15%) | 183Os | ||||||||||||||||||
184Os[n 10] | 76 | 108 | 183.95249292(89) | 1.12(23)×1013 y | α[n 11] | 180W | 0+ | 2(2)×10−4 | |||||||||||
185Os | 76 | 109 | 184.95404597(89) | 92.95(9) d | EC | 185Re | 1/2− | ||||||||||||
185m1Os | 102.37(11) keV | 3.0(4) μs | IT | 185Os | 7/2− | ||||||||||||||
185m2Os | 275.53(12) keV | 0.78(5) μs | IT | 185Os | 11/2+ | ||||||||||||||
186Os[n 10] | 76 | 110 | 185.95383757(82) | 2.0(11)×1015 y | α | 182W | 0+ | 0.0159(64) | |||||||||||
187Os[n 12] | 76 | 111 | 186.95574957(79) | Observationally Stable[n 13] | 1/2− | 0.0196(17) | |||||||||||||
187m1Os | 100.45(4) keV | 112(6) ns | IT | 187Os | 7/2− | ||||||||||||||
187m2Os | 257.10(7) keV | 231(2) μs | IT | 187Os | 11/2+ | ||||||||||||||
188Os[n 12] | 76 | 112 | 187.95583729(79) | Observationally Stable[n 14] | 0+ | 0.1324(27) | |||||||||||||
189Os | 76 | 113 | 188.95814595(72) | Observationally Stable[n 15] | 3/2− | 0.1615(23) | |||||||||||||
189mOs | 30.82(2) keV | 5.81(10) h | IT | 189Os | 9/2− | ||||||||||||||
190Os | 76 | 114 | 189.95844544(70) | Observationally Stable[n 16] | 0+ | 0.2626(20) | |||||||||||||
190mOs | 1705.7(1) keV | 9.86(3) min | IT | 190Os | 10− | ||||||||||||||
191Os | 76 | 115 | 190.96092811(71) | 14.99(2) d | β− | 191Ir | 9/2− | ||||||||||||
191mOs | 74.382(3) keV | 13.10(5) h | IT | 191Os | 3/2− | ||||||||||||||
192Os | 76 | 116 | 191.9614788(25) | Observationally Stable[n 17] | 0+ | 0.4078(32) | |||||||||||||
192m1Os | 2015.40(11) keV | 5.94(9) s | IT | 192Os | 10− | ||||||||||||||
β−? | 192Ir | ||||||||||||||||||
192m2Os | 4580.3(10) keV | 205(7) ns | IT | 192Os | (20+) | ||||||||||||||
193Os | 76 | 117 | 192.9641496(25) | 29.830(18) h | β− | 193Ir | 3/2− | ||||||||||||
193mOs | 315.6(3) keV | 121(28) ns | IT | 193Os | (9/2−) | ||||||||||||||
194Os | 76 | 118 | 193.9651794(26) | 6.0(2) y | β− | 194Ir | 0+ | ||||||||||||
195Os | 76 | 119 | 194.968318(60) | 6.5(11) min | β− | 195Ir | (3/2−) | ||||||||||||
195mOs | 427.8(3) keV | 47(3) s | IT | 195Os | (13/2+) | ||||||||||||||
β−? | 195Ir | ||||||||||||||||||
196Os | 76 | 120 | 195.969643(43) | 34.9(2) min | β− | 196Ir | 0+ | ||||||||||||
197Os | 76 | 121 | 196.97308(22)# | 93(7) s | β− | 197Ir | 5/2−# | ||||||||||||
198Os | 76 | 122 | 197.97466(22)# | 125(28) s | β− | 198Ir | 0+ | ||||||||||||
199Os | 76 | 123 | 198.97824(22)# | 6(3) s | β− | 199Ir | 5/2−# | ||||||||||||
200Os | 76 | 124 | 199.98009(32)# | 7(4) s | β− | 200Ir | 0+ | ||||||||||||
201Os | 76 | 125 | 200.98407(32)# | 3# s [>300ns] | β−? | 201Ir | 1/2−# | ||||||||||||
202Os | 76 | 126 | 201.98655(43)# | 2# s [>300ns] | β−? | 202Ir | 0+ | ||||||||||||
203Os | 76 | 127 | 202.99220(43)# | 300# ms [>300ns] | β−? | 203Ir | 9/2+# | ||||||||||||
β− n? | 202Ir | ||||||||||||||||||
This table header & footer: |
EC: | Electron capture |
IT: | Isomeric transition |
p: | Proton emission |
Daughter products other than osmium