Oxygen isotopic evidence for vigorous mixing during the Moon-forming giant impact
Earth and the Moon are shown here to have indistinguishable oxygen isotope ratios, with a difference in Δ'¹⁷ O of −1 ± 5 parts per million (2 standard error). On the basis of these data and our new planet formation simulations that include a realistic model for primordial oxygen isotopic reserv...
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| Veröffentlicht in: | Science (American Association for the Advancement of Science) 2016-01, Vol.351 (6272), p.493-496 |
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| container_title | Science (American Association for the Advancement of Science) |
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| creator | Young, Edward D. Kohl, Issaku E. Warren, Paul H. Rubie, David C. Jacobson, Seth A. Morbidelli, Alessandro |
| description | Earth and the Moon are shown here to have indistinguishable oxygen isotope ratios, with a difference in Δ'¹⁷ O of −1 ± 5 parts per million (2 standard error). On the basis of these data and our new planet formation simulations that include a realistic model for primordial oxygen isotopic reservoirs, our results favor vigorous mixing during the giant impact and therefore a high-energy, high-angular-momentum impact. The results indicate that the late veneer impactors had an average Δ'¹⁷ O within approximately 1 per mil of the terrestrial value, limiting possible sources for this late addition of mass to the Earth-Moon system. |
| doi_str_mv | 10.1126/science.aad0525 |
| format | Article |
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| source | American Association for the Advancement of Science; Jstor Complete Legacy |
| subjects | Astronomy Earth Geophysics Isotopes Moon Oxygen |
| title | Oxygen isotopic evidence for vigorous mixing during the Moon-forming giant impact |
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