OXYGEN ISOTOPIC HOMOGENEITY OF THE EARTH: NEW EVIDENCE

dc.contributor.authorRobert F.
dc.contributor.authorRejou-Michel A.
dc.contributor.authorJavoy M.
dc.date.accessioned2020-11-09T02:14:15Z
dc.date.available2020-11-09T02:14:15Z
dc.date.issued1992
dc.description.abstractThe two oxygen isotope ratios18O/16O and17O/16O were analyzed in Precambrian (3.5 Gy) and modern cherts and in mantle-derived lavas. All samples exhibit oxygen isotopic compositions consistent with mass-dependent isotopic fractionation from a single reservoir and thus suggest that 3.5 Gy ago the Earth was already a well-mixed body. These results would therefore not support models of ocean accretion by cometary impact later than 3.7 ± 0.1 Gy. New measurements on lunar rocks confirm oxygen isotopic homogeneity of the Earth-Moon system and thus suggests that the internal mixing of the two bodies pre-dates their accretion. The recent giant impact model used to explain how the Moon was formed is also compatible with our results.
dc.identifierhttps://elibrary.ru/item.asp?id=31564690
dc.identifier.citationEarth and Planetary Science Letters, 1992, , 1, 1-9
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/18696
dc.subjectPrecambrianen
dc.subject.agePrecambrianen
dc.titleOXYGEN ISOTOPIC HOMOGENEITY OF THE EARTH: NEW EVIDENCE
dc.typeСтатья

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