Oxygen-isotopic evolution of the solar nebula

Studies of the three oxygen isotopes in chondrite meteorites demonstrate that diverse O reservoirs (characterized by their Δ17O values) were present in the solar nebula. The discovery that some chondritic materials have O‐isotopic compositions that cannot be explained by mass‐dependent fractionation...

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Veröffentlicht in:	Reviews of geophysics (1985) 2000-11, Vol.38 (4), p.491-512
1. Verfasser:	Wasson, John T.
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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