Computer Science
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994metic..29q.463e&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 29, no. 4, p. 463
Computer Science
5
Carbonaceous Chondrites, Chemical Analysis, Chronometers, Meteoritic Composition, Dolomite (Mineral), Electron Probes, Granular Materials, Precipitation (Chemistry)
Scientific paper
Carbonates and sulfates are common in CI chondrites and are believed to have resulted from aqueous alteration processes on the CI parent body. The carbonates occur mostly either as single grains or as polycrystalline chunks and are dominated by dolomites with varying Fe, Mg, and Mn contents. Calcites and breunnerites are less abundant. Since dolomites have MnO contents of up to 15 wt% and generally low Cr2O3 contents, we carried our exploratory SIMS analyses on dolomites in order to determine, whether a Mn-53-Cr-53 chronometer could provide constraints on the formation times of carbonates in CIs. We focused on carbonate fragments in Ivuna, since they can be easily recognized in thin sections, but also measured one carbonate from Orgueil. Our data indicate that aqueous alteration must have occurred soon after formation of the Ivuna parent body, perhaps even before accretion and accumulation was completed. Our results are similar to, but more stringent than, those obtained from Sr isotope data on carbonates in Orgueil, which imply that Ca-Mg carbonate precipitation was completed within 50 m.y. after formation of the Orgueil parent body. Further Mn-Cr studies, now underway, are disigned to determine whether or not carbonate fragments and carbonate grains in distinct lithic units of Ivuna, and different carbonate phases like dolomites and breunnerites precipitated at the same time.
Bischoff Addi
Endress Magnus
Weber Darrell
Zinner Emst
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