期刊
METEORITICS & PLANETARY SCIENCE
卷 50, 期 4, 页码 810-833出版社
WILEY
DOI: 10.1111/maps.12410
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资金
- NASA Astrobiology grant [NNA09DA81A]
- NASA Cosmochemistry grant [NNX11AG67G, NNX11AG27G]
- NSF
- NASA
We report the bulk C abundances, and C and O isotopic compositions of carbonates in 64 CM chondrites, 14 CR chondrites, 2 CI chondrites, LEW 85332 (C2), Kaba (CV3), and Semarkona (LL3.0). For the unheated CMs, the total ranges of carbonate isotopic compositions are C-13 approximate to 25-75 parts per thousand and O-18 approximate to 15-35 parts per thousand, and bulk carbonate C contents range from 0.03 to 0.60wt%. There is no simple correlation between carbonate abundance and isotopic composition, or between either of these parameters and the extent of alteration. Unless accretion was very heterogeneous, the uncorrelated variations in extent of alteration and carbonate abundance suggests that there was a period of open system behavior in the CM parent body, probably prior to or at the start of aqueous alteration. Most of the ranges in CM carbonate isotopic compositions can be explained by their formation at different temperatures (0-130 degrees C) from a single fluid in which the carbonate O isotopes were controlled by equilibrium with water (O-18 approximate to 5 parts per thousand)
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