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- W2079652832 abstract "The times at which phyllosilicate matrix and euhedral olivines became associated have been determined for five C2 meteorites. The ages, calculated from fission track densities on crystal surfaces, are based on an initial244Pu/238U ratio in the matrix material of 0.0154 at 4.6 b.y., and range from 4.22 b.y. for Nogoya to 4.42 b.y. for Murray. Unless the initial244Pu/238U ratio was less than 0.004, the meteorites cannot have existed in their present form for 4.6 × 109 yr. The measured ages place limits on the time when pre-compaction effects such as micrometeorite craters and solar flare tracks were produced, and they may approximately date the formation of the olivine crystals themselves." @default.
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- W2079652832 date "1976-11-01" @default.
- W2079652832 modified "2023-09-28" @default.
- W2079652832 title "Formation chronology for C2 meteorites" @default.
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- W2079652832 doi "https://doi.org/10.1016/0012-821x(76)90155-2" @default.
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