Abstract
Considerable evidence points to a martian origin of the SNC meteorites. Noble gas isotopic compositions have been measured in most SNC meteorites. The 129Xe/132Xe vs. 84Kr/132Xe ratios in Chassigny, most shergottites, and lithology C of EETA 79001 define a linear array. This array is thought to be mixing line between martian mantle and martian atmosphere. One of the SNC meteorites, Nakhla contains a leachable component that has an elevated 129Xe/132Xe ratio relative to its 84Kr/132Xe ratio when compared to this approximately linear array. The elevated Xe isotopic ratio may represent a distinct reservoir in the martian crust or mantle. More plausibly, it is elementally fractioned martian atmosphere. -from Authors
| Original language | English (US) |
|---|---|
| Pages (from-to) | 854-859 |
| Number of pages | 6 |
| Journal | Meteoritics |
| Volume | 29 |
| Issue number | 6 |
| DOIs | |
| State | Published - 1994 |
ASJC Scopus subject areas
- General Environmental Science
- General Earth and Planetary Sciences
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