Variations in the Ar/Kr/Xe ratios of martian atmosphere trapped in martian meteorites correlate with the time of ejection of these meteorites from Mars. We suggest that these variations reflect actual differences in the Ar/Kr/Xe ratios of the martian atmosphere at the time of ejection of the meteori
✦ LIBER ✦
Release of Kr, Ag, Sn, I and Xe from UCx targets
✍ Scribed by B. Roussière; O. Bajeat; N. Barré; C. Bourgeois; F. Clapier; E. Cottereau; C. Donzaud; M. Ducourtieux; S. Essabaa; D. Guillemaud-Mueller; F. Ibrahim; C. Lau; F. Le Blanc; H. Lefort; C.F. Liang; A.C. Mueller; J. Obert; N. Pauwels; J.C. Potier; F. Pougheon; J. Proust; J. Sauvage; O. Sorlin; D. Verney; A. Wojtasiewicz
- Publisher
- Elsevier Science
- Year
- 2006
- Tongue
- English
- Weight
- 599 KB
- Volume
- 246
- Category
- Article
- ISSN
- 0168-583X
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