Isotopic signatures of volatiles in terrestrial planets - Working group report

被引：17
作者：
Becker, RH
Clayton, RN
Galimov, EM
Lammer, H
Marty, B
Pepin, RO
Wieler, R
机构：
[1] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[2] Univ Chicago, Dept Geophys Sci, Chicago, IL 60637 USA
[3] Russian Acad Sci, VI Vernadsky Inst Geochem & Analyt Chem, Moscow 117975 19, Russia
[4] Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria
[5] Ctr Rech Petrog & Geochim, CNRS, UPR 9046, F-54501 Vandoeuvre Les Nancy, France
[6] ETH, CH-8092 Zurich, Switzerland
来源：
SPACE SCIENCE REVIEWS | 2003年 / 106卷 / 1-4期
关键词：
D O I：
10.1023/A:1024610325914
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Variations in the isotopic ratios of volatile elements in different reservoirs on the terrestrial planets carry information about processes that operated on the planets since their formation. Comparisons between primordial planetary compositions, to the extent they can be determined, may help us understand the planetary formation process. This working group report summarizes our knowledge of terrestrial planet volatile inventories.
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收藏
页码：377 / 410
页数：34
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