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Comets, meteorites and atmospheresThe relatively low value of Xe/Kr in the atmospheres of Earth and Mars seems to rule out meteorites as the major carriers of noble gases to the inner planets. Laboratory experiments on the trapping of gases in ice forming at low temperatures suggest that comets may be a better choice. It is then possible to develop a model for the origin of inner planet atmospheres based on volatiles delivered by comets added to volatiles originally trapped in planetary rocks. The model will be tested by results from the Galileo Entry Probe.
Document ID
20040089698
Acquisition Source
Headquarters
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Owen, T.
(Institute for Astronomy, University of Hawaii Honolulu 96822, United States)
Bar-Nun, A.
Date Acquired
August 21, 2013
Publication Date
January 1, 1996
Publication Information
Publication: Earth, moon, and planets
Volume: 72
ISSN: 0167-9295
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ISSN: 0167-9295
Funding Number(s)
CONTRACT_GRANT: NAGW-2650
CONTRACT_GRANT: NAGW-2631
Distribution Limits
Public
Copyright
Other
Keywords
NASA Discipline Exobiology
Non-NASA Center
Earth (Planet)
Noble Gases/analysis
Xenon
Meteoroids
Atmosphere/analysis
Krypton
Support, U.S. Gov't, Non-P.H.S
Neon
Extraterrestrial Environment
Mars
Venus
Argon

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