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Generating an AtmosphereThe presence of water ice on most of the large satellites of the outer planets was established many years ago through near-infrared observations with ground-based telescopes. Frozen carbon dioxide, sulfur dioxide, methane, nitrogen, and other molecular ices are also found in various combinations on inner planets such as Mars to bodies far beyond Pluto. Recent discoveries of ice varieties on some asteroids and sequestered in protected regions on Mercury and the Moon point to the near-universal distribution of frozen volatiles throughout the solar system.
Document ID
20110016538
Acquisition Source
Ames Research Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cruikshank, Dale P.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 25, 2013
Publication Date
December 24, 2010
Publication Information
Publication: Science
Publisher: American Association for the Advancement of Science
ISSN: 1095-9203
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ARC-E-DAA-TN4053
ISSN: 1095-9203
Report Number: ARC-E-DAA-TN4053
Funding Number(s)
WBS: WBS 431924.02.01.01
Distribution Limits
Public
Copyright
Public Use Permitted.
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