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Pluto's structure and composition suggest origin in the solar, not a planetary, nebulaThe four explanations for Pluto's large rock/ice ratio, (1) formation in the inner solar system, (2) volatile loss during accretion, (3) volatile loss during the large-body impact that created Charon, and (4) formation as a large, ice-poor outer solar system planetesimal, are considered. It is shown that only the last two explanations are feasible, and that the depletion of water ice in Pluto is so severe that both explanations may be necessary.
Document ID
19890036066
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mckinnon, William B.
(Washington University Saint Louis, MO, United States)
Mueller, Steve
(Southern Methodist University Dallas, TX, United States)
Date Acquired
August 14, 2013
Publication Date
September 15, 1988
Publication Information
Publication: Nature
Volume: 335
ISSN: 0028-0836
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0028-0836
Accession Number
89A23437
Distribution Limits
Public
Copyright
Other

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