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Phobos and deimos: Analysis of surface features, ejecta dynamics and a volatile loss mechanismThe question of whether the crater population on Phobos represents a production population or an equilibrium population is considered. The absolute ages of cratered surfaces are interpreted and analyzed. A computer program was developed to study the dynamics of material ejected from Martian satellites and to investigate the hypothesis that at least some of the extensive set of linear features discovered on the surface of Phobos could be the result of secondary cratering from the Stickney impact. The possibility that Deimos was catastrophically disrupted by a large impact but subsequently reaccreted is considered as well as the probability the Phobos had an impact nearly large enough to disrupt it are also discussed.
Document ID
19800014750
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Davis, D. R.
(Planetary Science Inst. Tucson, AZ, United States)
Chapman, C. R.
(Planetary Science Inst. Tucson, AZ, United States)
Greenberg, R.
(Planetary Science Inst. Tucson, AZ, United States)
Weidenschilling, S. J.
(Planetary Science Inst. Tucson, AZ, United States)
Date Acquired
September 4, 2013
Publication Date
March 1, 1980
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
NASA-CR-163005
Accession Number
80N23239
Funding Number(s)
CONTRACT_GRANT: NASW-3272
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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