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Galilean Satellite Surface Non-Ice Constituents: New Results from the Cassini/Huygens VIMS Jupiter Flyby in the Context of the Galileo NIMS ResultsThe Cassini mission Visible and Infrared Mapping Spectrometer (VIMS) is currently returning data for the Galilean satellites. Examples of the new satellite data and the initial interpretations will be presented in the context of the Galileo NIMS data and results. Additional information is contained in the original extended abstract.
Document ID
20010044420
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
McCord, T. B. (Hawaii Univ. Honolulu, HI United States)
Brown, R. (Arizona Univ. Tucson, AZ United States)
Baines, K. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Bellucci, G. (Consiglio Nazionale delle Ricerche Italy)
Bibring, J.-P. (Institut d'Astrophysique Paris, France)
Buratti, B. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Capaccioni, F. (Consiglio Nazionale delle Ricerche Italy)
Cerroni, P. (Consiglio Nazionale delle Ricerche Italy)
Clark, R. (Geological Survey Denver, CO United States)
Coradini, A. (Consiglio Nazionale delle Ricerche Italy)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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