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Chapter 2.6: Physical Chemistry and Thermal Evolution of Ices at GanymedeGanymede’s surface is composed mostly of water ice and other icy materials in addition to minor non-ice components. The formation and evolution of Ganymede’s landforms highly depend on the nature of the icy materials as they present various thermal and rheological behaviors. This chapter reviews the currently known thermodynamic parameters of the ice phases and hydrates reported on Ganymede, which seem to affect the evolution of the surface, using mainly results from the Voyager and Galileo missions
Document ID
20210014758
Acquisition Source
Goddard Space Flight Center
Document Type
Contribution to a larger work
Authors
C Ahrens
(Universities Space Research Association Columbia, Maryland, United States)
A Solomonidou
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
K Stephan
(German Aerospace Center Cologne, Germany)
K Kalousova
(Charles University Prague, Czechia)
N Ligier
(University of Paris-Saclay Gif-sur-Yvette, France)
T McCord
(Bear Fight Institute Omak, Washington, United States)
C Hibbitts
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
Date Acquired
April 28, 2021
Publication Date
January 1, 2022
Publication Information
Publication: Ganymede
Publisher: Cambridge University Press
Subject Category
Physics (General)
Lunar And Planetary Science And Exploration
Funding Number(s)
CONTRACT_GRANT: NNH15CO48B
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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