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Grooved terrain on GanymedeIt is postulated that during a period in Ganymede's history when its lithosphere was thin, upwelling convection currents caused incipient rifting accompanied by intensive normal faulting. Where the rifting went to completion, crustal segments separated, spread apart locally, and sheared past one another. Subduction and compression may have occurred in places, but the evidence is inconclusive. The grooved terrain on Ganymede may therefore record an early phase of ice-plate tectonics that caused rifting and drifting of the icy lithosphere, but which, unlike silicate plate tectonics on earth, may have resulted in only minor vertical turnover. It is concluded that grooved terrain grew at the expense of cratered terrain, that cratered tracts were converted into grooved terrain in situ, and that vertical tectonism and shear movements dominated in the restructuring of Ganymede's surface.
Document ID
19810048219
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lucchitta, B. K.
(U.S. Geological Survey Flagstaff, Ariz., United States)
Date Acquired
August 11, 2013
Publication Date
November 1, 1980
Subject Category
Lunar And Planetary Exploration
Accession Number
81A32623
Funding Number(s)
CONTRACT_GRANT: NASA ORDER W-13709
Distribution Limits
Public
Copyright
Other

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