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The Taurus-Littrow dark mantle, light mantle, crater cluster, and scarpThe Taurus-Littrow landing site is on the floor of a grabenlike valley that is radial to the Serenitatis Basin; the valley is gently inclined to the east. It is bordered by steep-sided massifs that rise 2 km above the valley floor and form part of the Serenitatis Basin rim. The valley floor is exceptionally dark, and in one place it is overlain by a light-colored mantle apparently derived from the massif to the south. The floor is also peppered by overlapping craters. A scarp, up on the west, transects the valley floor and enters the highlands to the north. Pre- and post-mission analyses of this geological formation are presented.
Document ID
19930009612
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Lucchitta, Baerbel K.
(Geological Survey Flagstaff, AZ, United States)
Date Acquired
September 6, 2013
Publication Date
December 2, 1992
Publication Information
Publication: Lunar Science Inst., Workshop on Geology of the Apollo 17 Landing Site
Subject Category
Lunar And Planetary Exploration
Accession Number
93N18801
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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