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Structural history of southeastern Mare Serenitatis and adjacent highlandsDeformational events are identified from Apollo 17 low-sun photographs of southern Mare Serenitatis and the adjacent Taurus-Littrow region. Analysis of the data indicates that the rate of deformation, including subsidence of the Serenitatis basin, has decreased through time as the crust increased in strength. Three main basalt sequences are found: one each at 3.8, 3.5, and 3.2 b.y. Wrinkle ridges began forming at about 2.5 b.y.; asymmetrical scarps also formed much later than the deformations.
Document ID
19750055476
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Muehlberger, W. R.
(Texas, University Austin, Tex.; U.S. Geological Survey, Center of Astrogeology, Flagstaff, Ariz., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 18, 1974
End Date: March 22, 1974
Accession Number
75A39548
Funding Number(s)
CONTRACT_GRANT: NASA ORDER T-5874-A
Distribution Limits
Public
Copyright
Other

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