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Lunar global figure from mare surface elevationsLaser altimetry data from the Apollo 15, 16, and 17 missions show that the ringed maria surfaces lie on one particular reference surface and that the center of gravity is definitely displaced from the optical center. If these extensive surfaces are assumed to be near-hydrostatic surfaces, then there must have existed a time in lunar history when lunar tides, internal processes, or both were much different than they are today.
Document ID
19760045320
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Sjogren, W. L.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Wollenhaupt, W. R.
(NASA Johnson Space Center Houston, Tex., United States)
Date Acquired
August 8, 2013
Publication Date
February 1, 1976
Publication Information
Publication: The Moon
Volume: 15
Subject Category
Lunar And Planetary Exploration
Accession Number
76A28286
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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