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Remote sensing of Mare SerenitatisAn examination was made of earth based observations of optical color differences, infrared eclipse temperatures, and radar backscatter for Mare Serenitatis. Information is also included on orbital observations, physical properties of surface types, and correlation of surface types with geologic units. Differences in these remote observations are attributed to variations in chemical and minerological compositions.
Document ID
Acquisition Source
Legacy CDMS
Document Type
Thompson, T. W.
(JPL Washington, DC, United States)
Howard, K. A.
(Geological Survey Washington, DC, United States)
Shorthill, R. W.
(Boeing Aerospace Co. Washington, DC, United States)
Tyler, G. L.
(Stanford Univ.)
Zisk, S. H.
Whitaker, E. A.
(Arizona Univ.)
Schaber, G. G.
(Geological Survey)
Moore, H. J.
(Geological Survey)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.
Subject Category
Space Sciences
Accession Number
Distribution Limits
Work of the US Gov. Public Use Permitted.
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