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Mare Serenitatis - A preliminary definition of surface units by remote observationsMare Serenitatis is a ringed mare about 600 km in diameter situated in the northeast quadrant of the moon. The floor of the mare is comprised of several units. Remote observations of Mare Serenitatis are presented. Color difference photographs were produced by photographing the moon at two wavelength bands. Radar images were obtained by delay-Doppler mapping of radar echoes. The definition of surface units is discussed together with surface properties obtained from remote observations.
Document ID
19740042890
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Thompson, T. W. (California Institute of Technology, Jet Propulsion Laboratory, Space Sciences Div., Pasadena Calif., United States)
Shorthill, R. W. (Boeing Aerospace Co. Seattle, Wash., United States)
Whitaker, E. A. (Arizona, University Tucson, Ariz., United States)
Zisk, S. H. (Haystack Observatory Westford, Mass., United States)
Date Acquired
August 7, 2013
Publication Date
February 1, 1974
Subject Category
Space Sciences
Accession Number
74A25640
Funding Number(s)
CONTRACT_GRANT: NAS9-7830
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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