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Mars radar observations - A preliminary report.Radar observations of a narrow belt of the surface of Mars, centered at 16 deg south latitude, show a very rugged terrain, with elevation differences greater than 13 kilometers from peak to valley. For nearby points, the relative altitude is measured to 40 meters at best; the precision is worse for points at different latitudes, or widely separated in longitude, because of orbital uncertainties. Some of the larger craters have been resolved, and their depth and, in some cases, the height of the raised rim have been measured. Where high resolution photographs are available, the correlation is excellent.
Document ID
19720031694
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Downs, G. S.
Goldstein, R. M.
Green, R. R.
Morris, G. A.
(California Institute of Technology, Jet Propulsion Laboratory,Pasadena Calif., United States)
Date Acquired
August 6, 2013
Publication Date
December 24, 1971
Publication Information
Publication: Science
Volume: 174
Subject Category
Space Sciences
Accession Number
72A15360
Distribution Limits
Public
Copyright
Other

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