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Results from the Magellan mission to VenusMagellan's radar-mapping mission to Venus has thus far accomplished the mapping of nearly 95 percent of the planet's surface; the 100-m resolution of these data facilitate studies of Venus' geological evolution. Widespread evidence of horizontal compression and extension at many scales is noted. Crustal deformation appears to be distributed across most of the surface. The density distribution of the interior of Venus will be explored in an upcomimg gravity experiment, in which accurate tracking of spacecraft orbital accelerations is used to identify gravity anomalies.
Document ID
19930028683
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Plaut, Jeffrey J.
(JPL Pasadena, CA, United States)
Date Acquired
August 15, 2013
Publication Date
January 14, 1992
Publication Information
Publication: EOS
Volume: 73
Issue: 2
ISSN: 0096-3941
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0096-3941
Accession Number
93A12680
Distribution Limits
Public
Copyright
Other

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