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Variable features on Mars. II - Mariner 9 global results.Systematic Mariner 9 monitoring of the space and time distribution of Martian bright and dark markings, the streaks and splotches, indicates a range of global correlations. The time-variable classical dark markings owe their configurations and variability to their constituent streaks and splotches, produced by windblown dust. Streaks and splotches are consistent wind direction indicators. Correlation of global streak patterns with general circulation models shows that velocities of about 50 to 90 m/sec above the boundary layer are necessary to initiate grain motion on the surface and to produce streaks and splotches. Detailed examples of changes in Syrtis Major, Lunae Palus, and Promethei Sinus are generally consistent with removal of bright sand and dust and uncovering of darker underlying material as the active agent in such changes, although dark mobile material probably also exists on Mars. The generation of streaks and the progressive albedo changes observed require only threshold velocities of about 2 m/sec for about 1 day at the grain surface.
Document ID
19730052410
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sagan, C.
Veverka, J.
Fox, P.
Dubisch, F.
French, R.
Gierasch, P.
(Cornell University Ithaca, N.Y., United States)
Quam, L.
Lederberg, J.
Levinthal, E.
(Stanford University Stanford, Calif., United States)
Pollack, J. B.
(NASA Ames Research Center Moffett Field, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
July 10, 1973
Publication Information
Publication: Journal of Geophysical Research
Volume: 78
Subject Category
Space Sciences
Accession Number
73A37212
Distribution Limits
Public
Copyright
Other

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