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Science 1 October 1999: Vol. 286. no. 5437, pp. 94 - 97 DOI: 10.1126/science.286.5437.94
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Reports
The Gravity Field of Mars: Results from Mars Global Surveyor
David E. Smith,
1*
William L. Sjogren,
2
G. Leonard Tyler,
3
Georges Balmino,
4
Frank G. Lemoine,
1
Alex S. Konopliv
2
Observations of the gravity field of Mars reveal a
planet that has responded differently in its northern and southern
hemispheres to major impacts and volcanic processes. The rough,
elevated southern hemisphere has a relatively featureless gravitational
signature indicating a state of near-isostatic compensation, whereas
the smooth, low northern plains display a wider range of gravitational anomalies that indicates a thinner but stronger surface layer than in
the south. The northern hemisphere shows evidence for buried impact
basins, although none large enough to explain the hemispheric elevation
difference. The gravitational potential signature of Tharsis is
approximately axisymmetric and contains the Tharsis Montes but not the
Olympus Mons or Alba Patera volcanoes. The gravity signature of Valles
Marineris extends into Chryse and provides an estimate of material
removed by early fluvial activity.
1 Laboratory for Terrestrial Physics, National
Aeronautics and Space Administration (NASA) Goddard Space Flight
Center, Greenbelt, MD 20771, USA.
2 Jet Propulsion
Laboratory, Pasadena, CA 91109, USA.
3 Center for Radio
Astronomy, Stanford University, Stanford, CA 94035-4055, USA.
4 Group de Recherches de Geodesie Spatiales,
Toulouse, France.
*
To whom correspondence should be addressed:
dsmith{at}tharsis.gsfc.nasa.gov
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THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
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- P. Martin and E. R. Stofan (2007)
Geosphere
3, 435-455
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- Internal Structure and Early Thermal Evolution of Mars from Mars Global Surveyor Topography and Gravity.
- M. T. Zuber, S. C. Solomon, R. J. Phillips, D. E. Smith, G. L. Tyler, O. Aharonson, G. Balmino, W. B. Banerdt, J. W. Head, C. L. Johnson, et al. (2000)
Science
287, 1788-1793
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