The Gravity Field of Mars: Results from Mars Global Surveyor

Author:

Smith David E.1,Sjogren William L.2,Tyler G. Leonard3,Balmino Georges4,Lemoine Frank G.1,Konopliv Alex S.2

Affiliation:

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.

Abstract

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.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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4. Independent models were developed at NASA Goddard Space Flight Center (GSFC) and the Jet Propulsion Laboratory (JPL). The fields were solved (33) to degree and order 70 (7) and 75 (6) but are shown and interpreted only to degree and order 48 corresponding to a half-wavelength resolution of 220 km. Peak values of gravitational features depend on the effective resolution of the gravity model.

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