Ancient Geodynamics and Global-Scale Hydrology on Mars

Author:

Phillips Roger J.1,Zuber Maria T.23,Solomon Sean C.4,Golombek Matthew P.5,Jakosky Bruce M.6,Banerdt W. Bruce5,Smith David E.3,Williams Rebecca M. E.1,Hynek Brian M.1,Aharonson Oded2,Hauck II Steven A.1

Affiliation:

1. McDonnell Center for the Space Sciences and Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA.

2. Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.

3. Earth Sciences Directorate, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA.

4. Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA.

5. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

6. Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80309, USA.

Abstract

Loading of the lithosphere of Mars by the Tharsis rise explains much of the global shape and long-wavelength gravity field of the planet, including a ring of negative gravity anomalies and a topographic trough around Tharsis, as well as gravity anomaly and topographic highs centered in Arabia Terra and extending northward toward Utopia. The Tharsis-induced trough and antipodal high were largely in place by the end of the Noachian Epoch and exerted control on the location and orientation of valley networks. The release of carbon dioxide and water accompanying the emplacement of ∼3 × 10 8 cubic kilometers of Tharsis magmas may have sustained a warmer climate than at present, enabling the formation of ancient valley networks and fluvial landscape denudation in and adjacent to the large-scale trough.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference47 articles.

1. Evolution of the Tharsis Province of Mars: The importance of heterogeneous lithospheric thickness and volcanic construction

2. M. T. Zuber et al. Science 287 1788 (2000).

3. W. B. Banerdt M. P. Golombek K. L. Tanaka in Mars H. H. Kieffer B. M. Jakosky C. W. Snyder M. S. Matthews Eds. (Univ. of Arizona Press Tucson AZ 1992) pp. 249–297.

4. D. E. Smith et al. Science 286 94 (1999).

5. D. E. Smith et al. Science 284 1495 (1999).

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