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Science 13 March 1998:
Vol. 279. no. 5357, pp. 1686 - 1692
DOI: 10.1126/science.279.5357.1686

Reports

Topography of the Northern Hemisphere of Mars from the Mars Orbiter Laser Altimeter

D. E. Smith, * M. T. Zuber, dagger H. V. Frey, J. B. Garvin, J. W. Head, D. O. Muhleman, G. H. Pettengill, R. J. Phillips, S. C. Solomon, H. J. Zwally, W. B. Banerdt, T. C. Duxbury

The first 18 tracks of laser altimeter data across the northern hemisphere of Mars from the Mars Global Surveyor spacecraft show that the planet at latitudes north of 50° is exceptionally flat; slopes and surface roughness increase toward the equator. The polar layered terrain appears to be a thick ice-rich formation with a non-equilibrium planform indicative of ablation near the periphery. Slope relations suggest that the northern Tharsis province was uplifted in the past. A profile across Ares Vallis channel suggests that the discharge through the channel was much greater than previously estimated. The martian atmosphere shows significant 1-micrometer atmospheric opacities, particularly in low-lying areas such as Valles Marineris.

D. E. Smith, H. V. Frey, J. B. Garvin, H. J. Zwally, Earth Sciences Directorate, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA.
M. T. Zuber and G. H. Pettengill, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
J. W. Head, Brown University, Providence, RI 02912, USA.
D. O. Muhleman, California Institute of Technology, Pasadena, CA 91125, USA
R. J. Phillips, Washington University, St. Louis, MO 63130, USA.
S. C. Solomon, Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA.
W. B. Banerdt and T. C. Duxbury, Jet Propulsion Laboratory, Pasadena, CA 91109, USA.
*   To whom correspondence should be addressed.

dagger    Also at: Laboratory for Terrestrial Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.


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