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Science 13 March 1998: Vol. 279. no. 5357, pp. 1686 - 1692 DOI: 10.1126/science.279.5357.1686
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Reports
Topography of the Northern Hemisphere of Mars from the Mars Orbiter Laser Altimeter
D. E. Smith,
*
M. T. Zuber,
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.
Also at: Laboratory for Terrestrial Physics, NASA Goddard
Space Flight Center, Greenbelt, MD 20771, USA.
Read the Full Text
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