Topography of the Northern Hemisphere of Mars from the Mars Orbiter Laser Altimeter
Article 1998 en
Authors
DS
David E. Smith
MZ
M. T. Zuber
HF
Herbert Frey
Abstract
1 min read
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.
David E. Smith, M. T. Zuber, Herbert Frey, James Jim Brian Garvin, J. W. Head, D. O. Muhleman, G. H. Pettengill, R. J. Phillips, Sean C. Solomon, H. Jay Zwally, W. B. Banerdt, T. Duxbury, M. P. Golombek, F. G. Lemoine, G. A. Neumann, D. D. Rowlands, O. Aharonson, P. G. Ford, A. B. Ivanov, C. L. Johnson, P. J. McGovern, James B. Abshire, Robert S. Afzal, Xiaoli Sun
David E. Smith, M. T. Zuber, H. V. Frey, James Jim Brian Garvin, J. W. Head, D. O. Muhleman, G. A. Neumann, G. H. Pettengill, R. J. Phillips, Sean C. Solomon
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