Topography of the northern hemisphere of Mars from the Mars orbiter laser altimeter

被引:183
作者
Smith, DE [1 ]
Zuber, MT
Frey, HV
Garvin, JB
Head, JW
Muhleman, DO
Pettengill, GH
Phillips, RJ
Solomon, SC
Zwally, HJ
Banerdt, WB
机构
[1] NASA, Earth Sci Directorate, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] MIT, Cambridge, MA 02139 USA
[3] Brown Univ, Providence, RI 02912 USA
[4] CALTECH, Pasadena, CA 91125 USA
[5] Washington Univ, St Louis, MO 63130 USA
[6] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA
[7] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[8] NASA, Terr Phys Lab, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
关键词
D O I
10.1126/science.279.5357.1686
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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 degrees 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 chan nel was much greater than previously estimated. The martian atmosphere shows significant 1-micrometer atmospheric opacities, particularly in low-lying areas such as Valles Marineris.
引用
收藏
页码:1686 / 1692
页数:7
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