The global topography of Mars and implications for surface evolution

被引:682
作者
Smith, DE [1 ]
Zuber, MT
Solomon, SC
Phillips, RJ
Head, JW
Garvin, JB
Banerdt, WB
Muhleman, DO
Pettengill, GH
Neumann, GA
Lemoine, FG
Abshire, JB
Aharonson, O
Brown, CD
Hauck, SA
Ivanov, AB
McGovern, PJ
Zwally, HJ
Duxbury, TC
机构
[1] NASA, Goddard Space Flight Ctr, Earth Sci Directorate, Greenbelt, MD 20771 USA
[2] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
[3] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA
[4] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[5] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[6] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[7] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
D O I
10.1126/science.284.5419.1495
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
Elevations measured by the Mars Orbiter Laser Altimeter have yielded a high-accuracy global map of the topography of Mars. Dominant features include the low northern hemisphere, the Tharsis province, and the Hellas impact basin. The northern hemisphere depression is primarily a long-wavelength effect that has been shaped by an internal mechanism. The topography of Tharsis consists of two broad rises. Material excavated from Hellas contributes to the high elevation of the southern hemisphere and to the scarp along the hemispheric boundary. The present topography has three major drainage centers, with the northern Lowlands being the largest. The two polar cap volumes yield an upper limit of the present surface water inventory of 3.2 to 4.7 million cubic kilometers.
引用
收藏
页码:1495 / 1503
页数:11
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