Lunar polar topography derived from Clementine stereoimages

被引:25
|
作者
Cook, AC [1 ]
Watters, TR
Robinson, MS
Spudis, PD
Bussey, DBJ
机构
[1] Natl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USA
[2] Northwestern Univ, Dept Geol Sci, Evanston, IL 60208 USA
[3] Lunar & Planetary Inst, Houston, TX 77058 USA
[4] ESA, Estec, Dept Space Sci, Noordwijk, Netherlands
关键词
D O I
10.1029/1999JE001083
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Clementine stereoimagery has been used to produce digital elevation models of the Moon, at a scale of similar to 1 km/pixel. These models cover regions poleward of 60 degrees in both hemispheres and reveal topography beyond that covered by the Clementine laser altimeter or Earth-based radar. By combining these polar terrain models with the current Clementine laser altimeter data we have produced a global topographic map of the lunar surface. Several topographic features in the new polar including three previously unrecognized pre-Nectarian have also been mapped, including the southern extent other previously suspected basins have been verified.
引用
收藏
页码:12023 / 12033
页数:11
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