Lunar polar topography derived from Clementine stereoimages
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作者:
Cook, AC
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Natl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USANatl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USA
Cook, AC
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Watters, TR
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机构:Natl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USA
Watters, TR
Robinson, MS
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机构:Natl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USA
Robinson, MS
Spudis, PD
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机构:Natl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USA
Spudis, PD
Bussey, DBJ
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机构:Natl Air & Space Museum, Ctr Earth & Planetary Studies, Washington, DC 20560 USA
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
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.