Impact Crater Topography and Morphology on Saturnian Mid-Sized Satellites

Details Impact Crater Topography and Morphology on Saturnian Mid-Sized Satellites Impact Crater Topography and Morphology on Saturnian Mid-Sized Satellites

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.2305s&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

4

Scientific paper

New topographic mapping of Saturn's icy satellites reveal a wealth of
detail. Relaxed impact crater topography is evident on Enceladus, Dione,
and Tethys, but not the largest moons, Rhea and Iapetus. Central peaks
up to 10 km high tower above surrounding

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