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5![REPORTS exceeding 40° when referred to the ellipsoid. Gravitational slopes are slightly less steep but also reach up to ~ 40° on a lower-resolution shape model (~700 m). A considerable number of slopes on Vesta are mos REPORTS exceeding 40° when referred to the ellipsoid. Gravitational slopes are slightly less steep but also reach up to ~ 40° on a lower-resolution shape model (~700 m). A considerable number of slopes on Vesta are mos](https://www.pdfsearch.io/img/a4da2a4ebaaa0f05c2633ff690b641f6.jpg) | Add to Reading ListSource URL: www-ssc.igpp.ucla.eduLanguage: English - Date: 2012-06-22 13:09:07
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10![Microsymposium 38, MS090, 2003 (A4 format) THE MORPHOMETRIC ANALISYS OF THE FEATURES OF MARTIAN CRATERS. I.A. Ushkin1, G. G. Michael2, E.A. Kozlova3 . 1. Moscow State University, Vorobjovy Gory, 119899, Moscow, Russia, g Microsymposium 38, MS090, 2003 (A4 format) THE MORPHOMETRIC ANALISYS OF THE FEATURES OF MARTIAN CRATERS. I.A. Ushkin1, G. G. Michael2, E.A. Kozlova3 . 1. Moscow State University, Vorobjovy Gory, 119899, Moscow, Russia, g](https://www.pdfsearch.io/img/8fa8af8220abfb16cef2aa5c39a83c3d.jpg) | Add to Reading ListSource URL: selena.sai.msu.ruLanguage: English - Date: 2008-10-06 10:10:05
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