Occurrence of central peak craters on the Saturnian satellites - Implications for surface structure

Details Occurrence of central peak craters on the Saturnian satellites - Implications for surface structure Occurrence of central peak craters on the Saturnian satellites - Implications for surface structure

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986em%26p...35..117t&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 35, June 1986, p. 117, 118.

Computer Science

3

Planetary Craters, Planetary Structure, Satellite Surfaces, Saturn Satellites, Satellite Imagery, Surface Geometry, Topography

Scientific paper

The presence of craters with central peaks on the ice satellites of
Saturn implies that their surface elastic strength is comparable to that
of the Moon, Mars, and Mercury which have central peak craters, rather
than that of the Jovian ice satellites Ganymede and Callisto which do
not have central peak craters.

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