Escape of ejecta from cratered solar system satellites

Details Escape of ejecta from cratered solar system satellites Escape of ejecta from cratered solar system satellites

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204..635p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, Aug. 1983, p. 635-645. Research supported by the S

Astronomy and Astrophysics

Astronomy

2

Craters, Ejecta, Escape Velocity, Natural Satellites, Satellite Surfaces, Mimas, Phobos, Three Dimensional Models, Planets, Ejecta, Satellites, Craters, Escape, Velocity, Models, Tidal Effects, Rotation, Shape, Parameters, Mars, Phobos, Morphology, Stickney, Saturn, Mimas, Icy Bodies

Scientific paper

The authors investigate the effect of craters on the variation of the escape velocity over the surface of spherical and ellipsoidal satellites. Three-dimensional numerical models are used and several factors - planetary tides, satellite rotation and non-spherical shape - are included. It is found that in most cases craters have considerable effects only in their vicinity. However, in the case of Phobos the morphology of the satellite and the variation of the escape velocity over its surface are significantly affected by the presence of crater Stickney.

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