Planetary shape: internal constraints for small bodies.

Details Planetary shape: internal constraints for small bodies. Planetary shape: internal constraints for small bodies.

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984geoji..78..219b&link_type=abstract

Geophysical Journal International, Vol. 78, No. 1, p. 219 - 229

Physics

Scientific paper

This paper describes the attainment of sphericity, or equivalent
isopotential forms, for the surface of small Solar System objects
(linear dimensions ≡300 km) as a consequence of viscous relaxation
(creep).

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