Physics
Scientific paper
Oct 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993stgg...37..326b&link_type=abstract
Stud. Geophys. Geod., Vol. 37, No. 4, p. 326 - 330
Physics
Minor Planets: Figures
Scientific paper
The tri-axial figure of the asteroid 2 Pallas poses the question of the origin of this phenomenon. The tidal-forming potential and rotational disturbances may be fully responsible for it. However, this hypothesis requires Pallas to be a primordial satellite orbiting the hypothetical central body synchronously, i.e. in 1/1 orbital/rotational resonance; its mean motion has been estimated.
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