A model for the formation of the rotational motion of celestial bodies with constraints on the order of resonances

Details A model for the formation of the rotational motion of celestial bodies with constraints on the order of resonances A model for the formation of the rotational motion of celestial bodies with constraints on the order of resonances

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990avest..24..140b&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 24, Apr.-June 1990, p. 140-147. In Russian.

Astronomy and Astrophysics

Astronomy

Orbital Resonances (Celestial Mechanics), Planetary Rotation, Solar System, Tides, Astronomical Models, Axes Of Rotation, Circular Orbits, Elliptical Orbits, Inclination

Scientific paper

The tidal model of the formation of the inclinations and rotations of planetary and satellite systems in the solar system is examined, taking the compression process into account. The inclinations take either near-zero or relatively large values. For bodies with small inclinations, the order of the resonances cannot be higher than 2:1 (that is, they can take values of 1:1, 3:2, and 2:1).

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