The effects of tidal forces on the stability and dispersal rates of a protoplanet

Details The effects of tidal forces on the stability and dispersal rates of a protoplanet The effects of tidal forces on the stability and dispersal rates of a protoplanet

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.172..257d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 172, Aug. 1975, p. 257-269. Research supported by the Science Research

Computer Science

Numerical Analysis

30

Orbital Elements, Planetary Evolution, Solar System, Tides, Circular Orbits, Condensates, Dynamic Stability, Elliptical Orbits, Equations Of Motion, Numerical Analysis

Scientific paper

The tidal disruption of a protoplanet by the sun is considered using both analytical and numerical means. It is concluded that the disruption process is very rapid and that this implies that most conventional protoplanetary theories for the formation of planets need to be modified; otherwise, complete disruption would have occurred before a refractory core could form.

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