Other
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24.1511w&link_type=abstract
In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z p 1511-1512 (SEE N94-20636 05-91
Other
2
Angular Momentum, Astronomical Models, Escape Velocity, Orbital Velocity, Planetary Evolution, Planetary Gravitation, Planetary Systems, Solar System Evolution, Stellar Evolution, Cosmology, Gas Giant Planets, Mathematical Models, Natural Satellites, Stars, Stellar Envelopes, Terrestrial Planets
Scientific paper
Observation of circumstellar disks, regular satellite systems of outer planets, and planet-size objects orbiting pulsars support the supposition that formation of planetary systems is a robust, rather than a fragile, byproduct of the formation and evolution of stars. The extent to which these systems may be expected to resemble one another and our Solar System, either in overall structure or in detail remains uncertain. When the full range of possible stellar masses, disk masses, and initial specific angular momenta are considered, the possible variety of planetary configurations is very large. Numerical modeling indicates a difference between the formation of small, inner, terrestrial planets and the outer planets.
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