Statistics – Computation
Scientific paper
Jun 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pggp.rept..430w&link_type=abstract
In NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990 p 430-432 (SEE N92-10728 01-91)
Statistics
Computation
Accretion Disks, Density Wave Model, Eccentricity, Inclination, Orbit Calculation, Orbit Perturbation, Orbital Elements, Planetary Rings, Protoplanets, Astronomical Models, Celestial Mechanics, Computational Astrophysics, Nebulae, Orbital Mechanics, Orbital Resonances (Celestial Mechanics), Perturbation Theory, Planetary Evolution
Scientific paper
Disk tides may play an important role in the formation of a planetary system. Modification of protoplanet semi-major axes and eccentricities through density waves was suggested and calculations of linear and non-linear protoplanet-nebula interactions were carried out by a number of researchers. The possible significance of radial drift to the accretion process was discussed, while the evolution of orbital eccentricities was studied for a perturber orbiting external to a ring and for a perturber embedded in the ring. The possible importance of bending waves to the early evolution of protoplanet inclinations is described.
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