Collisional and dynamical processes in moon and planet formation

Details Collisional and dynamical processes in moon and planet formation Collisional and dynamical processes in moon and planet formation

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pggp.rept..112c&link_type=abstract

In NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986 p 112-114 (SEE N87-23341 16-91)

Physics

Geophysics

Collisions, Deposition, Lunar Evolution, Moon, Planetary Evolution, Planetary Rings, Planets, Protoplanets, Computerized Simulation, Dust, Gases, Mathematical Models, Monte Carlo Method, Planetary Orbits, Resonance

Scientific paper

Research on a variety of dynamical processes relevant to the formation
of planets, satellites and ring systems is discussed. The main focus is
on studies of accretionary formation of early protoplanets using a
numerical model, structures and evolution of ring systems and individual
bodies within planetary rings, and theories of lunar origin.

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