Provenance of the terrestrial planets.
Earlier work on the simultaneous accumulation of the asteroid belt and the terrestrial planets is extended to investigate the relative contribution to the final planets made by material from different heliocentric distances. As before, stochastic variations intrinsic to the accumulation processes lead to a variety of final planetary configurations, but include systems having a number of features similar to our solar system. Fifty-nine new simulations are presented, from which thirteen are selected as more similar to our solar system than the others. It is found that the concept of "local feeding zones" for each final terrestrial planet has no validity for this model. Instead, the final terrestrial planets receive major contributions from bodies ranging from 0.5 to at least 2.5 AU, and often to greater distances. Nevertheless, there is a correlation between the final heliocentric distance of a planet and its average provenance. Together with the effect of stochastic fluctuations, this permits variation in the composition of the terrestrial planets, such as the difference in the decompressed density of Earth and Mars. Biologically important light elements, derived from the asteroidal region, are likely to have been significant constituents of the Earth during its formation.
Wetherill
G W
GW
Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA.
D055580:Astronomical Phenomena; D001256:Astronomy; D003198:Computer Simulation; D019419:Evolution, Planetary; D018543:Minor Planets; D008962:Models, Theoretical; D016083:Planets; D016082:Solar System