Journal
ANNUAL REVIEW OF EARTH AND PLANETARY SCIENCES, VOL 38
Volume 38, Issue -, Pages 493-522Publisher
ANNUAL REVIEWS
DOI: 10.1146/annurev-earth-040809-152513
Keywords
planet formation; solar system; accretion; planets; circumstellar disks; fluid mechanics; turbulence
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Planets are built from planetesimals: solids larger than a kilometer that grow by colliding in pairs. Planetesimals themselves are unlikely to form by two-body collisions alone; subkilometer objects have gravitational fields individually too weak, and electrostatic attraction is too feeble for growth beyond a few centimeters. We review the possibility that planetesimals form when self-gravity brings together vast ensembles of small particles. Even when self-gravity is weak, aerodynamic processes can accumulate solids relative to gab, paving the way for gravitational collapse. Particles pile up as they drift radially inward. Gas turbulence stirs particles but can also seed collapse by Clumping them. Whereas the feedback of solids on gas triggers vertical-shear instabilities that obstruct self-gravity, this same feedback triggers streaming instabilities that strongly concentrate particles. Numerical simulations find that solids similar to 10-100 cm in size gravitationally collapse in turbulent disks. We outline areas for progress, including the possibility that still smaller objects self-gravitate.
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