Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass
Bruce D. Lindsay, Kimberly Orr, Truell Hyde, Laurie Barge
Abstract
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Bruce D. Lindsay, Kimberly Orr, Truell Hyde, Laurie Barge
Abstract
Open-access reader
Numerical simulations show that planetesimal systems with unevenly distributed masses may actually be more stable than those where all the bodies are of roughly equal size.
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Numerical simulations show that planetesimal systems with unevenly distributed masses may actually be more stable than those where all the bodies are of roughly equal size.
Key concepts: Protoplanet, Physics, Gravitation, Astronomy, Astrophysics, Classical mechanics, Astrobiology, Stars