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Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass

B. D. Lindsay·K. W. Orr·T. W. Hyde·L. Barge
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Abstract

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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B. D. Lindsay, K. W. Orr, T. W. Hyde, L. Barge. 2004-01-29. Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass. https://arxiv.org/abs/physics/0401160

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