2004arXiv (Cornell University)Open access

Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass

Bruce D. Lindsay, Kimberly Orr, Truell Hyde, Laurie 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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What this paper is about

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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Available 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.

Key concepts: Protoplanet, Physics, Gravitation, Astronomy, Astrophysics, Classical mechanics, Astrobiology, Stars

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