Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass

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dc.creatorLindsay, B. D.
dc.creatorOrr, K. W.
dc.creatorHyde, T. W.
dc.creatorBarge, L.
dc.date2004-01-29
dc.date.accessioned2026-07-07T05:51:07Z
dc.date.available2026-07-07T05:51:07Z
dc.descriptionNumerical 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.
dc.description2 pages, Lunar and Planetary Science XXXIV (2003)
dc.identifierhttps://arxiv.org/abs/physics/0401160
dc.identifierhttp://arxiv.org/abs/physics/0401160
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/85921
dc.subjectSpace Physics
dc.titleGravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass
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