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Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass

Autor: Lindsay, B. D., Orr, K. W., Hyde, T. W., Barge, L.

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.
Comment: 2 pages, Lunar and Planetary Science XXXIV (2003)

Externí odkaz: http://arxiv.org/abs/physics/0401160

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Dust Grain Orbital Behavior Around Ceres

Autor: Nazzario, R., Hyde, T. W., Barge, L.

Many asteroids show indications they have undergone impacts with meteoroid particles having radii between 0.01 m and 1 m. During such impacts, small dust grains will be ejected at the impact site. The possibility of these dust grains (with radii grea

Externí odkaz: http://arxiv.org/abs/physics/0308075

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Finite Coulomb Crystal Formation

Autor: Vasut, J., Hyde, T. W., Barge, L.

Dust particles immersed within a plasma environment, such as those found in planetary rings or comets, will acquire an electric charge. If the ratio of the inter-particle potential energy to average kinetic energy is large enough the particles will f

Externí odkaz: http://arxiv.org/abs/physics/0308074

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Enceladus as a potential oasis for life:science goals and investigations for future explorations

Enceladus is the first planetary object for which direct sampling of a subsurface water reservoir, likely habitable, has been performed. Over a decade of flybys and seven flythroughs of its watery plume, the Cassini spacecraft determined that Encelad

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______2423::043ba9070d93115adfa48e50e0281212
http://urn.fi/urn:nbn:fi-fe2023022328565

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