Výsledky vyhledávání - "Nazzario, R."

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Autor: Nazzario, R. C., Orr, K., Covington, C., Kagan, D., Hyde, T. W.

Publikováno v: Adv.SpaceRes.40:280-283,2007

It has been observed that binary Kuiper Belt Objects (KBOs) exist contrary to theoretical expectations. Their creation presents problems to most current models. However, the inclusion of a third body (for example, one of the outer planets) may provid

Externí odkaz: http://arxiv.org/abs/astro-ph/0507149

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Numerical Investigations of Kuiper Belt Binaries

Autor: Nazzario, R. C., Hyde, T. W.

Observations of the Kuiper Belt indicate that a larger than expected percentage of KBO's (approximately 8 out of 500) are in binary pairs. The formation and survival of such objects presents a conundrum [1]. Two competing theories have been postulate

Externí odkaz: http://arxiv.org/abs/physics/0501113

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Orbits of Dust Ejecta From Ceres

Autor: Nazzario, R. C., Hyde, T. W.

The question of whether asteroid ejecta can enter stable orbits about the parent body is examined.
Comment: 2 pages, Lunar and Planetary Science XXXIII (2002)

Externí odkaz: http://arxiv.org/abs/physics/0401152

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Further Investigations of Dust Grain Orbital Behavior Around Neptune

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

Dust grain orbital behavior around Neptune is investigated using a fifth order Runge-Jutta method.
Comment: 2 pages, Lunar and Planetary Science XXXII (2001)

Externí odkaz: http://arxiv.org/abs/physics/0401148

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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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