Results 31 to 40 of about 157 (99)
The relationship between the `limiting' Yarkovsky drift speed and asteroid families' Yarkovsky V-shape [PDF]
The Yarkovsky effect is an important force to consider in order to understand the long-term dynamics of asteroids. This non-gravitational force affects the orbital elements of objects revolving around a source of heat, especially their semi ...
Milić-Žitnik I.
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On Stable Chaos in The Asteroid Belt [PDF]
AbstractThe twenty most chaotic objects found among first hundred of numbered asteroids are studied. Lyapunov time calculated with and without inner planets indicates that for eleven of those asteroids the strongest chaotic effect results from the resonances with Mars.
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The transiting dust clumps in the evolved disc of the Sun-like UXor RZ Psc [PDF]
RZ Psc is a young Sun-like star, long associated with the UXor class of variable stars, which is partially or wholly dimmed by dust clumps several times each year.
Grant M. Kennedy+6 more
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The distribution of basaltic asteroids in the Main Belt [PDF]
We present the observational results of a survey designed to target and detect asteroids whose colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. Fifty basaltic candidates were selected with orbital elements that lie outside of the Vesta dynamical family.
Ronald Fevig+7 more
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Phase Curves of Kuiper Belt Objects, Centaurs, and Jupiter-family Comets from the ATLAS Survey
The Kuiper Belt objects (KBOs), the Centaurs, and the Jupiter-family comets (JFCs) form an evolutionary continuum of small outer solar system objects, and their study allows us to gain insight into the history and evolution of the solar system. Broadband
Matthew M. Dobson+11 more
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Intelligent Interplanetary Satellite Communication Network for the Exploration of Celestial Bodies
Recently, a significant interest in space exploration has emerged, driven by the lack of resources and the quest for answers to issues like climate change.
Abraham Urieta-Ortega+2 more
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Physical properties of asteroids
The most significant data on the physical properties of main-belt and near-Earth asteroids obtained by photometric, polarimetric, spectroscopic and other techniques, including space missions «Galileo» and NEAR, are presented.
D. F. Lupishko
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Orbital systems are often self-organized and/or characterized by harmonic relations. Inspired by music theory, we rewrite the Geddes and King-Hele (QJRAS, 24, 10–13, 1983) equations for mirror symmetries among the distances of the planets of the Solar ...
Michael J. Bank, Nicola Scafetta
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The Mid-plane of the Main Asteroid Belt [PDF]
Abstract We measure the mid-plane of the main asteroid belt by using the observational data of a nearly complete and unbiased sample of asteroids and find that it has inclination and longitude of ascending node
Saverio Cambioni, Renu Malhotra
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Asteroid Collisions: Expected Visibility and Rate
Asteroid collisions are one of the main processes responsible for the evolution of bodies in the main belt. Using observations of the Dimorphos impact by the DART spacecraft, we estimate how asteroid collisions in the main belt may look in the first ...
Eran O. Ofek+11 more
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