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Determination of Masses of Six Asteroids from Close Asteroid—Asteroid Encounters
2001New masses of six asteroids: (6) Hebe, (10) Hygiea, (15) Eunomia, (52) Europa, (511) Davida and (704) Interamnia were determined within the ongoing Asteroid Mass Determination Program, started in 1998 in the Wroclaw University Observatory. The masses were calculated by means of the least-squares method as weighted means of the values found separately ...
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Collisions of Asteroids: Asteroid (596) Sheila
Astrophysical Bulletin, 2019Among the small bodies of the Solar System, at present, a group of bodies, called comets of the main belt, exhibiting dynamic and/or physical properties of both comets and asteroids is distinguished. One of the reasons for such manifestations may be collisions with other bodies.
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Asteroid-Asteroid Interactions - Dynamically Irrelevant?
1991Structural investigations of the distribution of the asteroids have so far concentrated on the interactions with the major planets, especially Jupiter, and the resulting effects in element space. Here some less known structures of their distribution in actual space are shown: the radial number density and the orthogonal orbit density.
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First mission to Jupiter’s asteroids could reveal Solar System origins
Nature, 2021Witze Alexandra
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Fine-regolith production on asteroids controlled by rock porosity
Nature, 2021Saverio Cambioni +2 more
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Connecting asteroids and meteorites with visible and near-infrared spectroscopy
Icarus, 2022Benoit Carry +2 more
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