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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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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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Collisional evolution of asteroids and asteroid families.
1987After a general review of the current ideas about collisional evolution the problems concerning the interpretation of asteroid families as outcomes of catastrophic processes are discussed.
PAOLICCHI, PAOLO, Zappalà V.
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Rogue Asteroids in the Inner Main Asteroid Belt
2014Very red featureless asteroids (spectroscopic D-types) are common among Jupiter Trojans, Hildas, and the outer main belt, and are thought to have formed in the outer solar system. Dynamical models of planetary migration and orbital drift by the Yarkovsky effect predict these D-types could have been transported as close to the sun as the middle main ...
Demeo, Francesca E. +4 more
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