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Characteristics and Large Bulk Density of the C-type Main-Belt Triple Asteroid (93) Minerva
F. Marchis, F. Vachier, J. Ďurech +11
From a set of adaptive optics (AO) observations collected with the W.M. Keck telescope between August and September 2009, we derived the orbital parameters of the most recently dis…
An anisotropic distribution of spin vectors in asteroid families
J. Hanuš, M. Brož, J. Ďurech +11
Current amount of ~500 asteroid models derived from the disk-integrated photometry by the lightcurve inversion method allows us to study not only the spin-vector properties of the…
Sizes of main-belt asteroids by combining shape models and Keck adaptive aptics observations
J. Hanuš, F. Marchis, J. Ďurech
We select 50 main-belt asteroids with a diameter between 20 and 400 km for which we have (i) shape models derived by the lightcurve inversion method (LI) and (ii) resolved observat…
The Resolved Asteroid Program - Size, shape, and pole of (52) Europa
W. J. Merline, J. D. Drummond, B. Carry +14
With the adaptive optics (AO) system on the 10 m Keck-II telescope, we acquired a high quality set of 84 images at 14 epochs of asteroid (52) Europa on 2005 January 20. The epochs…