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Letters to Nature
Nature 374, 783 - 785 (27 April 1994); doi:10.1038/374783a0

Discovery and physical properties of Dactyl, a satellite of asteroid 243 Ida

C. R. Chapman*, J. Veverka, P. C. Thomas, K. Klaasen, M. J. S. Belton§, A. Harch, A. McEwen, T. V. Johnson, P. Helfenstein, M. E. Davies£, W. J. Merline* & T. Denkstar

*Planetary Science Institute/SJI, 620 N. 6th Avenue, Tucson, Arizona 85705, USA
Center for Radiophysics and Space Research, Cornell University, Ithaca, New York 14853, USA
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA
§National Optical Astronomy Observatories, Tucson, Arizona 85719, USA
US Geological Survey, Flagstaff, Arizona 86001, USA
£RAND, Santa Monica, California 90406, USA
starInstitut für Planetenerkundung, 12484 Berlin, Germany
Present address: Center for Radiophysics and Space Research, Cornell University, Ithaca, New York 14853, USA.

OBSERVATIONS of stellar occultations by asteroids have suggested that some may have satellites1. But given the absence of any confirmatory evidence, the prevailing view has been that although such satellites probably do exist, they are likely to be rare2. Here we report the discovery3 by the Galileo spacecraft of a satellite associated with the asteroid 243 Ida. Although the satellite, Dactyl, is only 1.6km across, it has been imaged with sufficient resolution for geological analysis. We describe the physical properties of Dactyl, with emphasis on its notably smooth shape, its crater population (which includes a crater chain) and its photometric properties. We find that, spectroscopically, Dactyl resembles both Ida and the other members of the Koronis asteroid family, implying a similar composition; small spectral differences may reflect a space weathering process that slightly alters the colours with time. We argue that Dactyl originated during the breakup of the Koronis parent body, and that satellites could be common around other asteroids (particularly members of asteroid families).

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