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The Galileo star scanner observations at Amalthea
Authors:Paul D Fieseler  Olen W Adams  Nancy Vandermey  EE Theilig  Kathryn A Schimmels  George D Lewis  Shadan M Ardalan  Claudia J Alexander
Institution:Galileo Project, Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
Abstract:In November of 2002, the Galileo spacecraft passed within 250 km of Jupiter's moon Amalthea. An onboard telescope, the star scanner, observed a series of bright flashes near the moon. It is believed that these flashes represent sunlight reflected from 7 to 9 small moonlets located within about 3000 km of Amalthea. From star scanner geometry considerations and other arguments, we can constrain the diameter of the observed bodies to be between 0.5 m to several tens of kilometers. In September of 2003, while crossing Amalthea's orbit just prior to Galileo's destruction in the jovian atmosphere, a single additional body seems to have been observed. It is suspected that these bodies are part of a discrete rocky ring embedded within Jupiter's Gossamer ring system.
Keywords:Satellites of Jupiter  Planetary rings  Jupiter  Impact processes
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