Title of article
The Galileo star scanner observations at Amalthea
Author/Authors
Fieseler، نويسنده , , Paul T. and Adams، نويسنده , , Olen W and Vandermey، نويسنده , , Nancy and Theilig، نويسنده , , E.E and Schimmels، نويسنده , , Kathryn A and Lewis، نويسنده , , George D and Ardalan، نويسنده , , Shadan M and Alexander، نويسنده , , Claudia J، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2004
Pages
12
From page
390
To page
401
Abstract
In November of 2002, the Galileo spacecraft passed within 250 km of Jupiterʹs 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 Amaltheaʹs orbit just prior to Galileoʹs 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 Jupiterʹs Gossamer ring system.
Keywords
Satellites of Jupiter , Impact processes , Planetary ringsJupiter
Journal title
Icarus
Serial Year
2004
Journal title
Icarus
Record number
2372948
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