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 ,
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.