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This mosaic of five images was taken through the clear filter (610 nanometers) of the solid state imaging system (CCD) aboard NASA's Galileo spacecraft on October 5, 1996. The mosaic is shown twice; the top panel displays only the data, while the bottom panel gives the location of some of Jupiter's small ring moons and presents a match between the image and a simple geometrical model of the gossamer rings. From the spacecraft's distance of approximately 6.6 million kilometers (km), the images have a resolution of about 134 km per pixel (picture element). The images were acquired when Galileo was in Jupiter's shadow, peering back toward the Sun, hidden behind the planet. The spacecraft was located only about 0.15 degrees above the ring plane at the time, making the images highly foreshortened in the vertical direction. North is to the bottom. The white vertical arc at the left edge of the top panel is caused by sunlight filtering through Jupiter's upper atmosphere; the white horizontal line in the left part of the figure is the main ring whose arms overlap in this foreshortened view. The next frame of the mosaic, taken at higher sensitivity to detect fainter material, shows (on the left part of this panel) the overexposed main ring and the halo (seen as material above and below the main ring) which is interior to the main ring and has become visible in this longer exposure. The middle panel, taken at twenty times the standard sensitivity, shows a tenuous horizontal stripe, which can be made out in the "10 times sensitivity" panel also. In contrast to the main ring, which ends in a narrow elliptical tip, this "gossamer ring" ends abruptly (in the middle of the image) without changing its vertical thickness; the ring is also unusual in that its top and bottom edges are about twice as bright as the central region. Interestingly this ring is only seen to precisely the orbital distance of Amalthea, a small (mean radius of 85 km) Jovian moon, and has a half-thickness that is the same as Amalthea's maximum excursion off Jupiter's equatorial plane.

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      EUN,LOM,LRE4,hdl:10494/259038,work-cmr-id:259038,http://photojournal.jpl.nasa.gov:http://photojournal.jpl.nasa.gov/catalog/PIA01623,ilox,learning resource exchange,LRE metadata application profile,LRE

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