Jupiter's Ringswn-jupring2.t.jpg (3221 bytes)
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JPL Planetary Photojournal Catalog #PIA01621

Jupiter's Gossamer Ring (Main ring at far right)
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JPL Planetary Photojournal Catalog #PIA00659


Diagram of Jupiter's Ring System
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JPL Planetary Photojournal Catalog #PIA01627

Galileo Reveals Process Behind Formation of Jupiter's Rings
September 15, 1998.

The Galileo spacecraft, now in orbit around Jupiter, returned images revealing new details of the giant planets' rings. The rings consist of an inner main ring and two outer Gossamer rings. Scientists now believe the rings are formed as asteroids and meteors, pulled in by Jupiter's massive gravitational field, strike the planet's inner satellites kicking up dust and debris. This dust and debris enters Jupiter's orbit at much the same distance and orientation as their source satellites. Scientists therefore believe Almathea and Thebe are the main source satellites for debris forming the Gossamer rings, while debris from the satellites Adrastea and Metis likely formed the inner main ring.
For more information, see the Galileo Project home page at http://www.jpl.nasa.gov/galileo

All images courtesy JPL Planetary Photojournal.

 

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