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Neptune's Ring System
Evidence for incomplete arcs around Neptune first arose in the
mid-1980's, when stellar occultation experiments were found to
occasionally show an extra "blink" just before or after the planet
occulted the star. Images by Voyager 2 in 1989 settled the issue, when
the ring system was found to contain several faint rings, the outermost
of which, Adams, contains three prominent arcs now named Liberty,
Equality and Fraternity. The existence of arcs is very difficult to
understand because the laws of motion would predict that arcs spread out
into a uniform ring over very short timescales. The gravitational
effects of Galatea, a moon just inward from the ring, are now believed
to confine the arcs. Several other rings were detected by the Voyager
cameras. In addition to the narrow Adams Ring 63,000 km from the center
of Neptune, the Leverrier Ring is at 53,000 km and the broader, fainter
Galle Ring is at 42,000 km. A faint outward extension to the Leverrier
Ring has been named Lassell; it is bounded at its outer edge by the
Arago Ring at 57,000 km.
Index
More Links to Rings Node Facilities...
Animations
Ring Arc Closeup
(QuickTime (MOV) format, 2.1 Mbytes).
This animation zooms in on one of Neptune's ring arcs. The "rope-like"
structure is caused by smear, since the clumps moved significantly while
the the camera shutter was open. See the "Twisted Rope" image below.
Taken from a NASA full motion video and converted to QuickTime format.
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Images
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Related Web Sites
These sites contain more information about Neptune and its ring system.
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