Prometheus is a moon of Saturn. It was discovered in 1980 (some time before October 25) from photos taken by the Voyager 1 probe, and was designated 1980 S 27.[1] In 1985 it was officially named after Prometheus, a Titan in Greek mythology. It is also designated Saturn XVI.[2]

This small moon is extremely elongated, measuring about 119 by 87 by 61 km. It has several ridges and valleys and a number of impact craters of about 20 km diameter are visible, but it is less cratered than nearby Pandora, Epimetheus and Janus. From its very low density and relatively high albedo, it seems likely that Prometheus is a very porous icy body. There is a lot of uncertainty in these values, however, and so this remains to be confirmed.

Prometheus acts as a shepherd satellite for the inner edge of Saturn's F Ring. Recent images from the Cassini probe show that the Promethean gravitational field creates kinks and knots in the F Ring as the moon 'steals' material from it.

The orbit of Prometheus appears to be chaotic, as a consequence of a mean motion resonance with Pandora. The most appreciable changes in their orbits occur approximately every 6.2 years [3], when the periapsis of Pandora lines up with the apoapsis of Prometheus and the moons approach to within about 1400 km. Prometheus is itsef a significant perturber of Atlas.

There is also an asteroid called 1809 Prometheus.


  1. Smith, B. A. (October 31, 1980). IAU Circular No. 3532. Retrieved on 2006-08-07.
  2. Planet and Satellite Names and Discoverers. Gazetteer of Planetary Nomenclature. USGS Astrogeology (July 21, 2006). Retrieved on 2006-08-07.
  3. Cite error: Invalid <ref> tag; no text was provided for refs named Spitale06

External links

... | Atlas | Prometheus | Pandora | ...

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