Prometheus as imaged by Cassini on Jan 27, 2010 from a distance of 36,000 km.
|A faint stream of material appears to connect
the F ring to Prometheus, the white blob at the bottom, in this
image taken by Cassini in Jul 2004.
Prometheus and Pandora act as shepherd moons for the inner edge of Saturn's F-ring. Prometheus is extremely elongated and has a number of ridges and valleys on its northern side. Although craters up to 20 km (12 mi) wide mark its icy surface, it appears to be less heavily cratered than its neighboring moons Pandora, Janus, and Epimetheus. Its low estimated density suggests that it may be a porous, icy body.
|discovery||1980, by S. Collins et al|
|semimajor axis||139,353 km (85,590 mi)|
|diameter||119 × 87 × 61 km (74 × 54 × 38 mi)|
|mean density||0.5 g/cm3|
|escape velocity||0.019 km/s (68 km/h, 43 mph)|
|orbital period||0.613 days (14 h 43 min)|
Prometheus is a volcano on Io known as the Jovian moon's "Old Faithful." Prometheus has been active during every observation of it since it was first seen by Voyager 1, though its plume, which is 80 km tall, has migrated about 85 km to the west.
See also Project Prometheus.