Janus, with Saturn in the background, seen by Cassini's narrow-angle camera at a distance of about 145,000 km (90,000 mi) and a Sun-Janus-spacecraft angle of 62°. The image was taken using a filter sensitive to wavelengths of infrared light centered at 930 nm. Image scale is 871 m (2,858 ft) per pixel.
Janus is an inner moon of Saturn. It was discovered on Dec 15, 1966, by Audouin Dollfus and is also known as Saturn X. It is nearly co-orbital (shares its orbit) with Epimetheus and is located between Saturn's F- and G-rings. Because Janus and Epimetheus differ in their orbital radii by only 50 km, their orbital velocities are very nearly equal and the lower, faster one gradually catches up and overtakes the other. As the moons approach each other they exchange a small amount of momentum as a result of which the lower one is boosted into a higher orbit while the higher one drops to a lower orbit. This exchange of places happens about once every four years.
Although Dollfus is credited with the discovery of Janus, it is not certain whether the object he saw was Janus or Epimetheus and his observations led to a spurious orbit. (Walker discovered it independently but his telegram arrived a few hours after that of Dollfus.) Larson and Fountain determined in 1978 that there are two moons at about 151,000 km from Saturn – a fact confirmed in 1980 by Voyager 1.
Janus is potato-shaped and extensively cratered, with several craters larger than 30 km (19 mi), but has few linear features. Its surface looks as though it has been smoothed by some process. Like Pandora and Telesto, Janus may be covered with a mantle of fine dust-sized, icy material.
|discovery||1966, by Audouin Dollfus|
|semimajor axis||151,460 km (94,130 mi)|
|diameter||193 × 173 × 137 km
(120 × 108 × 85 mi)
|mean density||0.6 g/cm3|
|surface gravity||0.014 m/s2|
|orbital period||0.695 day (16 h 41 min)|