Distant Phoebe

Voyager 2 took this photo of Saturn's outer satellite, Phoebe, on September 4, 1981, from 2.2 million kilometers (1.36 million miles)
away. The photo shows that Phoebe is about 200 kilometers (120 miles) in diameter, about twice the size of previous Earth-based
measurements; and dark, with five percent reflectivity--much darker than any other Saturnian satellite.

That, and information
from Earth-based observations, indicates Phoebe is almost certainly a captured asteroid, and did not form in the original Saturn
nebula as Saturn's other satellites did. Phoebe is the only Saturnian satellite that does not always show the same face to Saturn: Its
orbital period is 550 days. Its rotation period (length of day), determined from Voyager 2 observations, is nine to ten hours.


Other ground-based observations that indicate that Phoebe is a captured asteroid: It orbits Saturn in the ecliptic plane (the plane in
which Earth and most other planets orbit the Sun), rather than in Saturn's equatorial plane as the other Saturn satellites do. And
Phoebe's orbit is retrograde--in the direction opposite to that of the other satellites.



For a high resolution image, click here.