Phoebe (moon)

Phoebe
Cassini image of Phoebe. Jason crater occupies much of the upper image
Discovery
Discovered byW. H. Pickering
Discovery date18 March 1899 (from photos taken 16 August 1898)
Designations
Designation
Saturn IX
Pronunciation/ˈfbi/ FEE-bee
Named after
Φοίβη Phoíbē
AdjectivesPhoebean /fˈbən/ fee-BEE-ən
Orbital characteristics
12 960 000 km
Eccentricity0.1562415
550.564636 d
Inclination173.04° (to the ecliptic)
151.78° (to Saturn's equator)
Satellite ofSaturn
GroupNorse group
Physical characteristics
Dimensions(218.8±2.8)×(217.0±1.2)×(203.6±0.6) km
106.5±0.7 km
Mass(8.3123±0.0162)×1018 kg
Mean density
1.6428±0.0326 g/cm3
0.038–0.050 m/s2
0.102 km/s
9.2735 h (9h 16min 25s ± 3s)
152.14° (to orbit)
Albedo0.100±0.005
Temperature73(?) K
6.59±0.02

    Phoebe (/ˈfbi/ FEE-bee) is the most massive irregular satellite of Saturn with a mean diameter of 213 km (132 mi). It was discovered by William Henry Pickering on 18 March 1899 from photographic plates that had been taken by DeLisle Stewart starting on 16 August 1898 at the Boyden Station of the Carmen Alto Observatory near Arequipa, Peru. It was the first natural satellite to be discovered photographically.

    Phoebe was the first target encountered upon the arrival of the Cassini spacecraft in the Saturn system in 2004, and is thus unusually well-studied for an irregular moon of its size. Cassini's trajectory to Saturn and time of arrival were chosen to permit this flyby. After the encounter and its insertion into orbit, Cassini did not go much beyond the orbit of Iapetus.

    Phoebe is roughly spherical and has a differentiated interior. It was spherical and hot early in its history and was battered out of roundness by repeated impacts. There is some evidence that it may be a captured centaur that originated in the Kuiper belt. Phoebe is the second-largest retrograde satellite in the Solar System after Triton.