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Moon of Saturn From Wikipedia, the free encyclopedia
Pandora is an inner satellite of Saturn. It was discovered in 1980 from photos taken by the Voyager 1 probe and was provisionally designated S/1980 S 26.[5] In late 1985, it was officially named after Pandora from Greek mythology.[6] It is also designated as Saturn XVII.[7]
Discovery | |
---|---|
Discovered by | Stewart A. Collins D. Carlson Voyager 1 |
Discovery date | October, 1980 |
Designations | |
Designation | Saturn XVII |
Pronunciation | /pænˈdɔːrə/ |
Named after | Πανδώρα Pandōra |
Adjectives | Pandoran[1] |
Orbital characteristics [2] | |
Epoch December 31, 2003 (JD 2453005.5) | |
141720±10 km | |
Eccentricity | 0.0042 |
0.628504213 d | |
Inclination | 0.050°±0.004° to Saturn's equator |
Satellite of | Saturn |
Group | Possible outer shepherd moon of the F Ring |
Physical characteristics | |
Dimensions | 103.0 × 79.0 × 63.0 km (± 0.6 × 0.6 × 0.4 km)[3]: 2 |
80.0±0.6 km[3]: 2 | |
Volume | 268990±860 km3[4]: 4 |
Mass | (1.357±0.002)×1017 kg[b] |
Mean density | 0.5045±0.0017 g/cm3[4]: 4 |
0.0022–0.0061 m/s2[3]: 3 | |
0.019 km/s at longest axis to 0.024 km/s at poles | |
synchronous | |
zero | |
Albedo | 0.6 |
Temperature | ≈ 78 K |
Pandora was thought to be an outer shepherd satellite of the F Ring. However, recent studies indicate that it does not play such a role, and that only Prometheus, the inner shepherd, contributes to the confinement of the narrow ring.[8][9] It is more heavily cratered than nearby Prometheus and has at least two large craters 30 kilometres (19 mi) in diameter. The majority of craters on Pandora are shallow as a result of being filled with debris. Ridges and grooves are also present on the moon's surface.[10]
The orbit of Pandora appears to be chaotic as a consequence of a series of four 118:121 mean-motion resonances with Prometheus.[11] The most appreciable changes in their orbits occur approximately every 6.2 years,[2] when the periapsis of Pandora lines up with the apoapsis of Prometheus and the moons approach to within about 1,400 kilometres (870 mi). Pandora also has a 3:2 mean-motion resonance with Mimas.[2]
From its very low density and relatively high albedo, it seems likely that Pandora is a very porous icy body. However, there is much uncertainty in these values, so this remains to be confirmed.
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