Discovery | |
---|---|
Discovered by | M. R. Showalter |
Discovery date | July 16, 1990 |
Designations | |
Designation | Saturn XVIII |
Pronunciation | /ˈpæn/ |
Named after | Πάν Pān |
S/1981 S 13 | |
Adjectives | Pandean /pænˈdiːən/[1] |
Orbital characteristics[2] | |
133584.0±0.1 km | |
Eccentricity | 0.0000144±0.0000054 |
0.575050718 d (13.801217 h) | |
Inclination | 0.0001°±0.0004° |
Satellite of | Saturn |
Group | Shepherd moon of the Encke Gap |
Physical characteristics | |
Dimensions | 34.6 × 28.2 × 21.0 km (± 0.4 × 0.4 × 1.0 km)[3]: 2 |
27.4±0.6 km[3]: 2 | |
Volume | 10748 km3[3]: 8 |
Mass | (4.30±0.22)×1015 kg[3]: 3 |
Mean density | 0.400±0.031 g/cm3[3]: 3 |
0.0111–0.0169 m/s2[3]: 3 | |
0.006 km/s at longest axis to 0.007 km/s at poles | |
synchronous | |
zero | |
Albedo | 0.5 |
Temperature | ≈ 78 K |
Pan is the innermost named moon of Saturn.[4] It is a small, ravioli[5]-shaped moon approximately 35 kilometres across and 23 km wide that orbits within the Encke Gap in Saturn's A Ring. Pan is a ring shepherd and is responsible for keeping the Encke Gap free of ring particles. It is sometimes described as having the appearance of a walnut.
It was discovered by Mark R. Showalter in 1990 from analysis of old Voyager 2 probe photos and received the provisional designation S/1981 S 13 because the discovery images dated back to 1981.[6]
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