Discovery | |
---|---|
Discovered by | Carolyn Porco |
Discovery date | March 3, 2009 |
Cassini Imaging Science Team | |
Designations | |
Designation | Saturn LIII |
Pronunciation | /iːˈdʒiːɒn/[1] |
Named after | Αιγαίων Aigaiōn |
Adjectives | Aegaeonian /iːdʒiːˈoʊniən/[2] |
Orbital characteristics | |
Epoch JD 2454467.00075444 TDB | |
167493.665±0.004 km[3] | |
Eccentricity | 0.00042277±0.00000004[3] |
0.80812 d[4] | |
Inclination | 0.0007°±0.6°[3] |
Satellite of | Saturn |
Group | Source of the G Ring |
Physical characteristics | |
Dimensions | 1.40 × 0.50 × 0.40 km (± 0.10 × 0.12 × 0.16 km)[5]: 2 |
0.66±0.12 km[5]: 2 | |
Volume | 0.15 km3[a] |
Mass | (7.82±3.00)×1010 kg[5]: 3 |
Mean density | 0.539±0.140 g/cm3[5]: 3 |
0.009–0.013 mm/s2[5]: 3 (0.9–1.3 micro-g) | |
0.001 km/s at longest axis to 0.002 km/s at poles | |
assumed synchronous | |
Albedo | < 0.15 |
Aegaeon /iːˈdʒiːɒn/, or Saturn LIII (provisional designation S/2008 S 1), is a natural satellite of Saturn. It has an extremely elongated shape whose surface is thought to be similarly smooth as Methone.[6] It orbits between Janus and Mimas within Saturn's G Ring.
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