Discovery images of Anthe |
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| Discovery | |
|---|---|
| Discovered by | CICLOPS Team [1] |
| Discovery date | May 30, 2007 |
| Orbital characteristics [2] | |
| Semi-major axis | 197,700 km |
| Eccentricity | 0.001 |
| Orbital period | 1.03650 d |
| Inclination | 0.1° to Saturn's equator |
| Satellite of | Saturn |
| Physical characteristics | |
| Mass | 5 ×1012 kg [a] |
| Mean density | unknown |
| Equatorial surface gravity | unknown |
| Rotation period | assumed synchronous |
| Axial tilt | unknown |
| Albedo | unknown |
Anthe (pron.: /ˈænθiː/ AN-thee;[b] Greek: Άνθη) is a very small natural satellite of Saturn lying between the orbits of Mimas and Enceladus. It is also known as Saturn XLIX; its provisional designation was S/2007 S 4. It is named after one of the Alkyonides; the name means flowery. It is the sixtieth confirmed moon of Saturn.[3]
It was discovered by the Cassini Imaging Team[1] in images taken on May 30, 2007.[2] Once the discovery was made, a search of older Cassini images revealed this small satellite in observations from as far back as June 2004. It was first announced on July 18, 2007.[2]
Anthe is visibly affected by a perturbing mean-longitude resonance with the much larger Mimas. This causes its osculating orbital elements to vary with an amplitude of about 20 km in semi-major axis on a timescale of about 2 Earth years. The close proximity to the orbits of Pallene and Methone suggests that these moons may form a dynamical family.
Explanatory
Citations
Sources
Media related to Anthe at Wikimedia Commons
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