Anthe (moon)
Anthe is the object in the center. | |
| Discovery | |
|---|---|
| Discovered by | Cassini Imaging Team |
| Discovery date | May 30, 2007 |
| Designations | |
Designation | Saturn XLIX |
| Pronunciation | /ˈænθiː/ |
Named after | Άνθη Anthē |
| Adjectives | Anthean /ænˈθiːən/ |
| Orbital characteristics | |
| Epoch 2007 May 30 04:02:02.511 UTC (JED 2454250.66883907) | |
| 197655±26 km | |
| Eccentricity | 0.0012±0.0008 |
| 1.036517 d | |
Average orbital speed | 13.824 km/s |
| Inclination | 0.017°±0.004° (to Saturn's equator) |
| Satellite of | Saturn |
| Physical characteristics | |
| 0.75–2.4 km | |
Mean density | 0.5 g/cm3 (assumed) |
| assumed synchronous | |
| assumed zero | |
| Albedo | 0.25–1 (geometric) |
Anthe /ˈænθiː/ 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.
The designation S/2007 S 4 was also accidentally and incorrectly used for a different Saturnian satellite discovered later. The published discovery was retracted a few hours later and republished the next day under the correct name of S/2007 S 5.
It was discovered by the Cassini Imaging Team in images taken on 30 May 2007. Once the discovery was made, a search of older Cassini images revealed it in observations from as far back as June 2004. It was first announced on 18 July 2007.
Anthe is visibly affected by a perturbing 10:11 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.
The ratio of Anthe's medium axis to its long axis is ≈0.7, and the ratio of its short axis to its medium axis is ≈0.95. This implies that it has a similar shape to Methone.
Material blasted off Anthe by micrometeoroid impacts is thought to be the source of the Anthe Ring Arc, a faint partial ring about Saturn co-orbital with the moon first detected in June 2007.