Astronomy:Anthe (moon)
 Anthe is the ellipsoid in the center | |
| Discovery | |
|---|---|
| Discovered by | Cassini Imaging Team [1] |
| Discovery date | May 30, 2007 |
| Designations | |
Designation | Saturn XLIX |
| Pronunciation | /ˈænθiː/[lower-alpha 1] |
| Named after | Άνθη Anthē |
| Adjectives | Anthean /ænˈθiːən/ |
| Orbital characteristics [2] | |
| 197,700 km | |
| Eccentricity | 0.0011 |
| Orbital period | 1.05089 d |
| Average Orbital speed | 13.824 km/s |
| Inclination | 0.1° to Saturn's equator |
| Satellite of | Saturn |
| Group | Alkyonides |
| Physical characteristics | |
| Dimensions | 1.8 km [3] |
| Mean radius | 0.9 km |
| Circumference | ≈ 5.7 km |
| Surface area | 10.18 km2 |
| Volume | 3 km3 |
| Mass | 1.5×1012 kg[4] |
| Mean density | 0.5 g/cm3 |
| 0.00012 m/s2 (0.12 mm/s2) | |
| ≈ 0.56 m/s (≈ 2 km/h) | |
| Rotation period | assumed synchronous |
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.[5]
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 The published discovery was retracted a few hours later and republished the next day under the correct name of S/2007 S 5.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[1] in images taken on 30 May 2007.[2] 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.[2]
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.
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.[6][7]
References
- Notes
- ↑ This name is too new to appear in dictionaries, but the OED has the analogous rhodanthe /roʊˈdænθiː/ from the same root.
- Citations
- Sources
- "Cassini Imaging Science Team". Cassini Imaging Central Laboratory for OPerationS. http://ciclops.org/team/iss_team.php.
- Agle, D. C. (July 19, 2007). "Saturn Turns 60". Cassini Solstice Mission. JPL/NASA. http://saturn.jpl.nasa.gov/news/cassinifeatures/feature20070719/.
- Green, Daniel W. E. (July 18, 2007). "S/ 2007 S 4". IAU Circular 8857. http://www.cbat.eps.harvard.edu/iauc/08800/08857.html. Retrieved 2012-01-01.
- Hedman, M. M.; Murray, C. D.; Cooper, N. J.; Tiscareno, M. S.; Beurle, K.; Evans, M. W.; Burns, J. A. (2008-11-25). "Three tenuous rings/arcs for three tiny moons". Icarus 199 (2): 378–386. doi:10.1016/j.icarus.2008.11.001. ISSN 0019-1035. Bibcode: 2009Icar..199..378H.
- Porco C. C. (2008-09-05). "More Ring Arcs for Saturn". Cassini Imaging Central Laboratory for Operations. http://ciclops.org/view_event/90/More_Ring_Arcs_for_Saturn.
External links
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