Anthe is the ellipsoid 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 | |
Semi-major axis | 197,700 km |
Eccentricity | 0.0011 |
Orbital period (sidereal) | 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 |
Mean radius | 0.9 km |
Circumference | ≈ 5.7 km |
Surface area | 10.18 km |
Volume | 3 km |
Mass | 1.5×10 kg |
Mean density | 0.5 g/cm |
Surface gravity | 0.00012 m/s (0.12 mm/s) |
Escape velocity | ≈ 0.56 m/s (≈ 2 km/h) |
Synodic 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.
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 The published discovery was retracted a few hours later and republished the next day under the correct name of S/2007 S 5.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.
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.
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. Archived from the original on 2011-05-20. Retrieved 2012-01-01.
- Agle, D. C. (July 19, 2007). "Saturn Turns 60". Cassini Solstice Mission. JPL/NASA. Archived from the original on February 20, 2012. Retrieved 2012-01-01.
- Green, Daniel W. E. (July 18, 2007). "S/ 2007 S 4". IAU Circular. 8857. 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. Bibcode:2009Icar..199..378H. doi:10.1016/j.icarus.2008.11.001. ISSN 0019-1035.
- Porco C. C.; et al. (2008-09-05). "More Ring Arcs for Saturn". Cassini Imaging Central Laboratory for Operations. Archived from the original on 2008-10-10. Retrieved 2008-09-05.
External links
Listen to this article (1 minute) This audio file was created from a revision of this article dated 16 January 2010 (2010-01-16), and does not reflect subsequent edits.(Audio help · More spoken articles)Media related to Anthe at Wikimedia Commons
- From Dark Obscurity... A Tiny New Saturnian Moon Comes To Light Archived 2011-02-02 at the Wayback Machine
Moons of Saturn | |||||||
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Listed in approximate increasing distance from Saturn | |||||||
Ring moonlets | |||||||
Ring shepherds | |||||||
Other inner moons | |||||||
Alkyonides | |||||||
Large moons (with trojans) | |||||||
Inuit group (13) |
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Gallic group (7) | |||||||
Norse group (100) |
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Outlier prograde irregular moons |
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Saturn | |
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