Aegaeon (moon)
 Aegaeon imaged by the Cassini spacecraft from a distance of 15238.2 km in 2010 | |
| Discovery | |
|---|---|
| Discovered by | Carolyn Porco |
| Discovery date | March 3, 2009 |
| Cassini Imaging Science Team | |
| Orbital characteristics | |
| Epoch JD 2454467.00075444 TDB | |
| 167493.665±0.004 km [1] | |
| Eccentricity | 0.00042277±0.00000004 [1] |
| 0.80812 d [2] | |
| Inclination | 0.0007°±0.6° [1] |
| (linear drift) 445.475±0.007°/day | |
| Physical characteristics | |
| Dimensions | 1.4 km × 0.5 km × 0.4 km ± 0.1 km × 0.12 km × 0.16 km[3] |
| 0.33±0.06 km[3] | |
Mean density | 0.54+0.16 −0.13 g/cm3[3] |
| Albedo | < 0.15 |
Aegaeon (/iːˈdʒiːən/ ee-JEE-ən; or as Greek Αιγαίων), also Saturn LIII (provisional designation S/2008 S 1), is a natural satellite of Saturn. It is thought to be similarly smooth as Methone.[4] It orbits between Janus and Mimas within Saturn's G Ring.
Discovery and naming
Images of Aegaeon were taken by Cassini on 15 August 2008, and its discovery was announced on 3 March 2009 by Carolyn Porco of the Cassini Imaging Science Team using the provisional designation S/2008 S 1.[2]
Aegaeon was named after Ægæon, one of the hekatonkheires, on 5 May 2009.[5]
Orbit
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Aegaeon orbits within the bright segment of Saturn's G Ring, and is probably a major source of the ring.[6] Debris knocked off Aegaeon forms a bright arc near the inner edge, which in turn spreads to form the rest of the ring. Aegaeon orbits in a 7:6 corotation eccentricity resonance with Mimas,[1] which causes an approximately 4-year oscillation of about 4 km in its semi-major axis, and a corresponding oscillation of a few degrees in its mean longitude. It orbits Saturn at an average distance of 167,500 km in 0.80812 days, at an inclination of 0.001° to Saturn's equator, with an eccentricity of 0.0002.[2]
Physical characteristics
Aegaeon is the smallest known moon of Saturn and has a highly elongated shape, measuring 1.4 km × 0.5 km × 0.4 km (0.87 mi × 0.31 mi × 0.25 mi) in size.[7] Measurements of its mass, based on its interaction with the dust particles that make up the G ring arc the moon is embedded in, suggest a density similar to that of water ice.[8] Aegaeon has the lowest albedo, below 0.15, of any Saturnian moon inward of Titan.[8] This might be due to either darker meteoric material making up the dust in the G ring or due to Aegaeon having been disrupted, stripping away its ice-rich surface and leaving the rocky inner core behind.[8]
Exploration
The Cassini spacecraft has performed four flybys of Aegaeon closer than 20,000 km, though only one has occurred since it was discovered in 2008. The closest of these pre-discovery encounters took place on 5 September 2005 at a distance of 8,517 km.[9] An encounter on 27 January 2010 at a distance 13,306 km allowed Cassini to acquire its highest resolution images of Aegaeon to-date.[8] On 19 December 2015, Cassini was unable to acquire any images from a planned close flyby.
References
- ^ a b c d Hedman, M.M.; Cooper, N.J.; Murray, C.D.; Beurle, K.; Evans, M.W.; Tiscareno, M.S.; Burns, J.A. (May 2010). "Aegaeon (Saturn LIII), a G-ring object". Icarus. 207 (1): 433–447. arXiv:0911.0171. Bibcode:2010Icar..207..433H. doi:10.1016/j.icarus.2009.10.024.
- ^ a b c IAU Circular No. 9023
- ^ a b c Thomas, P. C.; Burns, J. A.; Tiscareno, M. S.; Hedman, M. M.; et al. (2013). "Saturn's Mysterious Arc-Embedded Moons: Recycled Fluff?" (PDF). 44th Lunar and Planetary Science Conference. p. 1598. Retrieved 2013-05-21.
{{cite conference}}: Unknown parameter|booktitle=ignored (|book-title=suggested) (help) - ^ Battersby, S. (2013-05-17). "Saturn's egg moon Methone is made of fluff". www.newscientist.com. New Scientist. Retrieved 2013-05-21.
- ^ Jennifer Blue, Saturnian Satellite Named Aegaeon, USGS Astrogeology Hot Topics, 5 May 2009
- ^ Petite Moon, CICLOPS, 29 May 2009
- ^ Thomas, P.C.; Burns, J.A.; Hedman, M.; Helfenstein, P.; Morrison, S.; Tiscareno, M.S.; Veverka, J. (2013). "The inner small satellites of Saturn: A variety of worlds" (PDF). Icarus. 226 (1): 999–1019. Bibcode:2013Icar..226..999T. doi:10.1016/j.icarus.2013.07.022. Retrieved 2 December 2015.
- ^ a b c d Hedman, M.M.; Burns, J.A.; Thomas, P.C.; Tiscareno, M.S.; Evans, M.W. (2011). Physical Properties of the small moon Aegaeon (Saturn LIII) (PDF). European Planetary Space Conference. Icarus. Vol. 6. Retrieved 2 December 2015.
- ^ Planetary Society Cassini Timeline
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