S/2004 S 6
 object seen on 21 June, 2005 by Cassini, thought to be S/2004 S 6 | |
| Discovery | |
|---|---|
| Discovered by | Cassini Imaging Science Team Archived 2011-05-20 at the Wayback Machine |
| Discovered on | 28 October, 2004 |
| Orbital characteristics[1] | |
| Epoch 13 April 2005 (JD 2453474.1) | |
| Semimajor axis | 140,134 ± 2 km |
| Eccentricity | 0.00200 ± 0.00004 |
| Revolution period | 0.6180116 ± 0.0000004 d |
| Inclination to Saturn's equator |
0.002 ± 0.001° |
| Is a satellite of | Saturn |
| Physical characteristics | |
| Mean diameter | < 5 km [1] |
| Rotation period | probably synchronous |
| Axial tilt | unknown |
| Albedo | unknown |
| Atmosphere | none |
S/2004 S 6 is the designation of a dusty object seen orbiting Saturn very close to the F ring. It is not clear whether it is only a clump of dust, or if there is a solid small moon at its core.
It was first seen by scientists in pictures taken by the Cassini-Huygens probe on October 28, 2004, and announced on 8 November that year.[2] It appears to be the best tracked object in this area with at least five possible sightings in the period till late 2005. In comparison, two objects in the F ring's area (S/2004 S 3 and S/2004 S 4) that were first seen months earlier have not been found again. An imaging sequence covering an entire orbital period at 4 km resolution taken on 15 November 2004, soon after it was discovered did not find the object, while it has been seen again later. The lighting conditions in S/2004 S 6's part of the orbit were different during these two sightings. The discovery was made when the area was strongly backlit by the sun. S/2004 S 6's visibility may be primarily due to a diffuse cloud of fine dust that is much brighter in forward scattered light (the conditions of the discovery image), and that the solid core (if any) is small.[1]
S/2004 S 6 has been seen both inside and outside the main F ring, and its orbit must cross the ring. Calculations show that the object periodically plows through the ring material, coming within 1.5 km of the densest core e.g. on 9 April, 2005. It has been suggested that a spiral structure in the thinnest material around the F ring may have been a result of this.[3]
The dusty halo seen in pictures is big, being around 2000 km in length. The solid object, if any, would be no bigger than 3−5 km in diameter based on brightness.
References[change | change source]
- ↑ 1.0 1.1 1.2 Spitale, J. N.; et al. (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations". The Astronomical Journal. 132 (2): 692–710. Bibcode:2006AJ....132..692S. doi:10.1086/505206. S2CID 26603974.
- ↑ IAUC 8432: Satellites and Rings of Saturn 2004 November 8 (claiming recovery of S/2004 S 3 on 17 October, 2004, in conflict with the later (2006) Spitale et al.)
- ↑ Charnoz, S.; et al. (2005). "Cassini Discovers a Kinematic Spiral Ring Around Saturn". Science. 310 (5752): 1300–1304. Bibcode:2005Sci...310.1300C. doi:10.1126/science.1119387. PMID 16311328. S2CID 6502280.