S/2004 S 3

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S/2004 S 3
Image:S2004 S 3 - PIA06115.png
Discovery image of S/2004 S 3
Discovery
Discovered by Carl Murray / Cassini Imaging Science Team
Discovered on 21 June 2004
Orbital characteristics
Semimajor axis 140,100 − 140,600 km [1][2][3]
Eccentricity < 0.002 [4]
Orbital period 0.62 d
Inclination close to zero
Is a satellite of Saturn
Physical characteristics
Mean diameter 3-5 km
Rotation period probably synchronous
Axial tilt unknown
Albedo unknown
Atmosphere none

S/2004 S 3 is the provisional designation of an object seen orbiting Saturn just beyond the outer strand of the F ring on 21 June 2004. It was first seen by Carl Murray of the Cassini Imaging Science Team in images taken by the Cassini-Huygens probe on June 21, 2004[3], and announced on September 9, 2004 [5].

Despite later attempts to recover it, it has not been reliably sighted since. Notably, an imaging sequence covering an entire orbital period at 4 km resolution taken on 15 November 2004 failed to recover the object. This suggests that it was a temporary clump of material that had disappeared by that time [1].

Another object, S/2004 S 4, was sighted nearby 5 hours later, but this time just inside the F Ring. Because of the differing localisation the second object was given a fresh designation, although their interpretation as a single object on a F-ring crossing orbit is also possible [5]. Such an object might also be orbiting at a slightly different inclination to the F ring, thereby not actually passing through the ring material despite being seen both radially inward and outward of it.

If a solid object after all, S/2004 S3 would be 3−5 km in diameter based on brightness, and might be a shepherd satellite for the outer edge of Saturn's F ring.

[edit] References

  1. ^ a b J.N. Spitale et al (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations". The Astronomical Journal 132: 692. 
  2. ^ IAUC 8432
  3. ^ a b Cassini Discovers Ring and One, Possibly Two, Objects at Saturn JPL news release (2004)
  4. ^ Based on above semimajor axis range, and Spitale et al (2006)
  5. ^ a b IAUC 8401

[edit] External links


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