Discovery | |
---|---|
Discovered by | CICLOPS Team [1][2] |
Discovery date | June 21, 2004 |
Orbital characteristics [3] | |
~140,100 km | |
Eccentricity | unknown, small |
~0.618 d | |
Inclination | unknown, small |
Satellite of | Saturn |
Group | F Ring |
Physical characteristics | |
~2 km | |
probably synchronous | |
unknown | |
Albedo | unknown |
S/2004 S 4 is the provisional designation of an unconfirmed object seen orbiting Saturn within the inner strand of the F ring on June 21, 2004. It was spotted while J. N. Spitale was trying to confirm the orbit of another provisional object, S/2004 S 3, that was seen 5 hours earlier just exterior to the F ring.[2] The announcement was made on September 9, 2004.[4]
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 November 15, 2004, failed to recover the object. The sequence should have been easily capable of detecting a moon of similar size, suggesting it to simply be a transient clump. An approximate linkage could be made of S/2004 S 3 to S/2004 S 4, and matched to two other detected clumps on other dates, but considering its non-detection in November, their relation is probably coincidental.[5]
An interpretation where S/2004 S 3 and S/2004 S 4 are or were a single object on a F-ring crossing orbit is also possible.[4] 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 S 4 would be 3–5 km in diameter based on brightness.
PGJ
was invoked but never defined (see the help page).