Discovery [1] | |
---|---|
Discovered by | Alex R. Gibbs |
Discovery site | Mount Lemmon Survey |
Discovery date | 19 September 2011 |
Orbital characteristics [2] | |
Epoch | 5 June 2013 (JD 2456448.5) |
Observation arc | 8.26 years |
Earliest precovery date | 29 September 2010 |
Number of observations | 148 |
Aphelion | 10.409 AU |
Perihelion | 6.894 AU |
Semi-major axis | 8.652 AU |
Eccentricity | 0.20315 |
Orbital period | 25.448 years |
Inclination | 2.679° |
218.89° | |
Argument of periapsis | 193.37° |
Mean anomaly | 342.76° |
Last perihelion | 24 August 2014 |
Next perihelion | 2 November 2039 [3] |
TJupiter | 3.124 |
Earth MOID | 5.903 AU |
Jupiter MOID | 1.885 AU |
Physical characteristics [2] [4] [5] | |
Mean diameter | < 8.0 km (5.0 mi) |
(V–R) = 0.11±0.09 (R–I) = 0.26±0.06 | |
Comet total magnitude (M1) | 7.1 |
Comet nuclear magnitude (M2) | 11.5 |
P/2011 S1 (Gibbs) is a periodic comet or an active centaur with a 25-year orbit around the Sun.
American astronomer, Alex R. Gibbs, reported the discovery of a new object from CCD images obtained from the 1.5 m (4.9 ft) reflector telescope from the Mount Lemmon Survey on 19 September 2011. [1] Precovery images show that the object produced comet-like activity as early as September 2010, a year before its discovery. [5]