C/2012 A1 PANSTARRS
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Comet C/2012 A1 was discovered on 2 January 2012, that is 1.9 yr before perihelion passage, and next observed 3.2 yr during four oppositions in a range of heliocentric distances: 8.73 au – 7.603 au (perihelion) – 8.12 au.
Comet had its closest approach to the Earth on 22 December 2013 (6.642 au, about three weeks after perihelion passage, see figure).
C/2012 A1 suffers a slight planetary perturbations during its passage through the planetary system.
See also Królikowska and Dybczyński 2017.
Comet had its closest approach to the Earth on 22 December 2013 (6.642 au, about three weeks after perihelion passage, see figure).
C/2012 A1 suffers a slight planetary perturbations during its passage through the planetary system.
See also Królikowska and Dybczyński 2017.
| solution description | ||
|---|---|---|
| number of observations | 330 | |
| data interval | 2012 01 02 – 2015 03 09 | |
| data type | perihelion within the observation arc (FULL) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 8.73 au – 7.60 au (perihelion) – 8.12 au | |
| detectability of NG effects in the comet's motion | NG effects not determinable | |
| type of model of motion | GR - gravitational orbit | |
| data weighting | YES | |
| number of residuals | 653 | |
| RMS [arcseconds] | 0.40 | |
| orbit quality class | 1a+ | |
| next orbit statistics, both Galactic and stellar perturbations were taken into account | ||
|---|---|---|
| no. of returning VCs in the swarm | 5001 | * |
| no. of escaping VCs in the swarm | 0 | |
| no. of hyperbolas among escaping VCs in the swarm | 0 | |
| next reciprocal semi-major axis [10-6 au-1] | 157.51 – 158.74 – 159.97 | |
| next perihelion distance [au] | 7.5822 – 7.5831 – 7.5839 | |
| next aphelion distance [103 au] | 12.49 – 12.59 – 12.69 | |
| time interval to next perihelion [Myr] | 0.494 – 0.499 – 0.505 | |
| percentage of VCs with qnext < 10 | 100 | |
Time distribution of positional observations with corresponding heliocentric (red curve) and geocentric (green curve) distance at which they were taken. The horizontal dotted line shows the perihelion distance for a given comet whereas vertical dotted line — the moment of perihelion passage.
| next orbit statistics, here only the Galactic tide has been included | ||
|---|---|---|
| no. of returning VCs in the swarm | 5001 | * |
| no. of escaping VCs in the swarm | 0 | |
| no. of hyperbolas among escaping VCs in the swarm | 0 | |
| next reciprocal semi-major axis [10-6 au-1] | 157.49 – 158.72 – 159.95 | |
| next perihelion distance [au] | 7.57912 – 7.57963 – 7.58013 | |
| next aphelion distance [103 au] | 12.5 – 12.59 – 12.69 | |
| time interval to next perihelion [Myr] | 0.494 – 0.5 – 0.505 | |
| percentage of VCs with qnext < 10 | 100 | |