C/2020 K2 PanSTARRS
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Comet C/2020 K2 was discovered on 21 May 2020, about 2.5 months before its perihelion passage and was observed to 28 June 2021.
Solutions given here are based on data span over 1.10 yr in a range of heliocentric distances: 8.89 au – 8.88 au (perihelion) – 9.08 au.
This comet entered the planetary zone having original semimajor axis of about 8,000 au and suffers small planetary perturbations during its passage through the planetary system that lead to a bit tight future orbit (semimajor axis of about 5,000 au).
Solutions given here are based on data span over 1.10 yr in a range of heliocentric distances: 8.89 au – 8.88 au (perihelion) – 9.08 au.
This comet entered the planetary zone having original semimajor axis of about 8,000 au and suffers small planetary perturbations during its passage through the planetary system that lead to a bit tight future orbit (semimajor axis of about 5,000 au).
| solution description | ||
|---|---|---|
| number of observations | 87 | |
| data interval | 2020 05 21 – 2021 06 28 | |
| data type | perihelion within the observation arc (FULL) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 8.89 au – 8.88 au (perihelion) – 9.08 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 | 166 | |
| RMS [arcseconds] | 0.23 | |
| orbit quality class | 1a | |
| previous 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 | |
| previous reciprocal semi-major axis [10-6 au-1] | 115.95 – 118.60 – 121.30 | |
| previous perihelion distance [au] | 8.977 – 8.986 – 8.996 | |
| previous aphelion distance [103 au] | 16.5 – 16.9 – 17.2 | |
| time interval to previous perihelion [Myr] | 0.748 – 0.773 – 0.8 | |
| percentage of VCs with qprev < 10 | 100 | |
| previous 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 | |
| previous reciprocal semi-major axis [10-6 au-1] | 115.95 – 118.60 – 121.30 | |
| previous perihelion distance [au] | 8.98 – 8.989 – 8.999 | |
| previous aphelion distance [103 au] | 16.5 – 16.9 – 17.2 | |
| time interval to previous perihelion [Myr] | 0.748 – 0.773 – 0.8 | |
| percentage of VCs with qprev < 10 | 100 | |