C/2017 E3 PANSTARRS
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Comet C/2017 E3 was discovered on 7 March 2017 with Pan-STARRS 1 telescope (Haleakala), that is about 3 months before its perihelion passage. Later, it was found on a series of earlier images going back to December 2013. This comet was observed until 20 June 2020.
Comet had its closest approach to the Earth on 24 April 2017 (3.480 au), about 1.5 month after discovery and more than a month before its perihelion passage.
Solutions given here are based on data spanning over 6.51 yr in a range of heliocentric distances: 10.28 au 5.915 au (perihelion) 9.53 au (July 2023).
This Oort spike comet suffers moderate planetary perturbations during its passage through the planetary system; these perturbations lead to escape the comet from the planetary zone on a hyperbolic orbit (see future barycentric orbits).
See also Królikowska and Dones 2023.
| solution description | ||
|---|---|---|
| number of observations | 152 | |
| data interval | 2013 12 14 – 2017 05 26 | |
| data arc selection | data generally limited to pre-perihelion (PRE) | |
| range of heliocentric distances | 10.28 au – 5.9au | |
| 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 | 300 | |
| RMS [arcseconds] | 0.21 | |
| 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] | 38.97 – 39.98 – 40.95 | |
| previous perihelion distance [au] | 760 – 870 – 980 | |
| previous aphelion distance [103 au] | 48.1 – 49.2 – 50.3 | |
| time interval to previous perihelion [Myr] | 3.36 – 3.51 – 3.67 | |
| percentage of VCs with qprev > 20 | 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.
| 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] | 41.62 – 42.92 – 44.24 | |
| previous perihelion distance [au] | 9.16 – 9.69 – 10.3 | |
| previous aphelion distance [103 au] | 45.2 – 46.6 – 48 | |
| time interval to previous perihelion [Myr] | 3.38 – 3.54 – 3.71 | |
| percentage of VCs with qprev < 10 | 75 | |
| percentage of VCs with 10 < qprev < 20 | 25 | |