C/2014 M1 PANSTARRS
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Comet C/2014 M1 was discovered on 24 June 2014 with Pan-STARRS 1 telescope (Haleakala), that is more than a year before its perihelion passage. This comet was rather rarely observed during four oppositions until 7 March 2017.
Comet had its closest approach to the Earth on 17 June 2015 (4.603 au), more than two months before perihelion passage.
Solution given here are based on data spanning over 2.70 yr in a range of heliocentric distances: 6.37 au – 5.577 au (perihelion) – 6.86 au.
This Oort spike comet suffers small planetary perturbations during its passage through the planetary system; these perturbations lead to a more tight future orbit (see future barycentric orbits).
Comet had its closest approach to the Earth on 17 June 2015 (4.603 au), more than two months before perihelion passage.
Solution given here are based on data spanning over 2.70 yr in a range of heliocentric distances: 6.37 au – 5.577 au (perihelion) – 6.86 au.
This Oort spike comet suffers small planetary perturbations during its passage through the planetary system; these perturbations lead to a more tight future orbit (see future barycentric orbits).
| solution description | ||
|---|---|---|
| number of observations | 86 | |
| data interval | 2014 06 24 – 2017 03 07 | |
| data type | perihelion within the observation arc (FULL) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 6.37 au – 5.58 au (perihelion) – 6.86 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 | 165 | |
| RMS [arcseconds] | 0.38 | |
| 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] | 189.15 – 191.68 – 194.14 | |
| next perihelion distance [au] | 5.5646 – 5.5653 – 5.5659 | |
| next aphelion distance [103 au] | 10.3 – 10.4 – 10.6 | |
| time interval to next perihelion [Myr] | 0.369 – 0.376 – 0.384 | |
| 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] | 189.12 – 191.65 – 194.11 | |
| next perihelion distance [au] | 5.56476 – 5.56536 – 5.56591 | |
| next aphelion distance [103 au] | 10.3 – 10.4 – 10.6 | |
| time interval to next perihelion [Myr] | 0.369 – 0.376 – 0.384 | |
| percentage of VCs with qnext < 10 | 100 | |