C/1978 R3 Machholz
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Comet C/1978 R3 was discovered on 12 September 1978 by Donald E. Machholz (Mt Loma Prita, California, USA), that is about a month after its perihelion passage.This comet was last observed on late September 1979.
Comet had its closest approach to the Earth on 15 October 1978 (1.510 au), about a month after discovery.
Solution given here is based on data spanning over 1.03 yr in a range of heliocentric distances from 1.82 au to 4.89 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 also Królikowska 2020.
Comet had its closest approach to the Earth on 15 October 1978 (1.510 au), about a month after discovery.
Solution given here is based on data spanning over 1.03 yr in a range of heliocentric distances from 1.82 au to 4.89 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 also Królikowska 2020.
| solution description | ||
|---|---|---|
| number of observations | 52 | |
| data interval | 1978 09 14 – 1979 09 25 | |
| data type | observed only after perihelion (POST) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 1.82 au – 4.89au | |
| detectability of NG effects in the comet's motion | NG effects not determinable | |
| type of model of motion | GR - gravitational orbit | |
| data weighting | NO | |
| number of residuals | 101 | |
| RMS [arcseconds] | 1.50 | |
| orbit quality class | 1b | |
| 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] | 250.40 – 286.61 – 322.34 | |
| next perihelion distance [au] | 1.764 – 1.7669 – 1.7684 | |
| next aphelion distance [103 au] | 6.2 – 7 – 8 | |
| time interval to next perihelion [Myr] | 0.17 – 0.21 – 0.25 | |
| 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] | 250.39 – 286.60 – 322.33 | |
| next perihelion distance [au] | 1.7613 – 1.7641 – 1.7657 | |
| next aphelion distance [103 au] | 6.2 – 7 – 8 | |
| time interval to next perihelion [Myr] | 0.17 – 0.21 – 0.25 | |
| percentage of VCs with qnext < 10 | 100 | |