C/2007 U1 LINEAR
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Comet C/2007 U1 was discovered on 19 October 2007 by LINEAR project, 9.5 months before its perihelion passage.
C/2007 U1 was observed 2.1 yr during three oppositions in a range of heliocentric distances: 4.28 au – 3.329 au (perihelion) – 5.36 au.
Comet had its closest approach to the Earth on 21 October 2008 (2.424 au, 2.5 months after perihelion).
This comet suffers small planetary perturbations during its passage through the planetary system that lead to a less tight orbit with semimajor axis larger than 10,000 au.
See also Królikowska and Dybczyński 2017.
C/2007 U1 was observed 2.1 yr during three oppositions in a range of heliocentric distances: 4.28 au – 3.329 au (perihelion) – 5.36 au.
Comet had its closest approach to the Earth on 21 October 2008 (2.424 au, 2.5 months after perihelion).
This comet suffers small planetary perturbations during its passage through the planetary system that lead to a less tight orbit with semimajor axis larger than 10,000 au.
See also Królikowska and Dybczyński 2017.
| solution description | ||
|---|---|---|
| number of observations | 896 | |
| data interval | 2007 10 19 – 2009 11 18 | |
| data type | perihelion within the observation arc (FULL) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 4.28 au – 3.33 au (perihelion) – 5.36 au | |
| type of model of motion | NS - non-gravitational orbits for standard g(r) | |
| data weighting | YES | |
| number of residuals | 1774 | |
| RMS [arcseconds] | 0.41 | |
| 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] | 57.37 – 66.22 – 85.35 | |
| next perihelion distance [au] | 21 – 31 – 260 | |
| next aphelion distance [103 au] | 23 – 30 – 35 | |
| time interval to next perihelion [Myr] | 1.44 – 1.54 – 1.69 | |
| percentage of VCs with qnext < 10 | 2 | |
| percentage of VCs with 10 < qnext < 20 | 1 | |
| percentage of VCs with qnext > 20 | 97 | |
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] | 69.80 – 74.41 – 78.97 | |
| next perihelion distance [au] | 2.74 – 2.84 – 2.92 | |
| next aphelion distance [103 au] | 25.3 – 26.9 – 28.7 | |
| time interval to next perihelion [Myr] | 1.42 – 1.56 – 1.71 | |
| percentage of VCs with qnext < 10 | 100 | |