C/2022 T1 Lemmon
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Comet C/2022 T1 was discovered on 3 October 2022 with the Mt. Lemmon Survey, that is a year and more than four months before its perihelion passage.
Comet had its closest approach to the Earth on 23 April 2024 (2.51 au), about two months after its perihelion passage.
GR solution given here is based on data span over 1.77 yr in a range of heliocentric distances: 5.60 au – 3.44 au (perihelion) – 3.69 au.
This Oort spike comet suffers smalll planetary perturbations during its passage through the planetary system that lead to escape this comet from the solar system on a hyperbolic orbit.
Comet had its closest approach to the Earth on 23 April 2024 (2.51 au), about two months after its perihelion passage.
GR solution given here is based on data span over 1.77 yr in a range of heliocentric distances: 5.60 au – 3.44 au (perihelion) – 3.69 au.
This Oort spike comet suffers smalll planetary perturbations during its passage through the planetary system that lead to escape this comet from the solar system on a hyperbolic orbit.
| solution description | ||
|---|---|---|
| number of observations | 626 | |
| data interval | 2022 10 03 – 2024 07 11 | |
| data type | perihelion within the observation arc (FULL) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 5.6 au – 3.44 au (perihelion) – 3.69 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 | 1241 | |
| RMS [arcseconds] | 0.43 | |
| orbit quality class | 1a | |
| next orbit statistics, both Galactic and stellar perturbations were taken into account | ||
|---|---|---|
| no. of returning VCs in the swarm | 0 | |
| no. of escaping VCs in the swarm | 5001 | |
| no. of hyperbolas among escaping VCs in the swarm | 5001 | * |
| next reciprocal semi-major axis [10-6 au-1] | -307.72 – -306.69 – -305.66 | |
| next perihelion distance [au] | 8.088 – 8.106 – 8.124 | |
| synchronous stop epoch [Myr] | 0.988 | S |
| 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_g orbit statistics, here only the Galactic tide has been included | ||
|---|---|---|
| no. of returning VCs in the swarm | 0 | |
| no. of escaping VCs in the swarm | 5001 | |
| no. of hyperbolas among escaping VCs in the swarm | 5001 | * |
| next reciprocal semi-major axis [10-6 au-1] | -307.64 – -306.61 – -305.58 | |
| next perihelion distance [au] | 9.09 – 9.112 – 9.135 | |
| synchronous stop epoch [Myr] | 1.04 | S |
| percentage of VCs with qnext < 10 | 100 | |