C/2021 T2 Fuls
more info
Comet C/2021 T2 was discovered on 2 October 2021 by Mt. Lemmon Survey, that is about eight months before its perihelion passage. this comet was observed only until 25 February 2022.
Comet had its closest approach to the Earth on 6 July 2022 (1.14 au), about one month after its perihelion passage.
Therefore, the GR solution given here is based on preperihelion data span over 0.400 yr in a range of heliocentric distances from 3.52 au to 1.96 au.
This Oort spike comet suffers tiny planetary perturbations during its passage through the planetary system that likely lead to escape this comet from the solar system on a marginally hyperbolic orbit.
Comet had its closest approach to the Earth on 6 July 2022 (1.14 au), about one month after its perihelion passage.
Therefore, the GR solution given here is based on preperihelion data span over 0.400 yr in a range of heliocentric distances from 3.52 au to 1.96 au.
This Oort spike comet suffers tiny planetary perturbations during its passage through the planetary system that likely lead to escape this comet from the solar system on a marginally hyperbolic orbit.
| solution description | ||
|---|---|---|
| number of observations | 186 | |
| data interval | 2021 10 02 – 2022 02 25 | |
| data type | observed only before perihelion (PRE) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 3.52 au – 1.96au | |
| 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 | 360 | |
| RMS [arcseconds] | 0.42 | |
| orbit quality class | 2a | |
| previous orbit statistics, both Galactic and stellar perturbations were taken into account | ||
|---|---|---|
| no. of returning VCs in the swarm | 4366 | * |
| no. of escaping VCs in the swarm | 635 | |
| no. of hyperbolas among escaping VCs in the swarm | 0 | |
| previous reciprocal semi-major axis [10-6 au-1] | 17.37 – 23.11 – 31.17 | R |
| previous perihelion distance [au] | 230 – 410 – 480 | R |
| previous aphelion distance [103 au] | 64 – 86 – 110 | R |
| time interval to previous perihelion [Myr] | 5.8 – 8.5 – 12 | R |
| 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_g orbit statistics, here only the Galactic tide has been included | ||
|---|---|---|
| no. of returning VCs in the swarm | 4786 | * |
| no. of escaping VCs in the swarm | 215 | |
| no. of hyperbolas among escaping VCs in the swarm | 0 | |
| previous reciprocal semi-major axis [10-6 au-1] | 18.91 – 25.11 – 32.11 | R |
| previous perihelion distance [au] | 7.4 – 53 – 350 | R |
| previous aphelion distance [103 au] | 62 – 80 – 110 | R |
| time interval to previous perihelion [Myr] | 5.4 – 7.6 – 11 | R |
| percentage of VCs with qprev < 10 | 14 | |
| percentage of VCs with 10 < qprev < 20 | 12 | |
| percentage of VCs with qprev > 20 | 74 | |