C/2020 O2 Amaral
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Comet C/2020 O2 was discovered on 23 July 2020, more than one year before its perihelion passage. In the moment of orbit determination, this comet was still observed.
Currently, solutions (GR and NG) based on pre-perihelion data are given. Therefore, the data arc span over 1.10 yr in a range of heliocentric distances from 5.76 au to 4.86 au.
This is Oort spike comet.
Currently, solutions (GR and NG) based on pre-perihelion data are given. Therefore, the data arc span over 1.10 yr in a range of heliocentric distances from 5.76 au to 4.86 au.
This is Oort spike comet.
solution description | ||
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number of observations | 507 | |
data interval | 2020 07 23 – 2021 08 28 | |
data arc selection | data generally limited to pre-perihelion (PRE) | |
range of heliocentric distances | 5.76 au – 4.86 au (perihelion) – 4.86 au | |
detectability of NG effects in the comet's motion | comet with determinable NG~orbit | |
type of model of motion | GR - gravitational orbit | |
data weighting | YES | |
number of residuals | 986 | |
RMS [arcseconds] | 0.27 | |
orbit quality class | 1a |
previous orbit statistics, both Galactic and stellar perturbations were taken into account | ||
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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 | |
previous reciprocal semi-major axis [10-6 au-1] | 40.60 – 41.01 – 41.41 | |
previous perihelion distance [au] | 510 – 546 – 583 | |
previous aphelion distance [103 au] | 47.78 – 48.22 – 48.68 | |
time interval to previous perihelion [Myr] | 3.33 – 3.39 – 3.46 | |
percentage of VCs with qprev > 20 | 100 |
previous orbit statistics, here only the Galactic tide has been included | ||
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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 | |
previous reciprocal semi-major axis [10-6 au-1] | 43.43 – 44.04 – 44.64 | |
previous perihelion distance [au] | 6.39 – 6.48 – 6.59 | |
previous aphelion distance [103 au] | 44.8 – 45.4 – 46 | |
time interval to previous perihelion [Myr] | 3.35 – 3.42 – 3.5 | |
percentage of VCs with qprev < 10 | 100 |