C/2020 N1 PanSTARRS
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Comet C/2020 N1 was discovered on 3 July 2020, about 8.5 months before its perihelion passage, later a single pre-discovery observation was found from 1 July 2020. This comet was observed to 14 April 2021.

Solutions given here (NG and GR) are based on data span over 0.786 yr in a range of heliocentric distances: 3.55 au – 1.32 au (perihelion) – 1.41 au.

This Oort spike comet suffers moderate planetary perturbations during its passage through the planetary system that lead to escape the comet from the solar system on hyperbolic barycentric orbit.
solution description
number of observations 915
data interval 2020 07 01 – 2021 04 14
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 3.55 au – 1.32 au (perihelion) – 1.41 au
type of model of motion NS - non-gravitational orbits for standard g(r)
data weighting YES
number of residuals 1763
RMS [arcseconds] 0.52
orbit quality class 1b
previous orbit statistics, both Galactic and stellar perturbations were taken into account
no. of returning VCs in the swarm 290
no. of escaping VCs in the swarm 4711 *
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 10.28 – 13.06 – 15.88
previous perihelion distance [au] 3020 – 3280 – 3520
previous aphelion distance [103 au] 120 – 150 – 190
time interval to previous perihelion [Myr] 3.6 ± 4.3983
percentage of VCs with qprev > 20100
previous orbit statistics, here only the Galactic tide has been included
no. of returning VCs in the swarm 428
no. of escaping VCs in the swarm 4573 *
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 10.94 – 13.72 – 16.55
previous perihelion distance [au] 14 – 16 – 18
previous aphelion distance [103 au] 120 – 150 – 180
time interval to previous perihelion [Myr] 3.59 ± 4.3983
percentage of VCs with 10 < qprev < 20100