C/2020 N1 PanSTARRS
more info
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
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] -757.90 – -744.34 – -730.34
next perihelion distance [au] 0.66 – 0.668 – 0.676
synchronous stop epoch [Myr] 0.667 S
percentage of VCs with qnext < 10100
next 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] -758.00 – -744.44 – -730.43
next perihelion distance [au] 0.6575 – 0.6633 – 0.6694
synchronous stop epoch [Myr] 0.687 S
percentage of VCs with qnext < 10100