C/2020 V2 ZTF
more info
Comet C/2020 V2 was discovered on 2 November 2020, about 2.5 yr before its perihelion passage; later a series of prediscovery images was found going back to 18 April 2020 (10.08 au from the Sun). 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 3.0 yr in a range of heliocentric distances from 10.08 au to 2.24 au.Orbits based on a distant part of data arc are also given (helicentric distances greater than 3.5 au).

This is Oort spike comet. According to orbits obtained using pre-perihelion data this comet suffers rather small planetary perturbations that lead to escape this comet from the solar system on hyperbolic orbit.
solution description
number of observations 2732
data interval 2020 04 18 – 2022 08 28
data arc selection data generally limited to pre-perihelion (PRE)
range of heliocentric distances 10.08 au – 3.55au
type of model of motion NC - non-gravitational orbits for symmetric CO-g(r)-like function
data weighting YES
number of residuals 5364
RMS [arcseconds] 0.21
orbit quality class 1a+
orbital elements (barycentric ecliptic J2000)
Epoch 1722 11 10
perihelion date 2023 05 09.72275141 ± 0.00096867
perihelion distance [au] 2.22484329 ± 0.00000489
eccentricity 0.99996555 ± 0.00000147
argument of perihelion [°] 162.539961 ± 0.000091
ascending node [°] 212.331653 ± 0.000034
inclination [°] 131.649029 ± 0.000026
reciprocal semi-major axis [10-6 au-1] 15.48 ± 0.66
file containing 5001 VCs swarm
2020v2dc.bmi
Six 2D-projections of the 6D space of original swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.