C/2020 H11 PanSTARRS-Lemmon
more info
Comet C/2020 H11 was discovered on 21 April 2020, about 5 months before its perihelion passage. Later a series of pre-discovery observations were found going ten months back to 2 June 2019. This comet was observed to 8 May 2021.

Solutions given here are based on data span over 1.93 yr in a range of heliocentric distances: 8.17 au – 7.63 au (perihelion) – 7.77 au.

This comet entered the planetary zone having original semimajor axis of about 4,500 au and suffers small planetary perturbations during its passage through the planetary system that lead to a bit tight future orbit (semimajor axis of about 3,100 au).
solution description
number of observations 53
data interval 2019 06 02 – 2021 05 08
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 8.17 au – 7.63 au (perihelion) – 7.77 au
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 106
RMS [arcseconds] 0.22
orbit quality class 1a
orbital elements (barycentric ecliptic J2000)
Epoch 2334 05 26
perihelion date 2020 09 12.13403887 ± 0.00352823
perihelion distance [au] 7.63386444 ± 0.00002112
eccentricity 0.99751254 ± 0.00001668
argument of perihelion [°] 91.429357 ± 0.000245
ascending node [°] 303.080922 ± 0.000060
inclination [°] 151.417118 ± 0.000015
reciprocal semi-major axis [10-6 au-1] 325.85 ± 2.19
file containing 5001 VCs swarm
2020h1a5.bpl
Six 2D-projections of the 6D space of future swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.