C/2020 H11 PanSTARRS-Lemmon
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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 1708 04 17
perihelion date 2020 09 11.79240376 ± 0.00351681
perihelion distance [au] 7.62697000 ± 0.00002115
eccentricity 0.99829484 ± 0.00001665
argument of perihelion [°] 91.335103 ± 0.000244
ascending node [°] 302.962052 ± 0.000059
inclination [°] 151.381409 ± 0.000014
reciprocal semi-major axis [10-6 au-1] 223.57 ± 2.18
file containing 5001 VCs swarm
2020h1a5.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.