C/2020 T4 PanSTARRS
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Comet C/2020 T4 was discovered on 15 October 2020, about 9.5 months before its perihelion passage, later two series of pre-discovery observations were found from 9 October 2020 and 26 September 2020. This comet was observed to 17 June 2021 (to about two weeks before perihelion passage).

Solutions given here are based on data span over 0.726 yr in a range of heliocentric distances from 3.78 au to 2.20 au.

This Oort spike comet suffers rather small planetary perturbations during its passage through the planetary system; however, they lead to escape the comet from the solar system on hyperbolic barycentric orbit.
solution description
number of observations 174
data interval 2020 09 26 – 2021 06 17
data type observed only before perihelion (PRE)
data arc selection entire data set (STD)
range of heliocentric distances 3.78 au – 2.2au
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 336
RMS [arcseconds] 0.23
orbit quality class 1b
orbital elements (barycentric ecliptic J2000)
Epoch 1720 10 11
perihelion date 2021 07 04.64745495 ± 0.00025476
perihelion distance [au] 2.18937405 ± 0.00000754
eccentricity 0.99989958 ± 0.00000410
argument of perihelion [°] 79.672856 ± 0.000236
ascending node [°] 50.729931 ± 0.000013
inclination [°] 83.757021 ± 0.000118
reciprocal semi-major axis [10-6 au-1] 45.87 ± 1.87
file containing 5001 VCs swarm
2020t4pa.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.