C/2017 U4 PANSTARRS
more info
Comet C/2017 U4 was discovered on 27 October 2017 with Pan-STARRS 1 telescope (Haleakala), that is about 11 months before its perihelion passage. Few prediscovery images of this comet were found: taken by the same survey from 2 January 2017.This comet was observed until 26 February 2020.

Comet had its closest approach to the Earth on 11 December 2018 (6.761 au), about 2.5 months after its perihelion passage.

The preferred solution given here is based on data spanning over 3.15 yr in a range of heliocentric distances: 8.64 au – 7.72 au (perihelion) – 8.36 au.

This near-parabolic comet suffers tiny planetary perturbations during its passage through the planetary system (original and future semimajor axes around 9,000 au).
solution description
number of observations 75
data interval 2017 01 02 – 2018 09 07
data arc selection data generally limited to pre-perihelion (PRE)
range of heliocentric distances 8.64 au – 7.72au
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 139
RMS [arcseconds] 0.31
orbit quality class 1a
previous orbit statistics, both Galactic and stellar perturbations were taken into account
no. of returning VCs in the swarm 5001 *
no. of escaping VCs in the swarm 0
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 106.79 – 110.61 – 114.27
previous perihelion distance [au] 7.7512 – 7.7544 – 7.7579
previous aphelion distance [103 au] 17.5 – 18.1 – 18.7
time interval to previous perihelion [Myr] 0.818 – 0.859 – 0.905
percentage of VCs with qprev < 10100
previous orbit statistics, here only the Galactic tide has been included
no. of returning VCs in the swarm 5001 *
no. of escaping VCs in the swarm 0
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 106.79 – 110.61 – 114.26
previous perihelion distance [au] 7.73862 – 7.73928 – 7.74009
previous aphelion distance [103 au] 17.5 – 18.1 – 18.7
time interval to previous perihelion [Myr] 0.818 – 0.859 – 0.905
percentage of VCs with qprev < 10100