C/2017 AB5 PANSTARRS
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Comet C/2017 AB5 was discovered on 3 January 2017 with Pan-STARRS 1 telescope (Haleakala), that is more than a year before its perihelion passage. This comet was rather rarely observed until 25 April 2019.

Comet had its closest approach to the Earth on 18 January 2018 (8.395 au), about a month before its perihelion passage.

The preferred solution given here is based on data spanning over 2.31 yr in a range of heliocentric distances: 9.50 au – 9.22 au (perihelion) – 9.53 au.

This Oort spike comet suffers small planetary perturbations during its passage through the planetary system and will have a bit more tight future orbit (see future barycentric orbit).
solution description
number of observations 85
data interval 2017 01 03 – 2019 04 25
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 9.5 au – 9.22 au (perihelion) – 9.53 au
detectability of NG effects in the comet's motion NG effects not determinable
type of model of motion GR - gravitational orbit
data weighting NO
number of residuals 158
RMS [arcseconds] 0.37
orbit quality class 1a
orbital elements (heliocentric ecliptic J2000)
Epoch 2018 02 11
perihelion date 2018 02 17.87049467 ± 0.00914449
perihelion distance [au] 9.21642817 ± 0.00003378
eccentricity 0.99987207 ± 0.00002120
argument of perihelion [°] 78.395277 ± 0.000463
ascending node [°] 42.690339 ± 0.000099
inclination [°] 32.431004 ± 0.000019
reciprocal semi-major axis [10-6 au-1] 13.88 ± 2.30