C/2018 V1 Machholz-Fujikawa-Iwamoto
more info
Comet C/2018 V1 was discovered on 7 November 2019, about one months before its perihelion passage, and was last seen on 15 December 2018.

Solutions (GR and NG) given here span over 0.101 yr in a range of heliocentric distances: 0.75 au – 0.39 au (perihelion) – 0.50 au;due to short data arc the orbital parameters are uncertain (orbit of 2b quality class).

This comet suffers notable planetary perturbations during its passage through the planetary system; in both cases (GR and NG model of motion) these perturbations lead to escape the comet from the planetary zone on a hyperbolic orbit (see future barycentric orbits).However, the original orbits in both solutions differ and the interstellar origin of this comet cannot be ruled out.
solution description
number of observations 766
data interval 2018 11 08 – 2018 12 15
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 0.75 au – 0.39 au (perihelion) – 0.5 au
detectability of NG effects in the comet's motion comet with determinable NG~orbit
type of model of motion GR - gravitational orbit
data weighting YES
number of residuals 1518
RMS [arcseconds] 0.56
orbit quality class 2b
orbital elements (heliocentric ecliptic J2000)
Epoch 2018 11 18
perihelion date 2018 12 03.50739841 ± 0.00009260
perihelion distance [au] 0.38694342 ± 0.00000112
eccentricity 1.00053119 ± 0.00001412
argument of perihelion [°] 88.774793 ± 0.000118
ascending node [°] 128.725097 ± 0.000260
inclination [°] 143.984738 ± 0.000244
reciprocal semi-major axis [10-6 au-1] -1,372.80 ± 36.48