C/2018 B1 Lemmon
more info
Comet C/2018 B1 was discovered on 25 January 2018, about two months before its perihelion passage; later a few prediscovery measurements going back to 16 January 2017 were found. This comet was last seen on 31 October 2019.

Solution given here is based on data span over 2.79 yr in the range of heliocentric distances from: 6.08 au – 5.12 au (perihelion) – 6.69 au.

This Oort spike comet suffers small planetary perturbations during its passage through the planetary system that lead to a more tight future orbit (see future barycentric orbit).
solution description
number of observations 320
data interval 2017 01 16 – 2019 10 31
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 6.08 au – 5.12 au (perihelion) – 6.69 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 634
RMS [arcseconds] 0.41
orbit quality class 1a+
orbital elements (barycentric ecliptic J2000)
Epoch 1710 05 17
perihelion date 2018 03 31.09429367 ± 0.00034957
perihelion distance [au] 5.12633456 ± 0.00000259
eccentricity 0.99893213 ± 0.00000349
argument of perihelion [°] 68.225912 ± 0.000055
ascending node [°] 133.077259 ± 0.000040
inclination [°] 162.45347 ± 0.000006
reciprocal semi-major axis [10-6 au-1] 208.31 ± 0.68
file containing 5001 VCs swarm
2018b1a5.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.