C/2017 F1 Lemmon
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Comet C/2017 F1 was discovered on 20 March 2017 with Mount Lemmon survey, that is about 8.5 months before its perihelion passage. Later single pre-discovery obsebation was found from 4 February 2017. This comet was rather rarely observed until 18 March 2018.

Comet had its closest approach to the Earth on 24 December 2017 (3.480 au), less than a month after its perihelion passage.

The preferred solution given here is based on data spanning over 1.12 yr in a range of heliocentric distances: 5.10 au – 4.50 au (perihelion) – 4.58 au.

This Oort spike comet suffers moderate planetary perturbations during its passage through the planetary system; these perturbations lead to escape the comet from the planetary zone on a hyperbolic orbit (see future barycentric orbits).
solution description
number of observations 89
data interval 2017 02 04 – 2018 03 18
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 5.1 au – 4.50 au (perihelion) – 4.58 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 165
RMS [arcseconds] 0.40
orbit quality class 1a
orbital elements (heliocentric ecliptic J2000)
Epoch 2017 11 23
perihelion date 2017 11 30.98593929 ± 0.00352510
perihelion distance [au] 4.49975834 ± 0.00000843
eccentricity 1.00435110 ± 0.00001423
argument of perihelion [°] 64.815466 ± 0.000477
ascending node [°] 158.742645 ± 0.000066
inclination [°] 146.481068 ± 0.000038
reciprocal semi-major axis [10-6 au-1] -966.96 ± 3.16