C/2000 OF8 Spacewatch
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Comet C/2000 OF8 was discovered on 24 July 2000 with Spacewatch Research project (Steward Observatory, Kitt Peak), that is a year before its perihelion passage. It was observed until 1 August 2001.
Preffered solution given here is based on pre-perihelion data spanning over 1.02 yr in a range of heliocentric distances from 4.56 au to 2.17 au.
Comet had its closest approach to the Earth on 4 June 2001 (1.390 au), about 2 months before perihelion passage.
This is Oort spike comet.
See also Sekanina 2019 and Królikowska 2020

solution description
number of observations 75
data interval 2000 07 24 – 2001 08 01
data type observed only before perihelion (PRE)
data arc selection entire data set (STD)
range of heliocentric distances 4.56 au – 2.23au
detectability of NG effects in the comet's motion comet lost close to perihelion or split comet
type of model of motion GR - gravitational orbit
data weighting NO
number of residuals 136
RMS [arcseconds] 0.52
orbit quality class 1b
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] 37.63 – 43.12 – 57.97
previous perihelion distance [au] 3.6 – 370 – 910
previous aphelion distance [103 au] 34 – 46 – 52
time interval to previous perihelion [Myr] 2.3 – 2.8 – 3.6
percentage of VCs with qprev < 1022
percentage of VCs with qprev > 2078
Time distribution of positional observations with corresponding heliocentric (red curve) and geocentric (green curve) distance at which they were taken. The horizontal dotted line shows the perihelion distance for a given comet whereas vertical dotted line — the moment of perihelion passage.
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] 42.37 – 49.69 – 57.29
previous perihelion distance [au] 3.3 – 4.3 – 6.4
previous aphelion distance [103 au] 35 – 40 – 47
time interval to previous perihelion [Myr] 2.3 – 2.8 – 3.6
percentage of VCs with qprev < 1098
percentage of VCs with 10 < qprev < 201
percentage of VCs with qprev > 201