C/2000 H1 LINEAR
more info
Comet C/2000 H1 was discovered three months after perihelion passage and next observed up to one year in a range of heliocentric distances from 3.72 au to 5.35 au. However, the observations are unevenly distributed in this period – there is a ten-month gap between 28 June 2000 and 24 April 2001.
Comet had its closest approach to the Earth on 19 May 2000 (3.385 au).
This Oort spike comet suffers moderate planetary perturbations during its passage through the planetary system that lead to a more tight future orbit (see future barycentric orbit).
See also Królikowska and Dybczyński 2017.

solution description
number of observations 116
data interval 2000 04 26 – 2001 04 25
data type observed only after perihelion (POST)
data arc selection entire data set (STD)
range of heliocentric distances 3.72 au – 5.35au
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 228
RMS [arcseconds] 0.60
orbit quality class 2a
orbital elements (barycentric ecliptic J2000)
Epoch 1696 07 28
perihelion date 2000 01 26.87317916 ± 0.00810809
perihelion distance [au] 3.64438682 ± 0.00004065
eccentricity 0.99978811 ± 0.00013895
argument of perihelion [°] 78.572883 ± 0.000974
ascending node [°] 356.430616 ± 0.000245
inclination [°] 118.232361 ± 0.000038
recip semi-major axis [10-6 au-1] 58.14 ± 38.13
file containing 5001 VCs swarm
2000h1a5.bmi
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
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.