C/2002 J5 LINEAR
more info
C/2002 J5 was discovered on 15 May 2002 by the LINEAR as an apparently asteroidal object. Next day, its cometary apperance was reported by M. Tichy and M. Kocer from Klet [IAUC 7904, 2002 May 18]. Later, pre-discovery detections (from August 2001) by LINEAR and AMOS were found.
This comet made its closest approach to the Earth on 19 June 2003 (5.233 au), three months before perihelion.
Solution given here is based on data spanning over 4.6 yr in a range of heliocentric distances: 7.87 au – 5.727 au (perihelion) – 8.44 au.
This Oort spike comet suffers slight planetary perturbations during its passage through the planetary system.
See also Królikowska 2014 and Królikowska and Dybczyński 2017.

solution description
number of observations 618
data interval 2001 08 06 – 2006 03 05
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 7.87 au – 5.73 au (perihelion) – 8.44 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 1227
RMS [arcseconds] 0.53
orbit quality class 1a+
orbital elements (heliocentric ecliptic J2000)
Epoch 2003 10 08
perihelion date 2003 09 19.30916500 ± 0.00042200
perihelion distance [au] 5.72679475 ± 0.00000292
eccentricity 1.00116654 ± 0.00000388
argument of perihelion [°] 74.832954 ± 0.000039
ascending node [°] 314.110065 ± 0.000013
inclination [°] 117.228214 ± 0.000007
recip semi-major axis [10-6 au-1] -203.70 ± 0.68
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