C/2006 P1 McNaught
more info
Comet C/2006 P1 was discovered on 7 August 2006 by Robert H. McNaught (Siding Spring Survey); that is about 5 months before its perihelion passage. It was observed until 11 July 2007 (see picture).
This comet with small perihelion distance of 0.17 au was the second brightest comet observed by ground-based observers since 1935 and developed a spectacularly structured huge dust tail.
Comet had its closest approach to the Earth on 15 January 2007 (0.817 au), about 3 days after its perihelion passage.
All orbits presented here are based on data spanning over 0.926 yr in a range of heliocentric distances: 2.74 au – 0.170 au (perihelion) – 3.34 au. NG orbit obtained using standard form of g(r) functionwith radial and transverse components of NG acceleration is quite well determined and was chosen here as preferred orbit; however, the NG orbit with three components of NG accelarations is also worth the attention.
This Oort spike comet suffers moderate planetary perturbations during its passage through the planetary system and these perturbations lead to more tight future orbit with semimajor axis a bit larger than 2,000 au (see future barycentric orbits).
See also Królikowska and Dybczyński 2013 and Królikowska 2020.

solution description
number of observations 334
data interval 2006 08 07 – 2007 07 11
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 2.74 au – 0.17 au (perihelion) – 3.34 au
type of model of motion NS - non-gravitational orbits for standard g(r)
data weighting YES
number of residuals 635
RMS [arcseconds] 0.23
orbit quality class 1b
orbital elements (barycentric ecliptic J2000)
Epoch 1709 10 29
perihelion date 2007 01 12.33767496 ± 0.00003231
perihelion distance [au] 0.17003736 ± 0.00000048
eccentricity 0.99999203 ± 0.00000069
argument of perihelion [°] 155.996007 ± 0.000089
ascending node [°] 267.457687 ± 0.000030
inclination [°] 77.652759 ± 0.000092
reciprocal semi-major axis [10-6 au-1] 46.90 ± 4.04
file containing 5001 VCs swarm
2006p1n7.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.