C/2011 L6 Boattini
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Comet C/2011 L6 was discovered ny Andrea Boattini (Mt Lemmon) on 8 June 2011, that is about 4.5 months after perihelion passage. Soon, the comet was found on earlier images taken on 28 May 2011 with the Mount Lemmon Survey.
Comet had its closest approach to the Earth on 14 May 2011 (5.819 au), about three weeks before discovery.
C/2011 L6 was observed 0.91 yr in a range of heliocentric distances from 6.84 au to 7.42 au.
This comet suffers very small planetary perturbations during its passage through the planetary system that lead to a less tight future orbit with semimjor axis larger than 10000 au. (see future barycentric orbit).
See also Królikowska and Dybczyński 2017.
Comet had its closest approach to the Earth on 14 May 2011 (5.819 au), about three weeks before discovery.
C/2011 L6 was observed 0.91 yr in a range of heliocentric distances from 6.84 au to 7.42 au.
This comet suffers very small planetary perturbations during its passage through the planetary system that lead to a less tight future orbit with semimjor axis larger than 10000 au. (see future barycentric orbit).
See also Królikowska and Dybczyński 2017.
| solution description | ||
|---|---|---|
| number of observations | 56 | |
| data interval | 2011 05 28 – 2012 04 24 | |
| data type | observed only after perihelion (POST) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 6.84 au – 7.42au | |
| 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 | 112 | |
| RMS [arcseconds] | 0.59 | |
| orbit quality class | 1b | |
| orbital elements (barycentric ecliptic J2000) | ||
|---|---|---|
| Epoch | 1701 08 12 | |
| perihelion date | 2011 01 21.34613319 | ± 0.04634191 |
| perihelion distance [au] | 6.78832443 | ± 0.00012547 |
| eccentricity | 0.99927158 | ± 0.00006839 |
| argument of perihelion [°] | 331.438066 | ± 0.003937 |
| ascending node [°] | 214.387264 | ± 0.000241 |
| inclination [°] | 171.448835 | ± 0.000133 |
| reciprocal semi-major axis [10-6 au-1] | 107.30 | ± 10.07 |
| file containing 5001 VCs swarm |
|---|
| 2011l6a1.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.