C/1997 BA6 Spacewatch
more info
Comet C/1997 BA6 was discovered as an asteroidal object by the Spacewatch program on 31 January 1997 (with also prediscovery images on January 11) (IAUC 6561). In February, two independent groups on the basis of exposures with 2.4-m Hiltner Telescope at Kitt Peak and 2.2-m telescope on Mauna Kea detected coma around C/1997 BA6 (IAUC 6561).
At the moment of discovery the comet was almost three years before its perihelion passage. C/1997 BA6 was last seen on 15 September 2004.
The comet made its closest approach to the Earth on 27 July 2000 (3.21 au), that was eight months after perihelion passage, however in the previous opposition it was within 3.66 au on 20 March 1999 (about seven months before perihelion).
Solutions given here is based on data span over 7.68 yr in the range of heliocentric distances: 9.15 au – 3.44 au (perihelion) – 13.39 au.
NG orbits using full data-arc as well as independently using pre-perihelion and post-perihelion data are determinable.
See also Królikowska and Dones 2023, Królikowska and Dybczyński 2017,and Królikowska 2014.
At the moment of discovery the comet was almost three years before its perihelion passage. C/1997 BA6 was last seen on 15 September 2004.
The comet made its closest approach to the Earth on 27 July 2000 (3.21 au), that was eight months after perihelion passage, however in the previous opposition it was within 3.66 au on 20 March 1999 (about seven months before perihelion).
Solutions given here is based on data span over 7.68 yr in the range of heliocentric distances: 9.15 au – 3.44 au (perihelion) – 13.39 au.
NG orbits using full data-arc as well as independently using pre-perihelion and post-perihelion data are determinable.
See also Królikowska and Dones 2023, Królikowska and Dybczyński 2017,and Królikowska 2014.
| solution description | ||
|---|---|---|
| number of observations | 258 | |
| data interval | 1997 01 11 – 1999 11 12 | |
| data arc selection | data generally limited to post-perihelion (POS) | |
| range of heliocentric distances | 3.45 au – 13.39au | |
| type of model of motion | NC - non-gravitational orbits for symmetric CO-g(r)-like function | |
| data weighting | YES | |
| number of residuals | 509 | |
| RMS [arcseconds] | 0.68 | |
| orbit quality class | 1a | |
| orbital elements (barycentric ecliptic J2000) | ||
|---|---|---|
| Epoch | 2307 06 17 | |
| perihelion date | 1999 11 28.37798923 | ± 0.00404670 |
| perihelion distance [au] | 3.43242532 | ± 0.00004134 |
| eccentricity | 0.99852438 | ± 0.00001524 |
| argument of perihelion [°] | 285.867769 | ± 0.000867 |
| ascending node [°] | 317.586721 | ± 0.000054 |
| inclination [°] | 72.674309 | ± 0.000127 |
| reciprocal semi-major axis [10-6 au-1] | 429.91 | ± 4.45 |
| file containing 5001 VCs swarm |
|---|
| 1997bard.bpl |
Upper panel: 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.
Middle panel(s): O-C diagram for a given solution (sometimes in comparison to another solution available in CODE), where residuals in right ascension are shown using magenta dots and in declination by blue open circles.
Lowest panel: Relative weights for a given data set(s).
Middle panel(s): O-C diagram for a given solution (sometimes in comparison to another solution available in CODE), where residuals in right ascension are shown using magenta dots and in declination by blue open circles.
Lowest panel: Relative weights for a given data set(s).
Six 2D-projections of the 6D space of future swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.