C/2017 M4 ATLAS
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Comet C/2017 M4 was discovered on 21 June 2017 by Asteroid Terrestrial-impact Last Alert System (ATLAS) Team, that is about months after its perihelion passage.
Some prediscovery images of this comet were found: taken on 16 June 2017 by Pan-STARRS 1 telescope (Haleakala).
Solutions given here are based on data spanning over 4.46 yr in a range of heliocentric distances: 6.09 au – 3.252 au (perihelion) – 9.19 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.
solution description | ||
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number of observations | 1293 | |
data interval | 2017 06 16 – 2018 05 24 | |
data arc selection | data generally limited to pre-perihelion (PRE) | |
range of heliocentric distances | 6.09 au – 3.95au | |
detectability of NG effects in the comet's motion | comet with NG effects strongly manifested in positional data fitting | |
type of model of motion | GR - gravitational orbit | |
data weighting | YES | |
number of residuals | 2552 | |
RMS [arcseconds] | 0.32 | |
orbit quality class | 1a |
orbital elements (barycentric ecliptic J2000) | ||
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Epoch | 2322 06 18 | |
perihelion date | 2019 01 17.71549151 | ± 0.00032250 |
perihelion distance [au] | 3.24192454 | ± 0.00000544 |
eccentricity | 0.99962239 | ± 0.00000177 |
argument of perihelion [°] | 167.372101 | ± 0.000079 |
ascending node [°] | 65.857842 | ± 0.000016 |
inclination [°] | 105.703297 | ± 0.000003 |
reciprocal semi-major axis [10-6 au-1] | 116.48 | ± 0.55 |
file containing 5001 VCs swarm |
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2017m4a5.bpl |