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
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
previous orbit statistics, both Galactic and stellar perturbations were taken into account
no. of returning VCs in the swarm 5001 *
no. of escaping VCs in the swarm 0
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 38.01 – 38.49 – 38.96
previous perihelion distance [au] 529 – 568 – 608
previous aphelion distance [103 au] 50.8 – 51.4 – 52
time interval to previous perihelion [Myr] 3.63 – 3.71 – 3.8
percentage of VCs with qprev > 20100
previous orbit statistics, here only the Galactic tide has been included
no. of returning VCs in the swarm 5001 *
no. of escaping VCs in the swarm 0
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 40.38 – 41.07 – 41.76
previous perihelion distance [au] 4.16 – 4.36 – 4.59
previous aphelion distance [103 au] 47.9 – 48.7 – 49.5
time interval to previous perihelion [Myr] 3.7 – 3.8 – 3.89
percentage of VCs with qprev < 10100