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
next 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
next reciprocal semi-major axis [10-6 au-1] 115.82 – 116.51 – 117.20
next perihelion distance [au] 3.2833 – 3.2844 – 3.2854
next aphelion distance [103 au] 17.06 – 17.16 – 17.27
time interval to next perihelion [Myr] 0.7873 – 0.7943 – 0.8015
percentage of VCs with qnext < 10100
next 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
next reciprocal semi-major axis [10-6 au-1] 115.79 – 116.49 – 117.18
next perihelion distance [au] 3.2849 – 3.2858 – 3.2868
next aphelion distance [103 au] 17.06 – 17.17 – 17.27
time interval to next perihelion [Myr] 0.7876 – 0.7946 – 0.8017
percentage of VCs with qnext < 10100