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 430
data interval 2019 02 01 – 2021 11 30
data arc selection data generally limited to post-perihelion (POS)
range of heliocentric distances 3.25 au – 9.19au
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 834
RMS [arcseconds] 0.33
orbit quality class 1a+
orbital elements (heliocentric ecliptic J2000)
Epoch 2019 02 06
perihelion date 2019 01 18.16519239 ± 0.00022700
perihelion distance [au] 3.25171638 ± 0.00000152
eccentricity 1.00230302 ± 0.00000241
argument of perihelion [°] 167.615632 ± 0.000053
ascending node [°] 65.867664 ± 0.000006
inclination [°] 105.657343 ± 0.000012
reciprocal semi-major axis [10-6 au-1] -708.25 ± 0.74
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).