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 2854
data interval 2017 06 16 – 2018 11 13
data arc selection data generally limited to pre-perihelion (PRE)
range of heliocentric distances 6.09 au – 3.31au
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 5658
RMS [arcseconds] 0.40
orbit quality class 1a
orbital elements (heliocentric ecliptic J2000)
Epoch 2019 02 06
perihelion date 2019 01 18.19121425 ± 0.00011067
perihelion distance [au] 3.25175176 ± 0.00000095
eccentricity 1.00229463 ± 0.00000111
argument of perihelion [°] 167.622212 ± 0.000028
ascending node [°] 65.867038 ± 0.000007
inclination [°] 105.657705 ± 0.000004
reciprocal semi-major axis [10-6 au-1] -705.66 ± 0.34
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).