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 | |
| type of model of motion | NH - non-gravitational orbits for water sublimation from subsolar point | |
| data weighting | YES | |
| number of residuals | 834 | |
| RMS [arcseconds] | 0.30 | |
| orbit quality class | 1a | |
| orbital elements (barycentric ecliptic J2000) | ||
|---|---|---|
| Epoch | 1716 12 11 | |
| perihelion date | 2019 01 18.65770879 | ± 0.00296211 |
| perihelion distance [au] | 3.24471435 | ± 0.00001710 |
| eccentricity | 1.00000799 | ± 0.00004552 |
| argument of perihelion [°] | 167.766843 | ± 0.000865 |
| ascending node [°] | 65.816342 | ± 0.000146 |
| inclination [°] | 105.658647 | ± 0.000372 |
| reciprocal semi-major axis [10-6 au-1] | -2.46 | ± 14.03 |
| file containing 5001 VCs swarm |
|---|
| 2017m4rs.bpl |
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).
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).
Six 2D-projections of the 6D space of future swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.