C/2018 S3 TESS
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Comet C/2018 S3 was discovered on 22 September 2018 by Transiting Exoplanet Survey Satellite (TESS), about two years after its perihelion passage; later 13 observations were found going more than 4.5 yr back to 29 June  2014 (all by Cerro Tololo-DECam). This comet was observed only by TESS and Cerro Tololo-DECam, and was last seen on 1 December 2018 by Cerro Tololo-DECam.

The solution given here is based solely on the data from Cerro Tololo-DECam and span over 4.79 yr in a range of heliocentric distances: 9.53 au – 8.01 au (perihelion) – 9.59 au.

This Oort spike comet suffers tiny planetary perturbations during its passage through the planetary system that lead to a future orbit with greater semimajor-axis (see future barycentric orbit).
solution description
number of observations 17
data interval 2014 02 15 – 2018 12 01
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 9.53 au – 8.01 au (perihelion) – 9.59 au
detectability of NG effects in the comet's motion NG effects not determinable
type of model of motion GR - gravitational orbit
data weighting NO
number of residuals 34
RMS [arcseconds] 0.13
orbit quality class 1a+
orbital elements (heliocentric ecliptic J2000)
Epoch 2023 02 25
perihelion date 2016 06 29.24907336 ± 0.00129350
perihelion distance [au] 8.01203755 ± 0.00001179
eccentricity 1.00244213 ± 0.00001016
argument of perihelion [°] 263.948836 ± 0.000070
ascending node [°] 25.045145 ± 0.000018
inclination [°] 78.297824 ± 0.000014
reciprocal semi-major axis [10-6 au-1] -304.81 ± 1.27