C/2014 R3 PANSTARRS
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Comet C/2014 R3 was discovered on 6 September 2014 with Pan-STARRS 1 telescope (Haleakala), that is almost two years before its perihelion passage. This comet was observed until the end of 2019, and is still observable.
Comet had its closest approach to the Earth on 24 February 2017 (6.829 au), about 6.5 months after its perihelion passage.
Solution given here is based on data spanning over 3.47 yr in a range of heliocentric distances: 8.51 au – 7.275 au (perihelion) – 8.11 au (25 February 2018).
This marginally Oort spike comet suffers slight planetary perturbations during its passage through the planetary system; these perturbations lead to a more tight future orbit (see future barycentric orbits).

solution description
number of observations 634
data interval 2014 09 06 – 2018 02 25
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 8.51 au – 7.28 au (perihelion) – 8.11 au
detectability of NG effects in the comet's motion NG effects not determinable
type of model of motion GR - gravitational orbit
data weighting YES
number of residuals 1255
RMS [arcseconds] 0.32
orbit quality class 1a+
orbital elements (barycentric ecliptic J2000)
Epoch 1706 04 28
perihelion date 2016 08 08.32460195 ± 0.00068478
perihelion distance [au] 7.27446861 ± 0.00000345
eccentricity 0.99923922 ± 0.00000298
argument of perihelion [°] 113.417665 ± 0.000047
ascending node [°] 334.072111 ± 0.000010
inclination [°] 90.825465 ± 0.000005
reciprocal semi-major axis [10-6 au-1] 104.58 ± 0.41