C/2017 E3 PANSTARRS
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Comet C/2017 E3 was discovered on 7 March 2017 with Pan-STARRS 1 telescope (Haleakala), that is about 3 months before its perihelion passage. This comet was observed until 24 July 2019.
Comet had its closest approach to the Earth on 24 April 2017 (3.480 au), about 1.5 month after discovery and more than a month before its perihelion passage.
Solution given here is based on data spanning over 1.21 yr in a range of heliocentric distances: 5.95 au – 5.915 au (perihelion) – 6.42 au (24 May 2018).
This Oort spike comet suffers moderate planetary perturbations during its passage through the planetary system; these perturbations lead to escape the comet from the planetary zone on a hyperbolic orbit (see future barycentric orbits).

solution description
number of observations 348
data interval 2017 03 07 – 2018 05 24
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 5.95 au – 5.92 au (perihelion) – 6.42 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 684
RMS [arcseconds] 0.45
orbit quality class 1a
orbital elements (heliocentric ecliptic J2000)
Epoch 2017 06 16
perihelion date 2017 05 31.58309653 ± 0.00278038
perihelion distance [au] 5.91525895 ± 0.00000569
eccentricity 1.00496498 ± 0.00000646
argument of perihelion [°] 333.664659 ± 0.000264
ascending node [°] 220.758558 ± 0.000009
inclination [°] 70.665041 ± 0.000021
recip semi-major axis [10-6 au-1] -839.35 ± 1.09