C/2015 D3 PANSTARRS
more info
Comet C/2015 D3 was discovered on 19 February 2015 with Pan-STARRS 1 telescope (Haleakala), that is about 2.5 months after its perihelion passage. Some prediscovery images of this comet were found: taken on 17 February 2015 by Space Surveillance Telescope (Atom Site) and 8 April 2013 by Siding Spring Survey. This comet was observed until 26 October 2019 (is still observable).
Comet had its closest approach to the Earth on 28 February 2016 (7.167 au), about 2 months before its perihelion passage.
Solution given here is based on data spanning over 4.85 yr in a range of heliocentric distances: 10.46 au – 8.149 au (perihelion) – 9.03 au.
This Oort spike comet suffers slight planetary perturbations during its passage through the planetary system; however, these perturbations likely lead to escape the comet from the planetary zone on a hyperbolic orbit (see future barycentric orbits).

solution description
number of observations 282
data interval 2013 04 08 – 2018 02 13
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 10.46 au – 8.15 au (perihelion) – 9.03 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 549
RMS [arcseconds] 0.33
orbit quality class 1a+
orbital elements (heliocentric ecliptic J2000)
Epoch 2016 05 12
perihelion date 2016 04 30.78880394 ± 0.00118321
perihelion distance [au] 8.14877530 ± 0.00000841
eccentricity 1.00249983 ± 0.00000711
argument of perihelion [°] 2.849893 ± 0.000066
ascending node [°] 156.980463 ± 0.000006
inclination [°] 128.509312 ± 0.000013
recip semi-major axis [10-6 au-1] -306.77 ± 0.87