C/2019 O3 Palomar
more info
Comet C/2019 O3 was discovered on 26 July 2019, more than 1.5 yr before its perihelion passage. Later a series of pre-discovery observations were found going back to 14 May 2019. In the moment of orbit determination, this comet was still observed.

Currently, solutions (GR and NG) given here are based on data span over 4.13 yr in a range of heliocentric distances: 9.61 au – 8.82 au (perihelion) – 10.1 au. Orbits based on pre-perihelion and post-perihelion data independently were also obtained.

This Oort spike comet suffers small planetary perturbations during its passage through the planetary system that lead to a more tight future orbit (see future barycentric orbits).
solution description
number of observations 1613
data interval 2021 02 25 – 2023 06 29
data arc selection data generally limited to post-perihelion (POS)
range of heliocentric distances 8.82 au – 8.82 au (perihelion) – 10.06 au
type of model of motion NC - non-gravitational orbits for symmetric CO-g(r)-like function
data weighting YES
number of residuals 3182
RMS [arcseconds] 0.39
orbit quality class 1a
orbital elements (heliocentric ecliptic J2000)
Epoch 2019 04 27
perihelion date 2021 03 06.17359463 ± 0.03171132
perihelion distance [au] 8.82221203 ± 0.00002011
eccentricity 1.00088092 ± 0.00001910
argument of perihelion [°] 59.944119 ± 0.001752
ascending node [°] 300.382966 ± 0.000139
inclination [°] 89.819091 ± 0.000106
reciprocal semi-major axis [10-6 au-1] -99.85 ± 2.16
non-gravitational parameters
A1 [10-8au/day2] 10.042 ± 4.089
A2 [10-8au/day2] -3.3255 ± 1.4231
A3 [10-8au/day2] 3.5137 ± 0.8007
m -2.00
n 3.000
k -2.6000
r0 [au] 10.000
α 0.0100