C/2019 K7 Smith
more info
Comet C/2019 K7 was discovered on 30 May 2019, more than one year before its perihelion passage. Later a few pre-discovery observations were found from 8 and 9 October 2017. In the moment of orbit determination, this comet was still observed.

Solutions (GR and NG) given here span over 5.49 yr in a range of heliocentric distances: 8.64 au – 4.48 au (perihelion) – 9.2 au; orbits based on pre-perihelion and post-perihelion data independently were also obtained.

This Oort spike comet suffers moderate planetary perturbations during its passage through the planetary system that lead to a more tight future orbit (see future barycentric orbit).
solution description
number of observations 2114
data interval 2020 06 18 – 2023 06 03
data arc selection data generally limited to post-perihelion (POS)
range of heliocentric distances 4.48 au – 9.2au
type of model of motion NC - non-gravitational orbits for symmetric CO-g(r)-like function
data weighting YES
number of residuals 4156
RMS [arcseconds] 0.40
orbit quality class 1a
orbital elements (barycentric ecliptic J2000)
Epoch 2329 04 02
perihelion date 2020 06 15.70667283 ± 0.00109001
perihelion distance [au] 4.46871943 ± 0.00000663
eccentricity 0.99828542 ± 0.00000411
argument of perihelion [°] 27.198183 ± 0.000123
ascending node [°] 307.986247 ± 0.000030
inclination [°] 103.568721 ± 0.000006
reciprocal semi-major axis [10-6 au-1] 383.69 ± 0.92
file containing 5001 VCs swarm
2019k7rc.bpl
Six 2D-projections of the 6D space of future swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.