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).
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 | ||
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number of observations | 2745 | |
data interval | 2017 10 08 – 2023 06 03 | |
data type | perihelion within the observation arc (FULL) | |
data arc selection | entire data set (STD) | |
range of heliocentric distances | 8.64 au – 4.48 au (perihelion) – 9.2 au | |
type of model of motion | NC - non-gravitational orbits for symmetric CO-g(r)-like function | |
data weighting | YES | |
number of residuals | 5402 | |
RMS [arcseconds] | 0.41 | |
orbit quality class | 1a+ |
orbital elements (barycentric ecliptic J2000) | ||
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Epoch | 2329 06 21 | |
perihelion date | 2020 06 15.68900983 | ± 0.00069793 |
perihelion distance [au] | 4.46869968 | ± 0.00000408 |
eccentricity | 0.99822755 | ± 0.00000304 |
argument of perihelion [°] | 27.196985 | ± 0.000089 |
ascending node [°] | 307.985987 | ± 0.000013 |
inclination [°] | 103.568778 | ± 0.000003 |
reciprocal semi-major axis [10-6 au-1] | 396.64 | ± 0.68 |
file containing 5001 VCs swarm |
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2019k7bc.bpl |