C/2019 U5 PanSTARRS
more info
Comet C/2019 U5 was discovered on 22 October 2019, about 3.5 yr before its perihelion passage (10.38 au from the Sun). Later two pre-discovery observations were found from 11 October 2019 (heliocentric disctance: 10.45 au). In the moment of orbit determination, this comet was still observed.

Currently, solutions (GR and NG) based on pre-perihelion data are given. Therefore, the data arc span over 3.46 yr in a range of heliocentric distances from 10.45 au to 3.62 au.

This is Oort spike comet.
solution description
number of observations 3637
data interval 2019 10 11 – 2023 03 29
data arc selection data generally limited to pre-perihelion (PRE)
range of heliocentric distances 10.45 au – 3.62 au (perihelion) – 3.62 au
detectability of NG effects in the comet's motion comet with NG effects strongly manifested in positional data fitting
type of model of motion GR - gravitational orbit
data weighting YES
number of residuals 7235
RMS [arcseconds] 0.35
orbit quality class 1a+
orbital elements (barycentric ecliptic J2000)
Epoch 1720 01 05
perihelion date 2023 03 29.38612211 ± 0.00011692
perihelion distance [au] 3.63082686 ± 0.00000095
eccentricity 0.99986704 ± 0.00000079
argument of perihelion [°] 181.493357 ± 0.000024
ascending node [°] 2.654324 ± 0.000003
inclination [°] 113.470499 ± 0.000003
reciprocal semi-major axis [10-6 au-1] 36.62 ± 0.22
file containing 5001 VCs swarm
2019u5pa.bmi
Time distribution of positional observations with corresponding heliocentric (red curve) and geocentric (green curve) distance at which they were taken. The horizontal dotted line shows the perihelion distance for a given comet whereas vertical dotted line — the moment of perihelion passage.
Six 2D-projections of the 6D space of original swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.