C/2014 A4 SONEAR
more info
Comet C/2014 A4 was discovered on 12 January 2014 with Southern Observatory for Near Earth Research (Oliveira, Brazil), that is about 8 months before its perihelion passage. This comet was observed during five oppositions until 17 September 2017.
Comet had its closest approach to the Earth on 19 October 2015 (3.203 au), about 1.5 month after its perihelion passage.
Solutions given here are based on data spanning over 3.68 yr in a range of heliocentric distances: 6.40 au – 4.180 au (perihelion) – 7.21 au.
This comet suffers small planetary perturbations during its passage through the planetary system; these perturbations lead to a more tight future orbit (see future barycentric orbits).

solution description
number of observations 2825
data interval 2014 01 12 – 2017 09 17
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 6.4 au – 4.18 au (perihelion) – 7.21 au
detectability of NG effects in the comet's motion comet with determinable NG~orbit
type of model of motion GR - gravitational orbit
data weighting YES
number of residuals 5510
RMS [arcseconds] 0.39
orbit quality class 1a+
orbital elements (barycentric ecliptic J2000)
Epoch 2322 09 06
perihelion date 2015 09 05.56926740 ± 0.00007427
perihelion distance [au] 4.18289818 ± 0.00000061
eccentricity 0.99884836 ± 0.00000123
argument of perihelion [°] 356.715815 ± 0.000010
ascending node [°] 29.704294 ± 0.000002
inclination [°] 121.334438 ± 0.000004
reciprocal semi-major axis [10-6 au-1] 275.32 ± 0.29
file containing 5001 VCs swarm
2014a4a5.bpl
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 future swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.