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
type of model of motion NC - non-gravitational orbits for symmetric CO-g(r)-like function
data weighting YES
number of residuals 5557
RMS [arcseconds] 0.41
orbit quality class 1a+
previous orbit statistics, both Galactic and stellar perturbations were taken into account
no. of returning VCs in the swarm 5001 *
no. of escaping VCs in the swarm 0
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 122.19 – 123.43 – 124.66
previous perihelion distance [au] 4.17594 – 4.17595 – 4.17596
previous aphelion distance [103 au] 16.04 – 16.2 – 16.36
time interval to previous perihelion [Myr] 0.717 – 0.728 – 0.739
percentage of VCs with qprev < 10100
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.
previous orbit statistics, here only the Galactic tide has been included
no. of returning VCs in the swarm 5001 *
no. of escaping VCs in the swarm 0
no. of hyperbolas among escaping VCs in the swarm 0
previous reciprocal semi-major axis [10-6 au-1] 122.19 – 123.43 – 124.66
previous perihelion distance [au] 4.16936 – 4.16976 – 4.17014
previous aphelion distance [103 au] 16.04 – 16.2 – 16.36
time interval to previous perihelion [Myr] 0.717 – 0.728 – 0.739
percentage of VCs with qprev < 10100