C/2014 B1 Schwartz
more info
Comet C/2014 B1 was discovered on 28 January 2014 with Tenagra Observatory near Nogales (U.S.A.), that is about 3.8 yr before its perihelion passage. This comet was observed until the end of 2019, and is still observable.
Comet had its closest approach to the Earth on 23 February 2018 (8.613 au), about 5.5 months after its perihelion passage. Similar close approach to the Earth was at the previous opposition on 11 February 2017 (8.664 au).
Solution given here is based on data spanning over 4.07 yr in a range of heliocentric distances: 11.97 au – 9.557 au (perihelion) – 9.60 au (23 February 2018).
This Oort spike comet suffers extremely slight planetary perturbations during its passage through the planetary system and its semimajor axis will be almost unchanged after leaving the planetary zone (see future barycentric orbits).

solution description
number of observations 689
data interval 2014 01 28 – 2018 02 23
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 11.97 au – 9.56 au (perihelion) – 9.6 au
detectability of NG effects in the comet's motion NG effects not determinable
type of model of motion GR - gravitational orbit
data weighting YES
number of residuals 1339
RMS [arcseconds] 0.29
orbit quality class 1a+
orbital elements (heliocentric ecliptic J2000)
Epoch 2017 09 04
perihelion date 2017 09 10.53692262 ± 0.00145105
perihelion distance [au] 9.55658183 ± 0.00000738
eccentricity 1.00374567 ± 0.00000498
argument of perihelion [°] 345.841812 ± 0.000070
ascending node [°] 161.395609 ± 0.000012
inclination [°] 28.37228 ± 0.00001
recip semi-major axis [10-6 au-1] -391.95 ± 0.52