C/1914 M1 Neujmin
more info
Comet C/1914 M1 was discovered on 24 June 1914, about one month before perihelion passage, and was last seen on 10 August 1915 [Kronk, Cometography: Volume 3].
This comet made its closest approach to the Earth on 25 June 1914 (2.75 au), that is the next day after its discovery.
Solution given here is based on data spanning over 1.13 yr in a range of heliocentric distances from 3.76 au through perihelion (3.75 au) to 4.06 au.
This Oort spike comet suffers very slight planetary perturbations during its passage through the planetary system.
More details in Królikowska et al. 2014 andKrólikowska and Dybczyński 2017

solution description
number of observations 70
data interval 1914 06 24 – 1915 08 10
data type perihelion within the observation arc (FULL)
data arc selection entire data set (STD)
range of heliocentric distances 3.76 au – 3.75 au (perihelion) – 4.96 au
detectability of NG effects in the comet's motion NG effects not determinable
type of model of motion GR - gravitational orbit
data weighting NO
number of residuals 122
RMS [arcseconds] 2.21
orbit quality class 1b
orbital elements (barycentric ecliptic J2000)
Epoch 2217 08 27
perihelion date 1914 07 30.31310400 ± 0.01083300
perihelion distance [au] 3.74262397 ± 0.00006880
eccentricity 0.99996809 ± 0.00009356
argument of perihelion [°] 13.874513 ± 0.002108
ascending node [°] 271.460496 ± 0.000169
inclination [°] 71.079539 ± 0.000423
reciprocal semi-major axis [10-6 au-1] 8.53 ± 25.00
file containing 5001 VCs swarm
1914m1a5.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.