C/1996 E1 NEAT
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Comet C/1996 E1 was discovered on 15 March 1996 by Near-Earth-Asteroid Tracking Team (Jet Propulsion Laboratory), that is about 4.5 months before its perihelion passage.This comet was last observed in the mid-October 1996.
Comet had its closest approach to the Earth on 25 September 1996 (1.168 au), about 2 months after its perihelion passage.
This is a comet with nongravitational effects strongly manifested in positional data fitting.
Solutions given here are based on data spanning over 0.578 yr in a range of heliocentric distances: 2.31 au – 1.36 au (perihelion) – 1.76 au.
This Oort spike comet suffers rather moderate planetary perturbations during its passage through the planetary system; these perturbations lead to a more tight future orbit.
See also Królikowska 2014 and Królikowska 2020.
Comet had its closest approach to the Earth on 25 September 1996 (1.168 au), about 2 months after its perihelion passage.
This is a comet with nongravitational effects strongly manifested in positional data fitting.
Solutions given here are based on data spanning over 0.578 yr in a range of heliocentric distances: 2.31 au – 1.36 au (perihelion) – 1.76 au.
This Oort spike comet suffers rather moderate planetary perturbations during its passage through the planetary system; these perturbations lead to a more tight future orbit.
See also Królikowska 2014 and Królikowska 2020.
solution description | ||
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number of observations | 249 | |
data interval | 1996 03 15 – 1996 10 12 | |
data type | significantly more measurements before perihelion (PRE+) | |
data arc selection | entire data set (STD) | |
range of heliocentric distances | 2.31 au – 1.36 au (perihelion) – 1.76 au | |
type of model of motion | NS - non-gravitational orbits for standard g(r) | |
data weighting | YES | |
number of residuals | 492 | |
RMS [arcseconds] | 0.60 | |
orbit quality class | 1b |
orbital elements (barycentric ecliptic J2000) | ||
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Epoch | 1697 06 13 | |
perihelion date | 1996 07 27.31103445 | ± 0.00015327 |
perihelion distance [au] | 1.36236744 | ± 0.00000644 |
eccentricity | 0.99995892 | ± 0.00000621 |
argument of perihelion [°] | 81.089949 | ± 0.000331 |
ascending node [°] | 149.760222 | ± 0.000036 |
inclination [°] | 114.474859 | ± 0.000027 |
reciprocal semi-major axis [10-6 au-1] | 30.15 | ± 4.56 |
file containing 5001 VCs swarm |
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1996e1n1.bmi |
![](media/img/1996e1/1996e1n1a1res.png)
Upper panel: 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.
Lower panel (panels): O-C diagram for this(two) solution (solutions) given in this database, where residuals in right ascension are shown using magenta dots and in declination by blue open circles.
Lower panel (panels): O-C diagram for this(two) solution (solutions) given in this database, where residuals in right ascension are shown using magenta dots and in declination by blue open circles.