C/1955 G1 Abell
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Comet C/1955 G1 was discovered on 13 April 1955, a year and three weeks after perihelion passage, and was last seen on 30 April 1956 [Kronk, Cometography: Volume 4].
The comet made two close approaches to the Earth: on 24 July 1953 (4.09 au, eight months before perihelion passage), and on 21 May 1954 (4.03 au, two months after perihelion).
Solution given here is based on data spanning over 1.1 yr in a range of heliocentric distances from 5.45 au to 7.42 au.
This Oort spike comet suffers small planetary perturbations during its passage through the planetary system that lead to escape the comet from the planetary zone on a hyperbolic orbit (see future barycentric orbit).
See also Królikowska and Dybczyński 2017.
The comet made two close approaches to the Earth: on 24 July 1953 (4.09 au, eight months before perihelion passage), and on 21 May 1954 (4.03 au, two months after perihelion).
Solution given here is based on data spanning over 1.1 yr in a range of heliocentric distances from 5.45 au to 7.42 au.
This Oort spike comet suffers small planetary perturbations during its passage through the planetary system that lead to escape the comet from the planetary zone on a hyperbolic orbit (see future barycentric orbit).
See also Królikowska and Dybczyński 2017.
| solution description | ||
|---|---|---|
| number of observations | 35 | |
| data interval | 1955 04 13 – 1956 04 30 | |
| data type | observed only after perihelion (POST) | |
| data arc selection | entire data set (STD) | |
| range of heliocentric distances | 5.45 au – 7.42au | |
| 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 | 63 | |
| RMS [arcseconds] | 1.00 | |
| orbit quality class | 1b | |
| orbital elements (barycentric ecliptic J2000) | ||
|---|---|---|
| Epoch | 1649 01 16 | |
| perihelion date | 1954 03 25.00060911 | ± 0.01192894 |
| perihelion distance [au] | 4.49692869 | ± 0.00010950 |
| eccentricity | 0.99963621 | ± 0.00007649 |
| argument of perihelion [°] | 73.796250 | ± 0.001859 |
| ascending node [°] | 321.294299 | ± 0.000333 |
| inclination [°] | 123.952116 | ± 0.000276 |
| reciprocal semi-major axis [10-6 au-1] | 80.90 | ± 17.01 |
| file containing 5001 VCs swarm |
|---|
| 1955g1a1.bmi |
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 original swarm including 5001 VCs. Each density map is given in logarithmic scale presented on the right in the individual panel.