Discovery | |
---|---|
Discovered by | Edward L. G. Bowell |
Discovery date | 11 February 1980 |
Orbital characteristics[1][2] | |
Epoch | 3 January 1982 (JD 2444972.5) |
Observation arc | 6.88 years |
Number of observations | 187 |
Aphelion | ~75,000 AU (inbound)[1] |
Perihelion | 3.3639 AU |
Eccentricity | 1.057(hyperbolic trajectory) 1.053 (epoch 1984+) |
Orbital period | ~7.1 million years (epoch 1950) Ejection (epoch 1977+) |
Inclination | 1.6617° |
114.558° | |
Argument of periapsis | 135.083° |
Last perihelion | 12 March 1982 |
Physical characteristics | |
Dimensions | > 1 km |
Comet total magnitude (M1) | 5.8 |
C/1980 E1 is a non-periodic comet discovered by Edward L. G. Bowell on 11 February 1980 and which came closest to the Sun (perihelion) in March 1982. It is leaving the Solar System on a hyperbolic trajectory due to a close approach to Jupiter. In the 43 years since its discovery only two objects with higher eccentricities have been identified, 1I/ʻOumuamua (1.2) and 2I/Borisov (3.35).[3][4]
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