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Non-periodic comet From Wikipedia, the free encyclopedia
Comet Skorichenko–George (sometimes spelled Scorichenko–George), formally designated as C/1989 Y1, 1990 VI, and 1989e1, is a non-periodic comet co-discovered by astronomers Boris Skorichenko and Doug George on December 17, 1989. It has a hyperbolic trajectory around the Sun,[3] but still weakly bound to it by its barycenter.[4]
Discovery[1][2] | |
---|---|
Discovered by | Boris Skoritchenko Douglas B. George |
Discovery date | 17 December 1989 |
Designations | |
1990 VI 1989e1 | |
Orbital characteristics[3][4] | |
Epoch | 24 February 1990 (JD 2447946.5) |
Observation arc | 1,008 days (2.76 years) |
Number of observations | 106 |
Aphelion | 1,188.42 AU |
Perihelion | 1.569 AU |
Semi-major axis | 594.994 AU |
Eccentricity | 0.997363 |
Orbital period | 14,514 years |
Inclination | 59.3660 |
279.998° | |
Argument of periapsis | 137.862° |
Last perihelion | 11 April 1990 |
Earth MOID | 0.7346 AU |
Jupiter MOID | 1.8047 AU |
Physical characteristics[3] | |
Comet total magnitude (M1) | 5.3 |
Comet nuclear magnitude (M2) | 11.9 |
9–10 (1990 apparition) |
It was discovered on December 17, 1989 by Doug George of Kanata (near Ottawa), Ontario, Canada, and Soviet astronomer Boris Skoritchenko (Mezmay, Krasnodar Krai). Skoritchenko was using 8×20 binoculars,[5] whilst George was using a 16" reflector and had searched for 65 hours[6]. The comet was magnitude 10.5 in the northern evening sky. It passed its perihelion on April 11, 1990 at a distance of 1.57 AU (235 million km),[3] and remained visible as a magnitude 9–10 object in the night sky until April 1990
C2 emission bands were observed in the comet Skorichenko-George. Unlike most comets, Skorichenko–George did not produce a tail.[7] Its coma remained consistently diffuse, estimated to be around 190,000–290,000 km (120,000–180,000 mi) in diameter.[7]
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