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C/1941 B2 (de Kock–Paraskevopoulos)
Non-periodic comet From Wikipedia, the free encyclopedia
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Comet de Kock–Paraskevopoulos (also known with the designations C/1941 B2, 1941 IV, 1941c) is a non-periodic comet discovered on 15 January 1941. The comet reached an apparent magnitude of about +2.[6]
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Observational history
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The comet was first observed by Reginald Purdon de Kock in Paarl, South Africa while he was observing variable star R Lupi on 15 January 1941 and notified the Royal Observatory. He estimated the comet had a magnitude of 5.8 and its tail was half a degree long.[7] The comet was independently discovered by Frank Skjellerup in Melbourne on 20 January and confirmed the discovery the next day, while a person named Barnes also notified Melbourne Observatory about the comet on 21 January.[7] John S. Paraskevopoulos of the Harvard College Observatory in Bloemfontein, unaware of the other discoveries, found the comet on 23 January and sent immediately a radiogram in Harvard College, and thus the comet became known in the United States as comet Paraskevopoulos.[7]
The comet brightened rapidly to a magnitude of 2 to 3 the next days, while its tail was reported to be about 5 degrees long. The comet reached its perihelion on 27 January and two days later was the closest approach to Earth, at a distance of 0.2655 AU. On 27 January the comet also reached its southernmost declination, at -57°.[7] On that day, Harley Weston Wood reported a magnitude of 3.26 at a tail length of 5° by naked eye. The comet brightened a bit more the following days, with Ronald Alexander McIntosh reporting magnitude 2.2 and a tail length of 6 degrees on 31 January.[7]
In February the comet began to fade, as it was moving away both from Earth and the Sun.[7] The tail appeared bent the first days of the month. By the mid of February the comet had faded to a magnitude of about 5 and stopped being visible with naked eye.[8] In March the solar elongation decreased and the comet passed 0.6 degrees from the Sun on April 28. The comet was recovered on 4 July by George van Biesbroeck and was last detected on 27 September 1941.[7]
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References
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