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C/2009 F6 (Yi–SWAN)

Non-periodic comet From Wikipedia, the free encyclopedia

C/2009 F6 (Yi–SWAN)
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C/2009 F6 (Yi–SWAN) is a non-periodic comet which first appeared in March 2009.

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Discovery and observations

On 4 April 2009, Robert D. Matson reported the discovery of a comet spotted from images taken by the SWAN instrument of the SOHO spacecraft.[5] Around the same time, Hereupon H. Yamaoka of the University of Tokyo received an email from South Korean astronomer, Dae-am Yi, where he reported that he had discovered the comet nine days earlier on 26 March, at the time a 12th-magnitude object within the constellation Lacerta.[4]

The comet was too dim to be seen by the naked eye, though it was observed through small telescopes. It is hard to watch because it is small with a tiny tail in the visible-light spectrum. The comet reached a peak magnitude of 8.3 on 6 April,[5] and passed 1.5 degrees south of the Double cluster in Perseus on 23 April.[6] Preliminary calculations of its orbit by Brian G. Marsden indicate the comet is traveling in a highly inclined parabolic orbit, tipped 85.7° to the plane of the ecliptic. It reached perihelion on 8 May, where it came as close as 1.27 AU (190 million km) from the Sun.[6]

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References

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