C/1490 Y1

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Discoverydate31 December 1490
Epoch26 December 1490 (JD 2265638.47)
C/1490 Y1
Discovery[1]
Discovery siteChina
Discovery date31 December 1490
Designations
1491 I[2]
Orbital characteristics[3][4]
Epoch26 December 1490 (JD 2265638.47)
Observation arc22 days
Number of
observations
3
Aphelion(Lee et al.) 5.32 AU; (JPL) not defined
Perihelion(Lee et al.) 0.769 AU; (JPL) 0.738 AU
Semi-major axis(Lee et al.) 3.040 AU; (JPL) not defined
Eccentricity(Lee et al.) 0.75; (JPL) 1.0
Orbital period(Lee et al.) 5.30 years; (JPL) not defined
Inclination(Lee et al.) 70.2°; (JPL) 51.6°
(Lee et al.) 283°; (JPL) 296°
Argument of
periapsis
(Lee et al.) 164°; (JPL) 130°
Last perihelion24 December 1490
(observed)
Next perihelionUncertain
(Presumed periodic)
Physical characteristics[1]
5.4
(1491 apparition)

C/1490 Y1 is a comet that was recorded and observed across East Asia, particularly China and Korea, from December 1490 to February 1491. It is believed to be the parent body of the Quadrantids meteor shower.[citation needed]

John Russell Hind,[5] Benjamin Peirce, and Ichiro Hasegawa[6] made the initial orbital calculations for the comet, which all resulted in a parabolic trajectory around the Sun.[1]

See also

References

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