C/2018 V1 (Machholz–Fujikawa–Iwamoto)

Hyperbolic comet From Wikipedia, the free encyclopedia

C/2018 V1 (Machholz–Fujikawa–Iwamoto) is a comet that follows a slightly hyperbolic trajectory. It was visually discovered on 7 November 2018 by Donald Machholz using an 18.5-inch reflecting telescope,[3][4] and was independently co-discovered by Shigehisa Fujikawa and Masayuki Iwamoto respectively. It reached perihelion on 3 December 2018.

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C/2018 V1 (Machholz–Fujikawa–Iwamoto)
Path of the comet C/2018 V1 across the sky, with a 7-day motion shown
Discovery
Discovered byDonald Machholz
Shigehisa Fujikawa
Masayuki Iwamoto
Discovery siteColfax, California
Japan
Discovery date7 November 2018
Orbital characteristics[1]
Epoch16 November 2018 (JD 2458438.5)
Observation arc37 days
Number of
observations
750
Perihelion0.387 AU
Eccentricity1.00039
Inclination143.988°
128.722°
Argument of
periapsis
88.775°
Last perihelion3 December 2018
TJupiter–0.624
Earth MOID0.115 AU
Jupiter MOID2.567 AU
Physical characteristics[2]
Comet total
magnitude
(M1)
12.8
Comet nuclear
magnitude (M2)
17.1
7.5
(2018 apparition)
Close

Overview

It was estimated to be between 8 and 10th magnitude from mid-November to mid-December 2018, visible in a small telescope. It was discovered by three amateur astronomers: by an observer in Colfax, California, USA and by two observers in Japan.[5] The observations by three astronomers result in the name for the comet, Machholz-Fujikawa-Iwamoto.[3][6] The current orbit determination of this comet is based on 750 observations with a 37-day observation arc.[1]

Comet C/2018 V1 has a significant probability (72.6%) of having an extrasolar provenance although an origin in the Oort Cloud cannot be excluded.[7] As the present-day value of its barycentric orbital eccentricity is greater than 1, this comet is currently escaping from the Solar System, aiming for interstellar space.[7]

See also

References

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