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C/2018 V1 (Machholz–Fujikawa–Iwamoto)
Hyperbolic comet From Wikipedia, the free encyclopedia
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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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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]
- Perihelion in early December 2018, above the orbit of Mercury
- Animation of C/2018 V1's orbit
Sun · Mercury · Venus · Earth · Mars · C/2018 V1
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