From Surf Wiki (app.surf) — the open knowledge base
147P/Kushida–Muramatsu
Periodic comet
Periodic comet
| Field | Value |
|---|---|
| name | 147P/Kushida–Muramatsu |
| discovery_ref | |
| discoverer | Yoshio Kushida |
| Osamu Muramatsu | |
| discovery_site | Yatsugatake, Japan |
| discovery_date | 8 December 1993 |
| mpc_name | P/1993 X1 |
| P/2000 T2 | |
| designations | 1993 XIX, 1993t |
| orbit_ref | |
| epoch | 17 October 2024 (JD 2460600.5) |
| observation_arc | 22.09 years |
| earliest_precovery_date | 7 December 1993 |
| obs | 290 |
| perihelion | 3.159 AU |
| aphelion | 4.859 AU |
| semimajor | 4.009 AU |
| period | 8.03 years |
| eccentricity | 0.21196 |
| inclination | 2.312° |
| asc_node | 91.667° |
| arg_peri | 348.57° |
| mean | 38.623° |
| tjup | 3.011 |
| Earth_moid | 1.769 AU |
| Jupiter_moid | 0.429 AU |
| dimensions | 0.42 km |
| rotation | hours |
| M1 | 13.6 |
| M2 | 16.7 |
| last_p | 6 December 2023 |
Osamu Muramatsu P/2000 T2
147P/Kushida–Muramatsu is a quasi-Hilda comet discovered in 1993 by Japanese astronomers Yoshio Kushida and Osamu Muramatsu.
Observational history
The comet was discovered photographically by Yoshio Kushida and Osamu Muramatsu from the Yatsugatake South Base Observatory on the night of 8 December 1993. Several orbital calculations by Shuichi Nakano later determined its periodic nature, at the time it has an orbital period of 7.40 years.
It was later recovered from the Saji Observatory on October 2000, where Brian G. Marsden and other astronomers were able to identify it as the same object as Kushida–Muramatsu of 1993.
Origin
According to calculations made by Katsuhiko Ohtsuka of the Tokyo Meteor Network and David Asher of Armagh Observatory, Kushida–Muramatsu was temporarily captured by Jupiter as an irregular moon between 14 May 1949, and 15 July 1962, ( years). It is the fifth such object known to have been captured.
It is thought that quasi-Hilda comets may be escaped Hilda asteroids. Comet Shoemaker–Levy 9, which collided with Jupiter in 1994, is a more famous example of a quasi-Hilda comet.
References
| display-authors= 3
| access-date= 7 August 2025 }}
| access-date= 1 June 2019 }}
| display-authors= 5 | doi-access= free }}
| doi-access= free }}
| access-date= 15 September 2009 | archive-date= 18 September 2009 | archive-url= https://web.archive.org/web/20090918085932/http://www.cosmosmagazine.com/news/3003/captured-comet-becomes-moon-jupiter | url-status= dead }}
| access-date= 18 June 2014 }}
| doi-access= free }}
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about 147P/Kushida–Muramatsu — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report