천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제37권1호
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- Pages.101.2-101.2
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- 2012
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- 1226-2692(pISSN)
Physical properties of Maria asteroid family
- Kim, Myung-Jin (Department of Astronomy, Yonsei University) ;
- Choi, Young-Jun (Korea Astronomy and Space Science Institute) ;
- Moon, Hong-Kyu (Korea Astronomy and Space Science Institute) ;
- Brosch, Noah (Tel Aviv University) ;
- Byun, Yong-Ik (Department of Astronomy, Yonsei University)
- 발행 : 2012.04.03
초록
An asteroid family is a population of asteroids in the proper orbital element space (a, e, i), considered to have been produced by a disruption of a large parent body presumably through a catastrophic collision. Asteroid families offer unique opportunities to reconstruct and characterize the break-up history of airless bodies in the main-belt. The Maria family is a typical old population (~3
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