On the cometary nature of near-Earth asteroid 2003 EH1
- 作者: Babadzhanov P.B.1, Kokhirova G.I.1, Obrubov Y.V.2
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隶属关系:
- Institute of Astrophysics
- Kaluga Branch of Bauman State Technical University
- 期: 卷 32, 编号 5 (2016)
- 页面: 250-254
- 栏目: Dynamics and Physics of Bodies of the Solar System
- URL: https://ogarev-online.ru/0884-5913/article/view/177915
- DOI: https://doi.org/10.3103/S0884591316050044
- ID: 177915
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详细
Differential evolution of the orbits of near-Earth asteroid (NEA) 2003 EH1 and comet 96P/Machholz 1 under perturbing action of planets was investigated for the time interval of 28000 years. The similarity of the orbits was analyzed with the Southworth–Hawkins criterion DSH. It has been shown that both the comet and the asteroid can be fragments of a nucleus of the same larger comet being a progenitor of the Quadrantid complex. A break-up of the parent comet apparently occurred approximately 9500 years ago. NEA 2003 EH1 is actually a dormant fragment of a nucleus of the parent comet. It was concluded that comet 96P/Machholz 1, NEA (186256) 2003 EH1 of the Amore group, and the Quadrantid meteorite swarm form a family of related objects.
作者简介
P. Babadzhanov
Institute of Astrophysics
Email: kokhirova2004@mail.ru
塔吉克斯坦, Bukhoro 22, Dushanbe, 734042
G. Kokhirova
Institute of Astrophysics
编辑信件的主要联系方式.
Email: kokhirova2004@mail.ru
塔吉克斯坦, Bukhoro 22, Dushanbe, 734042
Yu. Obrubov
Kaluga Branch of Bauman State Technical University
Email: kokhirova2004@mail.ru
俄罗斯联邦, Bazhenova 2, Kaluga, 248000
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