Yarkovsky-driven impact risk analysis for asteroid (99942) Apophis

被引:99
作者
Farnocchia, D. [1 ]
Chesley, S. R. [1 ]
Chodas, P. W. [1 ]
Micheli, M. [2 ]
Tholen, D. J. [2 ]
Milani, A. [3 ]
Elliott, G. T. [2 ]
Bernardi, F. [4 ]
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[3] Univ Pisa, Dipartimento Matemat, I-56127 Pisa, Italy
[4] SpaceDyS, I-56023 Pisa, Italy
基金
美国国家科学基金会;
关键词
Asteroids; Dynamics; Celestial mechanics; Near-Earth objects; Orbit determination; NEAR-EARTH ASTEROIDS; ENCOUNTERS;
D O I
10.1016/j.icarus.2013.02.020
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We assess the risk of an Earth impact for asteroid (99942) Apophis by means of a statistical analysis accounting for the uncertainty of both the orbital solution and the Yarkovsky effect. We select those observations with either rigorous uncertainty information provided by the observer or a high established accuracy. For the Yarkovsky effect we perform a Monte Carlo simulation that fully accounts for the uncertainty in the physical characterization, especially for the unknown spin orientation. By mapping the uncertainty information onto the 2029 b-plane and identifying the keyholes corresponding to subsequent impacts we assess the impact risk for future encounters. In particular, we find an impact probability greater than 10(-6) for an impact in 2068. We analyze the stability of the impact probability with respect to the assumptions on Apophis' physical characterization and consider the possible effect of the early 2013 radar apparition. (C) 2013 Elsevier Inc. All rights reserved.
引用
收藏
页码:192 / 200
页数:9
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