Dimorphos的轨道周期变化以及DART撞击后重塑造成的姿态扰动

IF 3.8 Q2 ASTRONOMY & ASTROPHYSICS The Planetary Science Journal Pub Date : 2024-06-01 DOI:10.3847/PSJ/ad4350
R. Nakano, M. Hirabayashi, S. Raducan, P. Pravec, S. Naidu, H. Agrusa, S. Chesley, F. Ferrari, M. Jutzi, C. C. Merrill, A. J. Meyer, P. Michel, Derek C. Richardson, P. Sánchez, Peter Scheirich, S. R. Schwartz, Yun Zhang, A. C. Bagatin, Po-Yen Liu, A. F. Cheng
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引用次数: 0

摘要

2022年9月26日(世界协调时),美国宇航局的双小行星重定向测试(DART)任务成功撞击了近地双小行星系统(65803)Didymos的次要组成部分Dimorphos。随后的地基观测表明,迪莫莫斯发生了显著的重塑,其赤道轴比从1.06变为1.3。在此,我们报告了这一重塑事件对Dimorphos轨道和姿态的影响。根据报告的重塑幅度,我们的相互动力学模拟显示,在DART撞击后观测到的33分钟轨道周期变化中,大约有125秒可能是重塑造成的。然而,这一数值对狄莫弗斯撞击后轴比的精确值非常敏感,其变化幅度可能是这一数值的2倍,在目前的不确定范围内可能达到约250秒。虽然按照目前估计的轴比,该天体的旋转状态是稳定的,但即使是这些轴比的微小变化或形状不对称的引入也会使其姿态不稳定。撞击直接对迪莫弗斯的轨道和旋转状态造成的扰动,再加上任何重塑,都极有可能导致其出现翻滚旋转状态。为了通过欧洲航天局赫拉航天器的测量准确确定动量增强因子(β),并评估动能偏转技术在未来行星防御计划中的有效性,重塑的影响不容忽视。
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Dimorphos’s Orbit Period Change and Attitude Perturbation due to Its Reshaping after the DART Impact
On 2022 September 26 (UTC), NASA's Double Asteroid Redirection Test (DART) mission achieved a successful impact on Dimorphos, the secondary component of the near-Earth binary asteroid system (65803) Didymos. Subsequent ground-based observations suggest a significant reshaping of Dimorphos, with its equatorial axis ratio changing from 1.06 to ∼1.3. Here we report the effects of this reshaping event on Dimorphos's orbit and attitude. Given the reported reshaping magnitude, our mutual dynamics simulations show that approximately 125 s of the observed 33 minute orbit period change after the DART impact may have resulted from reshaping. This value, however, is sensitive to the precise values of Dimorphos's post-impact axis ratios and may vary by up to 2 times that amount, reaching approximately 250 s within the current uncertainty range. While the rotational state of the body is stable at the currently estimated axis ratios, even minor changes in these ratios or the introduction of shape asymmetry can render its attitude unstable. The perturbation to Dimorphos’s orbital and rotational state delivered by the impact directly, combined with any reshaping, leads to a strong possibility for a tumbling rotation state. To accurately determine the momentum enhancement factor (β) through measurements by the European Space Agency’s Hera spacecraft and to evaluate the effectiveness of the kinetic deflection technique for future planetary defense initiatives, the effects of reshaping should not be overlooked.
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来源期刊
The Planetary Science Journal
The Planetary Science Journal Earth and Planetary Sciences-Geophysics
CiteScore
5.20
自引率
0.00%
发文量
249
审稿时长
15 weeks
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