DART 撞击前后迪迪莫斯系统的动力学状态

IF 3.8 Q2 ASTRONOMY & ASTROPHYSICS
Derek C. Richardson, Harrison F. Agrusa, Brent Barbee, Rachel H. Cueva, Fabio Ferrari, Seth A. Jacobson, Rahil Makadia, Alex J. Meyer, Patrick Michel, Ryota Nakano, Yun Zhang, Paul Abell, Colby C. Merrill, Adriano Campo Bagatin, Olivier Barnouin, Nancy L. Chabot, Andrew F. Cheng, Steven R. Chesley, R. Terik Daly, Siegfried Eggl, Carolyn M. Ernst, Eugene G. Fahnestock, Tony L. Farnham, Oscar Fuentes-Muñoz, Edoardo Gramigna, Douglas P. Hamilton, Masatoshi Hirabayashi, Martin Jutzi, Josh Lyzhoft, Riccardo Lasagni Manghi, Jay McMahon, Fernando Moreno, Naomi Murdoch, Shantanu P. Naidu, Eric E. Palmer, Paolo Panicucci, Laurent Pou, Petr Pravec, Sabina D. Raducan, Andrew S. Rivkin, Alessandro Rossi, Paul Sánchez, Daniel J. Scheeres, Peter Scheirich, Stephen R. Schwartz, Damya Souami, Gonzalo Tancredi, Paolo Tanga, Paolo Tortora, Josep M. Trigo-Rodríguez, Kleomenis Tsiganis, John Wimarsson, Marco Zannoni
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引用次数: 0

摘要

美国航天局的双小行星改向试验(DART)航天器于2022年9月26日撞击了迪迪莫斯(65803)的天然卫星迪莫莫斯(Dimorphos),这是对动能撞击器技术在空间偏转潜在危险物体的首次成功试验。这次试验导致迪迪莫斯系统的动力学状态发生了微小变化,符合预期和一级任务要求。在撞击前的论文中,对 "迪迪莫斯 "系统撞击前和撞击后的动力学状态进行了预测。在此,我们对这些预测进行了评估,更新了撞击后发表的初步发现,报告了与动力学有关的新发现,并提供了对欧空局计划于2024年10月发射、2026年12月到达迪迪莫斯的赫拉(Hera)任务的影响。迄今为止测试的撞击前预测与观测结果基本一致,尽管与雷达模型相比,迪迪莫斯的外观出乎意料地扁平,而且迪莫莫斯在撞击前明显呈扁球形(对系统起源的影响仍在调查中)。新的发现包括:迪莫莫斯很可能由于撞击而变得扁长,并可能进入了翻滚旋转状态。可能探测到撞击后双星轨道周期瞬时性下降,这表明可能与持续喷出物发生了动力学耦合。抑制任何翻滚和清除任何碎片的时间尺度尚不确定。DART撞击的动量传递增强因子的最大不确定性仍然是Dimorphos的质量,这将由Hera任务来解决。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Dynamical State of the Didymos System before and after the DART Impact
NASA’s Double Asteroid Redirection Test (DART) spacecraft impacted Dimorphos, the natural satellite of (65803) Didymos, on 2022 September 26, as a first successful test of kinetic impactor technology for deflecting a potentially hazardous object in space. The experiment resulted in a small change to the dynamical state of the Didymos system consistent with expectations and Level 1 mission requirements. In the preencounter paper, predictions were put forward regarding the pre- and postimpact dynamical state of the Didymos system. Here we assess these predictions, update preliminary findings published after the impact, report on new findings related to dynamics, and provide implications for ESA’s Hera mission to Didymos, scheduled for launch in 2024 October with arrival in 2026 December. Preencounter predictions tested to date are largely in line with observations, despite the unexpected, flattened appearance of Didymos compared to the radar model and the apparent preimpact oblate shape of Dimorphos (with implications for the origin of the system that remain under investigation). New findings include that Dimorphos likely became prolate due to the impact and may have entered a tumbling rotation state. A possible detection of a postimpact transient secular decrease in the binary orbital period suggests possible dynamical coupling with persistent ejecta. Timescales for damping of any tumbling and clearing of any debris are uncertain. The largest uncertainty in the momentum transfer enhancement factor of the DART impact remains the mass of Dimorphos, which will be resolved by the Hera mission.
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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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