2023 DZ2 行星防御战役

IF 3.8 Q2 ASTRONOMY & ASTROPHYSICS
Vishnu Reddy, Michael S. Kelley, L. Benner, J. Dotson, N. Erasmus, Davide Farnocchia, Tyler Linder, Joseph R. Masiero, Cristina Thomas, J. Bauer, M. R. Alarcon, P. Bacci, D. Bamberger, Adam Battle, Z. Benkhaldoun, Guido Betti, M. Birlan, Marina Brozovic, B. Burt, D. Cantillo, Sunil Chandra, Grégoire Chomette, Ashley Coates, F. DeMeo, M. Devogéle, P. Fatka, M. Ferrais, P. Fini, Carel van Gend, J. Giorgini, Dmitry Glamazda, Robert Holmes, Joseph L. Hora, Shinji Horiuchi, K. Hornoch, Marco Iozzi, Cristóvão Jacques, E. Jehin, Hai Jiang, Galina Kaiser, P. Kušnirák, Eduard Kuznetsov, J. de León, A. Liakos, J. Licandro, Tim A. Lister, Jing Liu, A. López-Oquendo, M. Maestripieri, D. Mathias, Marco Micheli, S. Naidu, A. Nastasi, A. Nedelcu, E. Petrescu, M. Popescu, Stephen B Potter, P. Pravec, Juan A. Sanchez, T. Santana-Ros, M. Serra-Ricart, N. Sioulas, A. Sonka, Alessio Squilloni, M. Tombelli, M. Trelia, D. Trilling, Elizabeth M. Warner, G. Wells, L. Wheeler, Mike Wiles
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引用次数: 0

摘要

我们介绍了第四次行星防御演习的结果,这次演习的重点是小型近地小行星(NEA)2023 DZ2,在其于2023年3月接近地球期间进行。国际小行星警报网(IAWN)在美国国家航空航天局行星防御协调办公室(PDCO)的支持下,自2017年以来一直在协调行星防御观测活动,以测试全球行星防御能力的运行准备情况。上一次活动的重点是近地天体 "阿波菲斯"(Apophis),这次活动的一个成果是需要开展一次短时间爆发活动,以复制现实生活中的近地天体撞击危险场景。2023 年 DZ2 活动的目标是将小型近地天体描述为潜在的撞击者,并演练行星防御系统,包括观测、假设风险评估和风险预测,以及在短短 24 小时内进行危害通报。活动小组根据特征描述方法分为几个工作组:光度测量、光谱学、热红外光度测量和光学偏振测量、雷达和风险评估。这次活动的科学结果表明,2023 DZ2 的旋转周期为 6.2745 ± 0.0030 分钟;可见光波长彩色测光/光谱/偏振和近红外光谱仪均表明该天体属于 E 型分类,其表面成分类似于奥比陨石;雷达观测表明,该天体的直径为 30 ± 10 米,与偏振和热红外观测得出的高反照率(0.49)相一致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
2023 DZ2 Planetary Defense Campaign
We present the results of a fourth planetary defense exercise, focused this time on the small near-Earth asteroid (NEA) 2023 DZ2 and conducted during its close approach to the Earth in 2023 March. The International Asteroid Warning Network (IAWN), with support from NASA's Planetary Defense Coordination Office (PDCO), has been coordinating planetary defense observational campaigns since 2017 to test the operational readiness of the global planetary defense capabilities. The last campaign focused on the NEA Apophis, and an outcome of that exercise was the need for a short burst campaign to replicate a real-life near-Earth object impact hazard scenario. The goal of the 2023 DZ2 campaign was to characterize the small NEA as a potential impactor and exercise the planetary defense system including observations, hypothetical risk assessment and risk prediction, and hazard communication with a short notice of just 24 hr. The entire campaign lasted about 10 days. The campaign team was divided into several working groups based on the characterization method: photometry, spectroscopy, thermal IR photometry and optical polarimetry, radar, and risk assessment. Science results from the campaign show that 2023 DZ2 has a rotation period of 6.2745 ± 0.0030 minutes; visible wavelength color photometry/spectroscopy/polarimetry and near-IR spectroscopy all point to an E-type taxonomic classification with surface composition analogous to aubrite meteorites; and radar observations show that the object has a diameter of 30 ± 10 m, consistent with the high albedo (0.49) derived from polarimetric and thermal IR observations.
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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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