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Deflection of fictitious asteroid 2017 PDC: Ion beam vs. kinetic impactor

机译:虚构小行星2017 PDC:离子束与动力学冲击器的偏转

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摘要

Mission scenarios for the deflection of fictitious asteroid 2017 PDC are investigated. Two deflection options, kinetic impactor (KI) and ion beam shepherd (IBS), are studied and compared on the basis of deflection performance, safety, as well as mission schedule and political aspects. Firstly, we propose the launch of a medium-size rendevous spacecraft equipped with at least two ionic thrusters that can serve as propulsion means for the interplanetary trajectory up to rendezvous with the asteroid and as contactless actuators for a possible follow-up deflection mission. The asteroid, whose uncertainty ellipsoid is initially too large to establish whether (and how) it should be deflected, is reached by the rendezvous spacecraft after a low-thrust interplanetary trajectory of reasonable duration. Following rendezvous the spacecraft is placed in the vicinity of the asteroid to estimate its mass, study its structure and composition and, crucially, reduce its uncertainty ellipsoid by ground tracking to confirm or rule out an impact. Assuming that an impact is confirmed two main deflection scenarios are considered based on the actual asteroid size. Ion beam deflection is considered with the possibility of full deflection (the asteroid misses the Earth by a safe margin) or impact location adjustment (the impact footprint is diplaced to the nearest unpopulated region) depending on the asteroid size and the predicted impact location. The launch of a kinetic impactor mission is also considered with the employment of the rendezvous spacecraft to measure the deflection outcome and possibly to refine the deflection in case it is needed. The deflection performance of the two methods is compared.
机译:调查了虚构小行星2017年PDC偏转的使命方案。在偏转性能,安全性以及任务时间表和政治方面的基础上,研究并比较了两个偏转选项,动力冲击器(KI)和离子束牧羊犬(IBS)。首先,我们建议推出配备有至少两个离子推进器的中型亚型航天器的发射,其可以用作行星轨迹的推进装置,该轨迹与小行星的与小行星和非接触式执行器一起用于可能的后续偏转任务。小行星,其不确定性椭球最初太大,无法建立它应该被偏转的(以及如何),在合理持续时间的低推力行星际轨迹之后,由Rendezvous航天器达到。在Rendezvous之后,航天器放置在小行星附近以估计其质量,研究其结构和组成,并且至关重要地,通过地面跟踪来降低其不确定性椭球以确认或排除影响。假设确认了影响,基于实际的小行星大小考虑了两个主要偏转场景。考虑离子束偏转,具有完全偏转的可能性(小行星通过安全裕度射击地球)或冲击位置调节(冲击足迹根据小行星尺寸和预测的冲击位置而透视到最近的未填充区域)。随着Rendezvous航天器的就业,也考虑了动力学影响团的推出,以衡量偏转结果,并且可能在需要时细化偏转。比较了两种方法的偏转性能。

著录项

  • 来源
    《Acta astronautica》 |2019年第3期|301-307|共7页
  • 作者单位

    Tech Univ Madrid Pl Cardenal Cisneros 3 Madrid 28040 Spain|Space Dynam Grp Madrid Spain;

    Tech Univ Madrid Pl Cardenal Cisneros 3 Madrid 28040 Spain|Space Dynam Grp Madrid Spain;

    Tech Univ Madrid Pl Cardenal Cisneros 3 Madrid 28040 Spain|Space Dynam Grp Madrid Spain;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
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