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LISA: Heliocentric formation design for the laser interferometer space antenna mission
Advances in Space Research ( IF 2.8 ) Pub Date : 2020-10-01 , DOI: 10.1016/j.asr.2020.09.034
Eric Joffre , Dave Wealthy , Christian Trenkel , Philipp Voigt , Tobias Ziegler , Waldemar Martens

Abstract The LISA (Laser Interferometer Space Antenna) mission has been selected by the European Space Agency’s Science Programme Committee as the third large-class mission of the Cosmic Vision Programme, addressing the science theme of the Gravitational Universe. With a planned launch date in 2034, LISA will be the first ever space-borne Gravitational Wave observatory, relying on laser interferometry between three spacecraft orbiting the Sun in a triangular formation. Airbus is currently leading an industrial Phase A system study on behalf of the European Space Agency. The paper will address the astrodynamics challenges associated with the LISA constellation design, driven by tight requirements on the geometric quality metrics of the near equilateral formation.

中文翻译:

LISA:激光干涉仪空间天线任务的日心编队设计

摘要 LISA(激光干涉仪空间天线)任务被欧洲航天局科学计划委员会选为宇宙视觉计划的第三个大型任务,解决了引力宇宙的科学主题。LISA 计划发射日期为 2034 年,它将成为有史以来第一个星载引力波天文台,它依赖于以三角形形式绕太阳运行的三个航天器之间的激光干涉测量。空中客车公司目前正在代表欧洲航天局领导一项工业 A 阶段系统研究。该论文将解决与 LISA 星座设计相关的天体动力学挑战,这是由对近等边地层几何质量指标的严格要求驱动的。
更新日期:2020-10-01
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