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Aligning the Demonstration Model of CHEOPS

机译:对齐Cheops的演示模型

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CHEOPS (CHaracterizing ExOPlanets Satellite) is an ESA Small Mission, planned to be launched in mid-2018 and whose main goal is the photometric precise characterization of radii of exoplanets orbiting bright stars (V<12) already known to host planets. Given the fast-track nature of this mission, we developed a non-flying Demonstration Model, whose optics are flight representative and whose mechanics provides the same interfaces of the flight model, but is not thermally representative. In this paper, we describe CHEOPS Demonstration Model handling, integration, tests, alignment and characterization, emphasizing the verification of the uncertainties in the optical quality measurements introduced by the starlight simulator and the way the alignment and optical surfaces are measured.
机译:Cheops(表征Exoplanets Satellite)是一个ESA小使命,计划于2018年中期推出,其主要目标是Exping亮恒星(V <12)已经已知主体行星的明亮恒星(V <12)的光度精确表征。鉴于这项任务的快速性质,我们开发了一个非飞行的示范模型,其光学器件是飞行代表,其力学提供飞行模型的相同界面,但并不是热代表性。在本文中,我们描述了Cheops演示模型处理,集成,测试,对准和表征,强调验证由星光模拟器引入的光学质量测量中的不确定性以及测量对准和光学表面的方式。

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