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Habitable exoplanet imaging mission (HabEx): initial flight system design

机译:可居住的外产成像使命(Habex):初始飞行系统设计

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The Habitable Exoplanet Imaging Mission (HabEx) is a concept for a mission to directly image planetary systems around Sun-like stars and to perform general astrophysics investigations being studied as part of a number of mission concepts for the upcoming 2020 Astrophysics Decadal Survey. HabEx would help assess the prevalence of habitable planets in our galaxy, searching in particular for potential biosignatures in the atmospheres of planets in habitable zones. More generally, HabEx would image our neighboring solar systems and characterize the variety of planets that inhabits them. Its direct imaging capability would also enable the mission to study the structure and evolution of debris disks around nearby stars, and their dynamical interaction with planets. Additionally, it will explore a number of more general astrophysics phenomena in our solar system, galaxy, and beyond, in the UV through NIR range. The exoplanet science goals lead to a mission concept with requirements for high contrast imaging and the continuous spectral coverage. The baseline for HabEx is a 4-meter diameter off-axis telescope designed to both search for habitable planets and perform general astrophysics observations, possibly combined with a starshade. In this paper, the initial flight system design for both the telescope and the starshade are presented, focusing on the key and driving requirements and subsystems, as well as the trajectory and station keeping and formation flying technique. Furthermore, some of the initial design trades undergone are described, as well as the key challenges and enablers. Finally, some of the future design and architecture trades to be performed within the flight systems as part of the continuing effort in the HabEx study are discussed.
机译:可居住的外产成像使命(Habex)是一项使命的特派团直接围绕太阳恒星的行星系统,并进行一般的天体物理调查,作为即将到来的2020个天体物理学过度调查的一些任务概念的一部分进行研究。 Habex将有助于评估我们的银河系中可居住行星的普遍存在,特别是在人行星中的潜在生物系列中寻找潜在的生物系列。更一般地,Habex会映像我们邻近的太阳系,并表征居住的各种行星。它的直接成像能力还将使命能够研究附近恒星周围的碎片磁盘的结构和演变,以及与行星的动态相互作用。此外,它将在UV通过NIR范围内探索我们太阳系,星系和超越的许多一般的天体物理现象。 Exoplanet科学目标导致特派团概念,具有高对比度成像和连续光谱覆盖的要求。 Habex的基线是一个4米直径的离轴望远镜,旨在搜索可居住的行星并进行一般的天体物理观察,可能与六角形相结合。在本文中,提出了望远镜和六角形的初始飞行系统设计,专注于关键和驾驶要求和子系统,以及轨迹和站保持和形成飞行技术。此外,描述了一些初始设计交易,以及关键挑战和推动者。最后,讨论了一些未来的设计和建筑交易作为Habex研究中的继续努力的一部分,将在飞行系统内进行。

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