系外行星
星光
切趾
望远镜
物理
直接成像
天体生物学
行星
航空航天工程
计算机科学
光学
天文
工程类
星星
作者
Manan Arya,Steve Warwick,David R. Webb,P. Douglas Lisman,Stuart Shaklan,Samuel C. Bradford,John Steeves,Evan Hilgemann,Brian Trease,Mark Thomson,Gregg Freebury,James G. McGown,Jamie Gull
摘要
An external occulter for starlight suppression – a starshade – flying in formation with the Habitable Exoplanet Imaging Mission Concept (HabEx) space telescope could enable the direct imaging and spectrographic characterization of Earthlike exoplanets in the habitable zone. This starshade is flown between the telescope and the star, and suppresses stellar light sufficiently to allow the imaging of the faint reflected light of the planet. This paper presents a mechanical architecture for this occulter, which must stow in a 5 m-diameter launch fairing and then deploy to about a 80 m-diameter structure. The optical performance of the starshade requires that the edge profile is accurate and stable. The stowage and deployment of the starshade to meet these requirements present unique challenges that are addressed in this proposed architecture. The mechanical architecture consists of a number of petals attached to a deployable perimeter truss, which is connected to central hub using tensioned spokes. The petals are furled around the stowed perimeter truss for launch. Herein is described a mechanical design solution that supports an 80 m-class starshade for flight as part of HabEx.
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