望远镜
天文台
系外行星
星周宜居带
物理
基线(sea)
天文
有源光学
波前
光学望远镜
行星
遥感
光学
地质学
海洋学
作者
H. Philip Stahl,Gary Kuan,William R. Arnold,Mike Baysinger,Thomas Brooks,Jay Garcia,James B. Knight
出处
期刊:Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave
日期:2020-12-13
摘要
The Habitable Exoplanet Observatory Mission (HabEx) is one of four missions under study for the 2020 Astrophysics Decadal Survey. Its goal is to directly image and spectroscopically characterize planets in the habitable zone around nearby sun-like stars. Additionally, HabEx will perform a broad range of general astrophysics science enabled by 115 to 1700 nm spectral range and 3x3 arc-minute FOV instruments. Critical to achieving its science goals is a large, ultra-stable UV/Optical/Near-IR (UVOIR) telescope. The baseline HabEx telescope is a 4-meter off-axis unobscured three-mirroranastigmatic, diffraction limited at 400 nm with wavefront stability on the order of a few 10s of picometers. This paper summarizes the opto-mechanical design of the HabEx baseline optical telescope assembly, including a discussion of how science requirements drive the telescope’s specifications, and presents analysis that the baseline telescope structure meets its specified tolerances.
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