Habitable-Zone Exoplanet Observatory (HabEx) Baseline 4-M Telescope Design and Predicted Performance

Stahl, H Philip ; Kuan, Gary ; Arnold, Willian ; Baysinger, Mike ; Brooks, Thomas ; Cormarkovic, Velibor ; Davis, Jacqueline ; Garcia, Jay ; Gaskin, Jonathan ; Knight, J Brent(NASA Marshall Space Flight Center, Huntsville, AL, United States)

关键词: DESIGN ANALYSIS;    EXTRASOLAR PLANETS;    HABITABILITY;    IMAGING TECHNIQUES;    INFRARED TELESCOPES;    LINE OF SIGHT;    MODELS;    OBSERVATORIES;    SPECIFICATIONS;    SPECTROSCOPY;    ULTRAVIOLET TELESCOPES;    WAVE FRONTS;   

RP-ID  :  MSFC-E-DAA-TN71282

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来源: NASA Technical Reports Server

【 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 planetary systems in the habitable zone around nearby sun-like stars. Additionally, HabEx will perform a broad range of general astrophysics science enabled by 100 to 2500 nm spectral range and 3 x 3 arc-minute FOV. Critical to achieving its the HabEx 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-mirror-anastigmatic, 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.