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HabEx Baseline Telescope: Design & Predicted PerformanceHabitable Exoplanet Observatory Mission (HabEx) will image & 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 a 150 to 1700 nm spectral range and 3 x 3 arc-minute FOV. Critical to achieving the HabEx science goals is a large, ultra-stable telescope. The baseline HabEx telescope is a 4-m off-axis unobscured three-mirror-anastigmatic design with diffraction limited performance at 400 nm and wavefront stability of picometers per mK. These specifications are driven by science requirements. STOP (structural thermal optical performance) analysis predicts that the baseline telescope’s opto-mechanical design meets its specified performance tolerances.
Document ID
20200000407
Acquisition Source
Marshall Space Flight Center
Document Type
Poster
Authors
Stahl, H. Philip
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
January 16, 2020
Publication Date
January 6, 2020
Subject Category
Astrophysics
Report/Patent Number
MSFC-E-DAA-TN75627
Report Number: MSFC-E-DAA-TN75627
Meeting Information
Meeting: American Astronomical Society Meeting
Location: Honolulu, HI
Country: United States
Start Date: January 4, 2020
End Date: January 8, 2020
Sponsors: American Astronomical Society
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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