Presentation + Paper
11 September 2019 Dynamic analyses of the proposed habitable exoplanet astrophysics facility
Author Affiliations +
Abstract
The proposed Habitable Exoplanet (HabEx) astrophysics facility is one of four large such facilities being proposed to the 2020 decadal. It is a large telescope that is sensitive to ultraviolet, optical, and near-infrared photons. The proposed design’s overall length is on the order of 17.2 m and its maximum cross section is on the order of 5.25 × 5.25 m. The primary mirror is 4 m in diameter. A transient dynamic analysis was performed to estimate the order of magnitude of ring down time after moving the telescope and pointing at a new target for science planning purposes. Without uncertainty factors, results from a simple re-pointing maneuver indicate that primary to secondary mirror LOS errors are on the order of 10-4 pico-m after 5 minutes. Also, a frequency response analysis was performed to predict the impact of planned micro-thruster vibrations on required stability. Based on provided noise level associated with the micro-thrusters and loading assumptions and without uncertainty factors, the assessed vibrations do not impact predicted performance requirements.
Conference Presentation
© (2019) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. Brent Knight, H. Philip Stahl, and Thomas Brooks "Dynamic analyses of the proposed habitable exoplanet astrophysics facility", Proc. SPIE 11103, Optical Modeling and System Alignment, 111030F (11 September 2019); https://doi.org/10.1117/12.2530385
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KEYWORDS
Finite element methods

Astrophysics

Mirrors

Exoplanets

Telescopes

Systems modeling

Infrared telescopes

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