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UVO to Far-IR (UVO-FIR) mirror technology development project is a multiyear effort initiated in Fiscal Year (FY) 2022 to mature the Technology Readiness Level (TRL) of critical technologies required to enable ultra-stable telescope of the Habitable Worlds Observatory (HWO) mission. 2023/24 accomplishments include: continued investigations into gravity sag by comparing rotation test vs flip test, quantifying gravity sag as a function of temperature and designing mount for mirror whose G-sag with elevation angle is only coma. Significant progress in developing a methodology for specify optical surface microstructure, contamination cleanliness level and allowable micrometeoroid impacts. Support of HWO. And, a parametric cost model for x-ray telescopes and a parametric volume cost model for normal incidence telescopes
H. Philip Stahl
"UVOIR to far-IR mirror technology development: year 2 status", Proc. SPIE 13134, Optical Manufacturing and Testing 2024, 131340D (30 September 2024); https://doi.org/10.1117/12.3028545
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H. Philip Stahl, "UVOIR to far-IR mirror technology development: year 2 status," Proc. SPIE 13134, Optical Manufacturing and Testing 2024, 131340D (30 September 2024); https://doi.org/10.1117/12.3028545