Paper
7 September 2013 The development of stacked core technology for the fabrication of deep lightweight UV-quality space mirrors
Gary W. Matthews, Charles S. Kirk, Steven P. Maffett, Calvin E. Abplanalp, H. Philip Stahl, Michael R. Effinger
Author Affiliations +
Abstract
The Decadal Survey stated that an advanced large-aperture ultraviolet, optical, near-infrared (UVOIR) telescope is required to enable the next generation of compelling astrophysics and exoplanet science; and, that present technology is not mature enough to affordably build and launch any potential UVOIR mission concept. Under Science and Technology funding, NASA’s Marshall Space Flight Center (MSFC) and Exelis have developed a more cost effective process to make up to 4m monolithic spaceflight UV quality, low areal density, thermally and dynamically stable primary mirrors. A proof of concept mirror was completed at Exelis and tested down to 250K at MSFC which would allow imaging out to 2.5 microns. The parameters and test results of this concept mirror will be shown. The scale-up process will be discussed and the technology development path to a 4m mirror system by 2018 will also be outlined.
© (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gary W. Matthews, Charles S. Kirk, Steven P. Maffett, Calvin E. Abplanalp, H. Philip Stahl, and Michael R. Effinger "The development of stacked core technology for the fabrication of deep lightweight UV-quality space mirrors", Proc. SPIE 8838, Optical Manufacturing and Testing X, 88380L (7 September 2013); https://doi.org/10.1117/12.2024630
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Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

Space mirrors

Ultraviolet radiation

Space telescopes

Glasses

Hubble Space Telescope

Optical testing

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