Abstract
NASA's Marshall Space Flight Center (MSFC) maintains an active research program toward the development of high-resolution, lightweight, grazing-incidence x-ray optics to serve the needs of future x-ray astronomy missions such as Lynx. MSFC development efforts include both direct fabrication (diamond turning and deterministic computer-controlled polishing) of mirror shells and replication of mirror shells (from figured, polished mandrels). Both techniques produce full-circumference monolithic (primary + secondary) shells that share the advantages of inherent stability, ease of assembly, and low production cost. However, to achieve high-angular resolution, MSFC is exploring significant technology advances needed to control sources of figure error including fabrication- and coating-induced stresses and mounting-induced distortions.
Highlights
Lynx is a concept for a future NASA flagship observatory operating in the x-ray energy range
Marshall Space Flight Center (MSFC) has more than two decades of experience in the development of grazing incidence x-ray optics through electroformed replication.[2,3]
The Chandra mirrors prove that direct polishing of lightweight stiff materials, such as glass, can result in sub-arc sec, resolution large-diameter x-ray optics
Summary
Lynx is a concept for a future NASA flagship observatory operating in the x-ray energy range. Our high-resolution mirror development team envisions full-shell monolithic mirror elements fabricated from commonplace, lightweight, machinable metal, and metal alloy substrates. These materials combine low density and low coefficient of thermal expansion (CTE) with high-elastic modulus and high-yield strength. Together with monolithic full-shell construction, the MSFC design provides structural integrity throughout the fabrication process, system integration, launch, and operation over the mission lifetime. This contribution to this special section presents current efforts in the MSFC x-ray optics group to develop high-resolution grazing-incidence mirrors and related technologies. In addition to exploring technologies to fabricate precisely figured thin shells, the team at MSFC is pursuing capabilities to coat (Sec. 7) and to align and mount (Sec. 5) precisely formed mirrors including (static) postfabrication figure correction (Sec. 6) and associated metrology (Sec. 3.3)
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More From: Journal of Astronomical Telescopes, Instruments, and Systems
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