This paper is an overview of the Next Generation X-ray Optics effort at NASA’s Goddard Space Flight Center. The objective of the NGXO team is to develop and mature an X-ray mirror technology that is capable of building a mirror assembly for flagship missions like Lynx and Probe missions like AXIS, LEM, and HEX-P, as well as Explorer missions like STAR-X. These missions require X-ray mirror assemblies that have comparable or better angular resolution than Chandra’s 0.5 arc-seconds, but have ten to twenty times more effective area under similar mass constraints. The NGXO team combines the stress-free nature of single crystal silicon with advanced polishing techniques to make mirror segments that are of higher figure quality than the Chandra mirror shells, but are at least ten times thinner and therefore lighter. The NGXO work encompasses all elements that make a complete process to design, build, test, and deliver a complete mirror assembly, including optical design, mirror segment fabrication, coating, alignment and bonding to make mirror modules, integration of mirror modules into meta-shells, and integration of meta-shells into a mirror assembly. In addition, the NGXO team also adopts the latest mass-production techniques to ensure that building such a mirror assembly can also meet programmatic, such as schedule and cost, requirements of future missions.
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