Wavefront Control for a Segmented Deployable Space Telescope
By segmenting and folding the primary mirror, quite large telescopes can be packed into the nose cone of a rocket.
Engineering topics
Publications and source records attributed to Davila, P..
By segmenting and folding the primary mirror, quite large telescopes can be packed into the nose cone of a rocket.
Control algorithms developed for coarse phasing the segmented mirrors of the Next Generation Space Telescope (NGST)are being tested in realistic modeling and on the NGST wavefront control testbed, also known as DCATT.
A telescope simulator was built as part of the Nexus wavefront control testbed, an NGST technology experiment at NASA's Goddard Space Flight Center.
An Integrated Product Team (IPT) was formed to develop a detailed concept for optical test methodology for testing of the NGST individual primary, secondary and tertiary mirrors and the full telescope system on the ground. Optical testing is a significant cost driver therefore the testing has to understood in detailed fashion early. A brief summary of the preliminary metrology test plan at the mirror component and telescope system level is presented.
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