TPF-C Technology Plan - Exoplanet Exploration Program - NASA
TPF-C Technology Plan - Exoplanet Exploration Program - NASA
TPF-C Technology Plan - Exoplanet Exploration Program - NASA
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<strong>Plan</strong> for <strong>Technology</strong> Development<br />
7.5.9 Sub-scale EM Primary Mirror Assembly<br />
Scope<br />
This testbed is essentially the same testbed as described in the preceding section but with added<br />
features. In the initial build-up of the testbed, vibration isolation will be included for convenience<br />
and efficiency, but is not required for the thermal control system evaluation. The interferometer<br />
and its attendant controls can be added after the tests on the sunshield/thermal enclosure systems<br />
have been completed. Optical testing of the thermal control system will occur during Phase B.<br />
The sub-scale EM primary mirror assembly has achieved TRL 3. The assembly schedule is given<br />
in Table 7-19.<br />
Table 7-19. Sub-scale EM Primary Mirror Assembly Schedule<br />
<strong>Plan</strong>ned<br />
Completion<br />
Date<br />
<strong>Plan</strong>ned Activities Performance Targets TRL<br />
Phase B<br />
Convert the<br />
Sunshield/Isothermal<br />
Cavity testbed into the Subscale<br />
PM Assembly testbed,<br />
and test the sub-scale PM in<br />
the new testbed.<br />
Design and procure the high-quality sub-scale mirror<br />
needed for the optical testing of the<br />
Sunshield/Isothermal Cavity testbed. This will likely<br />
need to be started sometime late in Phase A.<br />
In the presence of external thermal disturbances<br />
simulating the effects of dithers and slews, demonstrate<br />
optical shape control at the required flight levels.<br />
5-6<br />
(sys)<br />
Correlate analytical models to the test data to validate<br />
models that can later be scaled to predict the optical<br />
response of the full-scale <strong>TPF</strong>-C to dithers and slews.<br />
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