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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 />

129

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