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 />
7.4.9 Small Precision Optics<br />
Scope<br />
The key issues for masks are surface roughness, transmitted wavefront, and material<br />
homogeneity. We will fabricate and test substrates that meet the mask PSD requirements with<br />
emphasis on 15-100 micron spatial scales.<br />
For the cube beamsplitters, stress birefringence is identified as the primary limiting factor. Two<br />
approaches will be explored: redesign to eliminate cube beamsplitters and work with<br />
manufacturers to develop techniques and materials for ultralow-stress birefringence.<br />
For the remaining small optics, we will work with manufacturers to obtain 1 nm surface flatness<br />
on mounted optics. The small precision optics have achieved TRL 3.Their schedule is given in<br />
Table 7-10.<br />
Table 7-10. Small Precision Optics Schedule<br />
<strong>Plan</strong>ned<br />
Completion<br />
Date<br />
<strong>Plan</strong>ned Activities Performance Targets TRL<br />
Pre-Phase A<br />
Work with manufacturers to<br />
define specifications<br />
Set of specifications manufacturers are willing to<br />
attempt<br />
Phase A Build components Substrate meets mask PSD requirements,<br />
1 nm surface flatness for 10-20 cm reflective optics<br />
3<br />
4<br />
119