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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Chapter 7<br />
7.4 Optics and Starlight Suppression Testbeds<br />
7.4.1 Phase A and B <strong>Plan</strong>s for HCIT and PDS<br />
Scope<br />
All the pre-Phase A milestones will probably be met using the half-dark hole configuration.<br />
Full-dark hole performance requires two deformable mirrors to control both phase and<br />
amplitude. Trade studies to determine the optimum architecture (Michelson configuration or two<br />
DMs in series) and necessary control algorithms are underway as part of the Wavefront Sensing<br />
and Control task. Design and fabrication of opto-mechanical hardware is planned for FY06, with<br />
installation in the HCIT and experimentation commencing at the beginning of Phase A.<br />
Completion of this activity had been planned for pre-Phase A, but it resulted in an unreasonable<br />
schedule that put required milestone performance at risk. If modeling shows that two DMs are<br />
needed to get the broadband performance required in Milestone 2, the HCIT schedule and<br />
resources will be adjusted. Also in Phase A, a custom bench and mounts will be designed and<br />
fabricated for the HCIT, with completion at the end of Phase A. This will provide the thermal<br />
stability needed to achieve and maintain 1 × 10 -10 contrast, as well as enabling full structural and<br />
thermal modeling of the testbed. Initial study work for the <strong>Plan</strong>et Detection Simulator will<br />
commence near the end of pre-Phase A, with detailed design and fabrication of the hardware<br />
during Phase A and installation in the HCIT occurring at the beginning of Phase B, after the<br />
custom testbed bench has been integrated. During Phases A and B, the spectral bandwidth will<br />
be increased and the center wavelength shifted to lower wavelengths, with the performance<br />
target for Phase B matching the required <strong>TPF</strong>-C planet detection bandpass (currently 500-600<br />
nm). The HCIT and PDS milestone schedule is given in Table 7-2.<br />
State of the Art TRL 4<br />
Laboratory results from the HCIT have shown an average contrast of 0.9 × 10 -9 for laser light as<br />
measured in the half-dark hole over angles from 4 to 10 λ/D.<br />
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