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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Structural, Thermal, and Spacecraft <strong>Technology</strong><br />
Figure 4-13. Schematic of the Pointing Control Testbed.<br />
Critical Testbed Components<br />
(1) RWA disturbances on the S/C. The reaction wheels assembly (RWA) will induce vibrations<br />
on the S/C. There is a separate structures testbed that will perform detailed evaluation of the<br />
induced vibration and allow the creation of a vibration model. This model will then be used to<br />
simulate the disturbances at the isolation interface. Additional disturbance models will include<br />
the unloading of RWA.<br />
(2) A model of the disturbances of the S/C transmitted to the telescope as a function of the<br />
disturbance into the isolator. The testbed will require an isolator or isolator simulator with the<br />
characteristics of the flight system (or an appropriate model of the performance) and a computer<br />
controllable vibration inducing system, which can induce disturbance onto the testbed.<br />
(3) A number of additional sources of disturbance are present on the telescope. These include<br />
those caused by cryopumps, steering mirror actuation, secondary mirror actuation, and science<br />
shutter actuations and disturbances transmitted through the cabling between the spacecraft and<br />
payload.<br />
(4) The acquisition camera will be part of the testbed. The acquisition camera is required to have<br />
highly accurate measurements over up to a 60 arcsec FOV to provide for handoff and pointing to<br />
the coronagraph. The acquisition camera design is not yet made final, but a simulated<br />
acquisition camera will be included in the testbed.<br />
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