Share Email Print

Proceedings Paper

Edge sensor concept for segment stabilization
Author(s): Laura E. Coyle; J. Scott Knight; Michael Adkins
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

To meet ambitious science goals and leverage NASA investments for the James Webb Space Telescope, some proposed mission concepts include large aperture telescopes with segmented primary mirrors. Aberration control at the segment level becomes critical for these architectures because rigid body motion of the individual mirrors overtakes full aperture aberrations as the driver for wavefront stability. Perturbations at the segment level cannot be effectively sensed by existing full pupil low-order wavefront sensors because the errors are discontinuous and low-order techniques applied to individual segments would have insufficient photon flux. Thus, an additional “mid-order” control loop is required. We propose the use of capacitive edge sensors to locally sense the relative motion of segments in piston, tip and tilt, which then provide input to a compensation arm. Ball Aerospace has developed capacitive sensor technology with proven measurement precision of <12 pm RMS that can be adapted for measuring primary mirror segment motion. This performance approaches the 10 pm stability often stated as a requirement for direct imaging of earth-like exoplanets with a coronagraph. Using the geometry of the existing hardware as a baseline, the sensor gap and plate area can be scaled to accommodate mounting to mirror segments while maintaining or increasing sensitivity and multiple plates in different orientations can be used to sense individual degrees of freedom. This paper will present measured results from the Ball capacitive sensor and use those results to develop expected sensitives and a notional sensor head geometry for stabilizing a large, segmented primary mirror with edge sensors.

Paper Details

Date Published: 12 July 2018
PDF: 9 pages
Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 1069869 (12 July 2018); doi: 10.1117/12.2312224
Show Author Affiliations
Laura E. Coyle, Ball Aerospace (United States)
J. Scott Knight, Ball Aerospace (United States)
Michael Adkins, Ball Aerospace (United States)

Published in SPIE Proceedings Vol. 10698:
Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
Makenzie Lystrup; Howard A. MacEwen; Giovanni G. Fazio; Natalie Batalha; Nicholas Siegler; Edward C. Tong, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?