1 December 1984 Space Telescope Low-Scattered-Light Camera: A Model
Author Affiliations +
Abstract
A design approach for a camera to be used with the Space Telescope is given. Camera optics relay the system pupil onto an annular Gaussian ring apodizing mask to control diffracted light. Image plane intensity distributions for both one- and two-dimensional models of ripple on the primary mirror were calculated. Calculations using ripple amplitudes between X/20 and X/200 with spatial correlations of the ripple across the primary mirror between 0.2 and 2.0 cm indicate that the detection of an object 109 times fainter than a bright source in the field is possible. We thus conclude that detection of a Jovian-type planet in orbit about a Centauri with a camera on the Space Telescope may be possible.
J. B. Breckinridge, J. B. Breckinridge, T. G. Kuper, T. G. Kuper, R. V. Shack, R. V. Shack, } "Space Telescope Low-Scattered-Light Camera: A Model," Optical Engineering 23(6), 236816 (1 December 1984). https://doi.org/10.1117/12.7973388 . Submission:
JOURNAL ARTICLE
5 PAGES


SHARE
RELATED CONTENT

A fiber injection unit for the Keck Planet Imager and...
Proceedings of SPIE (August 31 2017)
Design Features Of The Space Telescope
Proceedings of SPIE (September 13 1977)
Discovery Channel Telescope: progress and status
Proceedings of SPIE (June 26 2006)

Back to Top