Paper
15 April 1993 Very high pointing accuracy star-tracker optics trade-off analysis
M. Magnani
Author Affiliations +
Abstract
The Far-Infrared and Sub-millimeter Space Telescope (FIRST) Astronomy Mission, is a cornerstone of the ESA science program for space observations in the 0.1 to 1 mm wavelength band. A very high accuracy star tracker has to be developed for the pointing and stabilization functions of the FIRST spacecraft. This paper deals with the optics trade-off analysis of this new star tracker VHPA, acronym derived from `very high pointing accuracy.' The optics trade-off consists of a comparative analysis of the following configurations: dioptric, catadioptric, Schmidt and Ritchey-Chretien telescopes. The results are shown and the polychromatic tests of image quality are reported, including centroid error function. A table of merit is provided in order to select the configuration proposed as baseline.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. Magnani "Very high pointing accuracy star-tracker optics trade-off analysis", Proc. SPIE 1780, Lens and Optical Systems Design, 17801Z (15 April 1993); https://doi.org/10.1117/12.142870
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Mirrors

Stars

Charge-coupled devices

Combined lens-mirror systems

Glasses

Image quality

RELATED CONTENT

Space-based CCD experiment for high-precision astrometry
Proceedings of SPIE (November 01 1993)
OSIRIS optics
Proceedings of SPIE (March 07 2003)
Telescope Structures: An Evolutionary Overview
Proceedings of SPIE (June 03 1987)
Optical design for DIVA
Proceedings of SPIE (August 28 1998)
HyperSuprime: imaging optics
Proceedings of SPIE (June 29 2006)

Back to Top