Paper
23 September 1993 Stellar attitude determination accuracy with multiple-star-tracking advanced star tracker
Rene Abreu
Author Affiliations +
Abstract
Inertially referenced attitude determination for pointing and control is a well established need which demands continual optimization. Star trackers can accomplish the task by direct stellar measurements. This paper presents the results of design trades for Hughes Danbury Optical System's (HDOS) Advanced Star Tracker (ASTRA) products with the built in capability to output inertial attitude, typically in the form of a quaternion in an earth centered inertial (ECI) coordinate system. This is an enhanced capability from standard tracker products which only output star image centroid positions. Attitude accuracy predictions for a variety of trades have been evaluated using an orbital flight simulator. This simulator integrates star tracker performance modeling with algorithms for attitude determination. Trades include field of view (FOV) size, sensitivity, number of stars tracked and star catalog size.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rene Abreu "Stellar attitude determination accuracy with multiple-star-tracking advanced star tracker", Proc. SPIE 1949, Space Guidance, Control, and Tracking, (23 September 1993); https://doi.org/10.1117/12.157084
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Cited by 5 scholarly publications.
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KEYWORDS
Stars

Charge-coupled devices

Signal to noise ratio

Error analysis

Interference (communication)

Optical tracking

Monte Carlo methods

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