Stellar Positioning System Part I: Applying Ancient Theory to a Modern World
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abstract
Two different theoretical approaches to the position determination problem are presented, one matrix-based and the other vector-based. Both approaches are designed for implementation in an autonomous Stellar Positioning System (SPS) that uses the following measurement sources: an astronomical camera, a clock, and a set of two inclinometers. Before presenting each of the algorithms, the reference frames utilized are defined. The two position estimation techniques are then individually presented, followed by a discussion of real-world gravity and geometry model refinements. Copyright 2008 by the American Institute of Aeronautics and Astronautics, Inc.
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AIAA/AAS Astrodynamics Specialist Conference and Exhibit