Please use this identifier to cite or link to this item: https://hdl.handle.net/10356/86013
Title: A robust star identification algorithm with star shortlisting
Authors: Mehta, Deval Samirbhai
Chen, Shoushun
Low, Kay Soon
Keywords: Lost-in-space Mode
Star Pattern Recognition
DRNTU::Science::Astronomy
Issue Date: 2018
Source: Mehta, D. S., Chen, S., & Low, K. S. (2018). A robust star identification algorithm with star shortlisting. Advances in Space Research, 61(10), 2647-2660. doi:10.1016/j.asr.2018.02.029.
Journal: Advances in Space Research
Abstract: A star tracker provides the most accurate attitude solution in terms of arc seconds compared to the other existing attitude sensors. When no prior attitude information is available, it operates in “Lost-In-Space (LIS)” mode. Star pattern recognition, also known as star identification algorithm, forms the most crucial part of a star tracker in the LIS mode. Recognition reliability and speed are the two most important parameters of a star pattern recognition technique. In this paper, a novel star identification algorithm with star ID shortlisting is proposed. Firstly, the star IDs are shortlisted based on worst-case patch mismatch, and later stars are identified in the image by an initial match confirmed with a running sequential angular match technique. The proposed idea is tested on 16,200 simulated star images having magnitude uncertainty, noise stars, positional deviation, and varying size of the field of view. The proposed idea is also benchmarked with the state-of-the-art star pattern recognition techniques. Finally, the real-time performance of the proposed technique is tested on the 3104 real star images captured by a star tracker SST-20S currently mounted on a satellite. The proposed technique can achieve an identification accuracy of 98% and takes only 8.2 ms for identification on real images. Simulation and real-time results depict that the proposed technique is highly robust and achieves a high speed of identification suitable for actual space applications.
URI: https://hdl.handle.net/10356/86013
http://hdl.handle.net/10220/48329
ISSN: 0273-1177
DOI: 10.1016/j.asr.2018.02.029
Schools: School of Electrical and Electronic Engineering 
Organisations: Satellite Research Center
Rights: © 2018 COSPAR. All rights reserved. This paper was published by Elsevier in Advances in Space Research and is made available with permission of COSPAR.
Fulltext Permission: open
Fulltext Availability: With Fulltext
Appears in Collections:EEE Journal Articles

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