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APPARILLO: a fully operational and autonomous staring system for LEO debris detection

For safe operation of active space crafts, the space debris population needs to be continuously scanned, to avoid collisions of active satellites with space debris. Especially the low Earth orbit (LEO) shows higher risks of collisions due to the highest density of orbital debris. Laser ranging stati...

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Detalles Bibliográficos
Autores principales: Wagner, Paul, Clausen, Tim
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Vienna 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8256648/
https://www.ncbi.nlm.nih.gov/pubmed/34777620
http://dx.doi.org/10.1007/s12567-021-00380-6
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author Wagner, Paul
Clausen, Tim
author_facet Wagner, Paul
Clausen, Tim
author_sort Wagner, Paul
collection PubMed
description For safe operation of active space crafts, the space debris population needs to be continuously scanned, to avoid collisions of active satellites with space debris. Especially the low Earth orbit (LEO) shows higher risks of collisions due to the highest density of orbital debris. Laser ranging stations can deliver highly accurate distance measurements of debris objects allowing precise orbit determination and more effective collision avoidance. However, a laser ranging station needs accurate a priori orbit information to track an orbital object. To detect and track unknown orbital objects in LEO, here, a passive optical staring system is developed for autonomous 24/7 operation. The system is weather-sealed and does not require any service to perform observations. To detect objects, a wide-angle imaging system with 10° field of view equipped with an astronomical CCD camera was designed and set up to continuously observe the sky for LEO objects. The system can monitor and process several passing objects simultaneously without limitations. It automatically starts an observation, processes the images and saves the 2D angular measurements of each object as equatorial coordinates in the TDM standard. This allows subsequent initial orbit determination and handover to a laser tracking system. During campaigns at twilight the system detected up to 36 objects per hour, with high detection efficiencies of LEO objects larger than 1 m(3). It is shown that objects as small as 0.1 m(3) can be detected and that the estimated precision of the measurements is about 0.05° or 7 × the pixel scale.
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spelling pubmed-82566482021-07-06 APPARILLO: a fully operational and autonomous staring system for LEO debris detection Wagner, Paul Clausen, Tim CEAS Space J Original Paper For safe operation of active space crafts, the space debris population needs to be continuously scanned, to avoid collisions of active satellites with space debris. Especially the low Earth orbit (LEO) shows higher risks of collisions due to the highest density of orbital debris. Laser ranging stations can deliver highly accurate distance measurements of debris objects allowing precise orbit determination and more effective collision avoidance. However, a laser ranging station needs accurate a priori orbit information to track an orbital object. To detect and track unknown orbital objects in LEO, here, a passive optical staring system is developed for autonomous 24/7 operation. The system is weather-sealed and does not require any service to perform observations. To detect objects, a wide-angle imaging system with 10° field of view equipped with an astronomical CCD camera was designed and set up to continuously observe the sky for LEO objects. The system can monitor and process several passing objects simultaneously without limitations. It automatically starts an observation, processes the images and saves the 2D angular measurements of each object as equatorial coordinates in the TDM standard. This allows subsequent initial orbit determination and handover to a laser tracking system. During campaigns at twilight the system detected up to 36 objects per hour, with high detection efficiencies of LEO objects larger than 1 m(3). It is shown that objects as small as 0.1 m(3) can be detected and that the estimated precision of the measurements is about 0.05° or 7 × the pixel scale. Springer Vienna 2021-07-05 2022 /pmc/articles/PMC8256648/ /pubmed/34777620 http://dx.doi.org/10.1007/s12567-021-00380-6 Text en © The Author(s) 2021 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) .
spellingShingle Original Paper
Wagner, Paul
Clausen, Tim
APPARILLO: a fully operational and autonomous staring system for LEO debris detection
title APPARILLO: a fully operational and autonomous staring system for LEO debris detection
title_full APPARILLO: a fully operational and autonomous staring system for LEO debris detection
title_fullStr APPARILLO: a fully operational and autonomous staring system for LEO debris detection
title_full_unstemmed APPARILLO: a fully operational and autonomous staring system for LEO debris detection
title_short APPARILLO: a fully operational and autonomous staring system for LEO debris detection
title_sort apparillo: a fully operational and autonomous staring system for leo debris detection
topic Original Paper
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8256648/
https://www.ncbi.nlm.nih.gov/pubmed/34777620
http://dx.doi.org/10.1007/s12567-021-00380-6
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