Abstract
This paper presents a tool for the numerical propagation of high-fidelity astrodynamics, called PHiFA. The coupled orbit-attitude dynamics for space objects are modeled by considering various types of perturbative forces and torques. Two methods have been implemented to calculate the surface forces: the area matrix method and the beam method. The beam method is more precise as it discretizes the source media (e.g., sunlight and aerodynamic wind) and the surface of the target into multiple rays and finite elements, respectively, and then accumulates the effect of each hit. The PHiFA tool was tested and validated using a 3U CubeSat model and the defunct European environment satellite (Envisat) model.
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Acknowledgements
We would like to acknowledge the support from the Guangdong Basic and Applied Basic Research Foundation Project (No. 2020A1515110216) and the support of the Cooperative Research Center for Space Environment Management (SERC Limited) through the Australian Government’s Cooperative Research Center Program when the work was initialized. We would also like to appreciate Dr. Daniel Kucharski from The University of Texas at Austin for sharing the fitted spin period values of Envisat based on satellite laser ranging measurements.
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Yang Yang was previously an assistant professor at the School of Aeronautics and Astronautics, Sun Yat-sen University, Shenzhen, China, during 2020–2021. He used to work as a postdoctoral research fellow at SPACE Research Centre, RMIT University, Melbourne, Australia, during 2015–2019. His doctoral degree was with the School of Astronautics, Northwestern Polytechnical University, Xi’an, China, during 2010–2015. His current research interests include astrodynamics, data association, orbit determination & prediction, nonlinear and non-Gaussian estimation/filtering, space situational awareness, and GNSS based positioning & applications.
Erik Klein is currently a Ph.D. student at the Institute of Space Systems, German Aerospace Center (DLR) Bremen, Germany. He used to work as a master student at the Institute for Space Systems, TU Braunschweig, Braunschweig, Germany, and visited SPACE Research Centre, RMIT University, Melbourne, Australia, from Oct. 2018 to Apr. 2019. His master thesis “Influence of laser-matter interaction on resident space objects” was supported by both universities.
Changyong He received his B.S. degree in geomagnetics and M.S. degree in GPS navigation and positioning from Wuhan University, Wuhan, China, in 2011 and 2013, respectively, and his Ph.D. degree from RMIT University, Melbourne, Australia, in 2019. He is currently working at IGN/ENSG in France. His research interest includes the modeling of the thermospheric mass density, precise orbit determination, GPS meteorology, space geodesy, and the terrestial coordinate framework.
Han Cai received his Ph.D. degree in geospatial science from RMIT University, Melbourne, Australia, in 2019, and was a postdoctoral research fellow at the Oden Institute for Computational Engineering and Sciences, The University of Texas at Austin, from 2019 to 2021. In 2021, he joined Beijing Institute of Technology as an assistant professor. His areas of expertise are in orbit determination, multi-target tracking, sensor tasking, information fusion, and uncertainty quantification.
Yan Zhang is currently a full professor at the School of Aeronautics and Astronautics, Sun Yat-sen University, Shenzhen, China. She received her doctoral degree of aerospace science and technology from National University of Defense Technology, Changsha, China, in 2005. She has published more than 40 journal/conference papers and 4 monographs. Her main research interests include photoelectric devices design and information fusion techniques.
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Yang, Y., Klein, E., He, C. et al. PHiFA—A tool for numerical propagation of high-fidelity astrodynamics. Astrodyn 6, 189–204 (2022). https://doi.org/10.1007/s42064-021-0113-1
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DOI: https://doi.org/10.1007/s42064-021-0113-1