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This paper describes the guidance and navigation technique used by Hayabusa2 for the asteroid rendezvous operation to reach Ryugu. The operation results, including the achieved guidance and navigation performance, are also summarized. Multiple assessment and navigation teams worked closely to provide reliable navigation solutions with a short solution delivery cycle. Although the uncertainty of the Ryugu’s ephemeris was considerable before Hayabusa2’s arrival, a combination of radiometric-optical hybrid navigation and a stochastic-constrained optimum guidance method was able to achieve an accuracy of less than 100 m and 1 cm/s, and the arrival was precisely timed.


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Rendezvous to asteroid with highly uncertain ephemeris: Hayabusa2’s Ryugu-approach operation result

Show Author's information Yuichi Tsuda1( )Hiroshi Takeuchi1Naoko Ogawa1Go Ono2Shota Kikuchi1Yusuke Oki3Masateru Ishiguro4Daisuke Kuroda5Seitaro Urakawa6Shin-ichiro Okumura6
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan
Research and Development Directorate, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan
Research and Development Directorate, Japan Aerospace Exploration Agency, Tsukuba 305-8505, Japan
Seoul National University, Seoul 08826, Republic of Korea
Okayama Observatory, Kyoto University, Asakuchi 719-0232, Japan
Japan Spaceguard Association, Bisei 714-1411, Japan

Abstract

This paper describes the guidance and navigation technique used by Hayabusa2 for the asteroid rendezvous operation to reach Ryugu. The operation results, including the achieved guidance and navigation performance, are also summarized. Multiple assessment and navigation teams worked closely to provide reliable navigation solutions with a short solution delivery cycle. Although the uncertainty of the Ryugu’s ephemeris was considerable before Hayabusa2’s arrival, a combination of radiometric-optical hybrid navigation and a stochastic-constrained optimum guidance method was able to achieve an accuracy of less than 100 m and 1 cm/s, and the arrival was precisely timed.

Keywords: optical navigation, trajectory optimization, solar system exploration, sample return, spacecraft guidance

References(11)

[1]
Tsuda, Y., Yoshikawa, M., Abe, M., Minamino, H., Nakazawa, S. System design of the Hayabusa 2—Asteroid sample return mission to 1999 JU3. Acta Astronautica, 2013, 91: 356-362.
[2]
Tsuda, Y., Saiki, T., Terui, F., Nakazawa, S., Yoshikawa, M., Watanabe, S., Hayabusa2 Project Team. Hayabusa2 mission status: Landing, roving and cratering on asteroid Ryugu. Acta Astronautica, 2020, 171: 42-54.
[3]
Tsuda, Y., Takeuchi, H., Ogawa, N., Ono, G., Kikuchi, S., Oki, Y., Yamaguchi, T., Ishiguro, M., Kuroda, O., Utakawa, S., Okumura, S. Guidance and navigation result of Hayabusa2 asteroid rendezvous operation. In: Proceedings of the 32nd International Symposium on Space Technology and Science, 2019: 2019-d-074.
[4]
Tsuda, Y., Saiki, T., Ogawa, N., Morimoto, M. Trajectory Design for Japanese New Asteroid Sample Return Mission Hayabusa-2. In: Proceedings of the 23rd International Symposium on Space Flight Dynamics, 2012: IMD-1-1.
[5]
Kameda, S., Suzuki, H., Takamatsu, T., Cho, Y., Yasuda, T., Yamada, M., Sawada, H., Honda, R., Morota, T., Honda, C. et al. Preflight calibration test results for optical navigation camera telescope (ONC-T) onboard the Hayabusa2 spacecraft. Space Science Reviews, 2017, 208(1-4): 17-31.
[6]
Takeuchi, H., Yoshikawa, K., Takei, Y., Oki, Y., Kikuchi, S., Ikeda, H., Soldini, S., Ogawa, N., Mimasu, Y., Ono, G., et al. The deepspace multi-object orbit determination system and its application to Hayabusa2’s asteroid proximity operations. Astrodynamics, 2020, .
[7]
Nakatani, I., Kubota, T., Isaka, T. Navigation for small body rendezvous by visual active sensing. In: Proceedings of International Symposium on Space Dynamics, 1995: 853-858.
[8]
Van Dokkum, P. G. Cosmic-ray rejection by laplacian edge detection. Publications of the Astronomical Society of the Pacific, 2001, 113(789): 1420-1427.
[9]
Lang, D., Hogg, D. W., Mierle, K., Blanton, M., Roweis, S. Astrometry.net: blind astrometric calibration of arbitrary astronomical images. The Astronomical Journal, 2010, 139(5): 1782-1800.
[10]
Bertin, E., Arnouts, S. SExtractor: Software for source extraction. Astronomy and Astrophysics Supplement Series, 1996, 117(2): 393-404.
[11]
Watanabe, S., Hirabayashi, M., Hirata, N., Hirata, N., Noguchi, R., Shimaki, Y., Ikeda, H., Tatsumi, E., Yoshikawa, M., Kiknchi, S. et al. Hayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top-shaped rubble pile. Science, 2019, 364(6437): 268-272.
Publication history
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Acknowledgements

Publication history

Received: 24 January 2020
Accepted: 22 March 2020
Published: 18 June 2020
Issue date: June 2020

Copyright

© Tsinghua University Press 2020

Acknowledgements

The authors are grateful to the entire Hayabusa2 operation team for achieving this goal and supplying the operation product used in this analysis. JSPS KAKENHI Grant No. 18H01628 also supported this work.

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