Autonomous optical navigation for DESTINY+: Enhancing misalignment robustness in flyby observations with a rotating telescope

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Hauptverfasser: Hosonuma, Takayuki, Miyabara, Takeshi, Ozaki, Naoya, Ishibashi, Ko, Suzaki, Yuta, Hong, Peng, Ohta, Masayuki, Takashima, Takeshi
Format: Preprint
Veröffentlicht: 2025
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author Hosonuma, Takayuki
Miyabara, Takeshi
Ozaki, Naoya
Ishibashi, Ko
Suzaki, Yuta
Hong, Peng
Ohta, Masayuki
Takashima, Takeshi
author_facet Hosonuma, Takayuki
Miyabara, Takeshi
Ozaki, Naoya
Ishibashi, Ko
Suzaki, Yuta
Hong, Peng
Ohta, Masayuki
Takashima, Takeshi
contents DESTINY+ is an upcoming JAXA Epsilon medium-class mission to flyby multiple asteroids including Phaethon. As an asteroid flyby observation instrument, a telescope mechanically capable of single-axis rotation, named TCAP, is mounted on the spacecraft to track and observe the target asteroids during flyby. As in past flyby missions utilizing rotating telescopes, TCAP is also used as a navigation camera for autonomous optical navigation during the closest-approach phase. To mitigate the degradation of the navigation accuracy, past missions performed calibration of the navigation camera's alignment before starting optical navigation. However, such calibration requires significant operational time to complete and imposes constraints on the operation sequence. From the above background, the DESTINY+ team has studied the possibility of reducing operational costs by allowing TCAP alignment errors to remain. This paper describes an autonomous optical navigation algorithm robust to the misalignment of rotating telescopes, proposed in this context. In the proposed method, the misalignment of the telescope is estimated simultaneously with the spacecraft's orbit relative to the flyby target. To deal with the nonlinearity between the misalignment and the observation value, the proposed method utilizes the unscented Kalman filter, instead of the extended Kalman filter widely used in past studies. The proposed method was evaluated with numerical simulations on a PC and with hardware-in-the-loop simulation, taking the Phaethon flyby in the DESTINY+ mission as an example. The validation results suggest that the proposed method can mitigate the misalignment-induced degradation of the optical navigation accuracy with reasonable computational costs suited for onboard computers.
format Preprint
id arxiv_https___arxiv_org_abs_2504_01835
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Autonomous optical navigation for DESTINY+: Enhancing misalignment robustness in flyby observations with a rotating telescope
Hosonuma, Takayuki
Miyabara, Takeshi
Ozaki, Naoya
Ishibashi, Ko
Suzaki, Yuta
Hong, Peng
Ohta, Masayuki
Takashima, Takeshi
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Machine Learning
DESTINY+ is an upcoming JAXA Epsilon medium-class mission to flyby multiple asteroids including Phaethon. As an asteroid flyby observation instrument, a telescope mechanically capable of single-axis rotation, named TCAP, is mounted on the spacecraft to track and observe the target asteroids during flyby. As in past flyby missions utilizing rotating telescopes, TCAP is also used as a navigation camera for autonomous optical navigation during the closest-approach phase. To mitigate the degradation of the navigation accuracy, past missions performed calibration of the navigation camera's alignment before starting optical navigation. However, such calibration requires significant operational time to complete and imposes constraints on the operation sequence. From the above background, the DESTINY+ team has studied the possibility of reducing operational costs by allowing TCAP alignment errors to remain. This paper describes an autonomous optical navigation algorithm robust to the misalignment of rotating telescopes, proposed in this context. In the proposed method, the misalignment of the telescope is estimated simultaneously with the spacecraft's orbit relative to the flyby target. To deal with the nonlinearity between the misalignment and the observation value, the proposed method utilizes the unscented Kalman filter, instead of the extended Kalman filter widely used in past studies. The proposed method was evaluated with numerical simulations on a PC and with hardware-in-the-loop simulation, taking the Phaethon flyby in the DESTINY+ mission as an example. The validation results suggest that the proposed method can mitigate the misalignment-induced degradation of the optical navigation accuracy with reasonable computational costs suited for onboard computers.
title Autonomous optical navigation for DESTINY+: Enhancing misalignment robustness in flyby observations with a rotating telescope
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Machine Learning
url https://arxiv.org/abs/2504.01835