Takayuki Hosonuma , Takeshi Miyabara , Naoya Ozaki , Ko Ishibashi , Yuta Suzaki , Peng Hong , Masayuki Ohta , Takeshi Takashima
{"title":"DESTINY+的自主光学导航:利用旋转望远镜增强飞掠观测中的失调鲁棒性","authors":"Takayuki Hosonuma , Takeshi Miyabara , Naoya Ozaki , Ko Ishibashi , Yuta Suzaki , Peng Hong , Masayuki Ohta , Takeshi Takashima","doi":"10.1016/j.actaastro.2025.04.023","DOIUrl":null,"url":null,"abstract":"<div><div><span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> 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 capturing large number of images by the navigation camera and downlinking them to the ground station. In the case of small spacecraft with limited link capacity, such as <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span>, such ground-in-the-loop calibration requires significant operational time to complete and imposes constraints on the operation sequence. From the above background, the <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> 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 <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> mission as an example. In the example case, the misalignment-induced navigation accuracy degradation of 4.6<!--> <!-->km-<span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> can be reduced to 0.1<!--> <!-->km-<span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> by the proposed method. The required time to run one-cycle of the navigation process on the onboard computer for the <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> mission is less than 0.18<!--> <!-->s. These results validate that the proposed method can mitigate the misalignment-induced degradation of the optical navigation accuracy with reasonable computational costs suited for onboard computers.</div></div>","PeriodicalId":44971,"journal":{"name":"Acta Astronautica","volume":"234 ","pages":"Pages 117-130"},"PeriodicalIF":3.1000,"publicationDate":"2025-04-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Autonomous optical navigation for DESTINY+: Enhancing misalignment robustness in flyby observations with a rotating telescope\",\"authors\":\"Takayuki Hosonuma , Takeshi Miyabara , Naoya Ozaki , Ko Ishibashi , Yuta Suzaki , Peng Hong , Masayuki Ohta , Takeshi Takashima\",\"doi\":\"10.1016/j.actaastro.2025.04.023\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div><span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> 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 capturing large number of images by the navigation camera and downlinking them to the ground station. In the case of small spacecraft with limited link capacity, such as <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span>, such ground-in-the-loop calibration requires significant operational time to complete and imposes constraints on the operation sequence. From the above background, the <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> 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 <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> mission as an example. In the example case, the misalignment-induced navigation accuracy degradation of 4.6<!--> <!-->km-<span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> can be reduced to 0.1<!--> <!-->km-<span><math><mrow><mn>1</mn><mi>σ</mi></mrow></math></span> by the proposed method. The required time to run one-cycle of the navigation process on the onboard computer for the <span><math><msup><mrow><mtext>DESTINY</mtext></mrow><mrow><mtext>+</mtext></mrow></msup></math></span> mission is less than 0.18<!--> <!-->s. These results validate that the proposed method can mitigate the misalignment-induced degradation of the optical navigation accuracy with reasonable computational costs suited for onboard computers.</div></div>\",\"PeriodicalId\":44971,\"journal\":{\"name\":\"Acta Astronautica\",\"volume\":\"234 \",\"pages\":\"Pages 117-130\"},\"PeriodicalIF\":3.1000,\"publicationDate\":\"2025-04-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Acta Astronautica\",\"FirstCategoryId\":\"5\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0094576525002231\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ENGINEERING, AEROSPACE\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Acta Astronautica","FirstCategoryId":"5","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0094576525002231","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ENGINEERING, AEROSPACE","Score":null,"Total":0}
Autonomous optical navigation for DESTINY+: Enhancing misalignment robustness in flyby observations with a rotating telescope
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 capturing large number of images by the navigation camera and downlinking them to the ground station. In the case of small spacecraft with limited link capacity, such as , such ground-in-the-loop calibration requires significant operational time to complete and imposes constraints on the operation sequence. From the above background, the 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 mission as an example. In the example case, the misalignment-induced navigation accuracy degradation of 4.6 km- can be reduced to 0.1 km- by the proposed method. The required time to run one-cycle of the navigation process on the onboard computer for the mission is less than 0.18 s. These results validate that the proposed method can mitigate the misalignment-induced degradation of the optical navigation accuracy with reasonable computational costs suited for onboard computers.
期刊介绍:
Acta Astronautica is sponsored by the International Academy of Astronautics. Content is based on original contributions in all fields of basic, engineering, life and social space sciences and of space technology related to:
The peaceful scientific exploration of space,
Its exploitation for human welfare and progress,
Conception, design, development and operation of space-borne and Earth-based systems,
In addition to regular issues, the journal publishes selected proceedings of the annual International Astronautical Congress (IAC), transactions of the IAA and special issues on topics of current interest, such as microgravity, space station technology, geostationary orbits, and space economics. Other subject areas include satellite technology, space transportation and communications, space energy, power and propulsion, astrodynamics, extraterrestrial intelligence and Earth observations.