A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure Models
China is planning to launch the “Tianwen-4” mission around the year 2030, with its aim being the exploration of Jupiter and its moon, Callisto. Within the realm of deep space exploration, the accuracy of ephemerides is of great importance. Current ephemerides employ a simplified rotation model for C...
| Published in: | The Astrophysical Journal |
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| Main Authors: | , , , , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adfe65 |
| _version_ | 1848758857877159936 |
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| author | Kai Huang Yongzhang Yang Yuhao Chen Yining Zhang Yuqiang Li |
| author_facet | Kai Huang Yongzhang Yang Yuhao Chen Yining Zhang Yuqiang Li |
| author_sort | Kai Huang |
| collection | DOAJ |
| container_title | The Astrophysical Journal |
| description | China is planning to launch the “Tianwen-4” mission around the year 2030, with its aim being the exploration of Jupiter and its moon, Callisto. Within the realm of deep space exploration, the accuracy of ephemerides is of great importance. Current ephemerides employ a simplified rotation model for Callisto, which this study addresses by proposing a novel dynamical model. This model enhances the existing orbital dynamics by integrating Callisto’s rotational motions influenced by gravitational torques from the Sun, Jupiter, and other Galilean moons within an inertial frame, capturing the intricate coupling between Callisto’s orbital and rotational dynamics. The study establishes a full dynamical model by deriving analytical expressions for this coupling and developing an adjustment model for data fitting using precise orbit determination methods. Furthermore, the influence of tidal effects on Callisto’s motion is investigated, considering its multilayered internal structure. Results demonstrate that the difference between the newly established full model and the model in current ephemerides is on the order of tens of meters. When calculating the impact of different internal structures of Callisto on its orbit, the influence of three-layered and two-layered structures is on the order of meters, suggesting that the development of a high-precision dynamical model requires additional constraints on the internal structure of Callisto. This research provides a novel alternative for a new generation of precise numerical ephemerides for Callisto. Additionally, these findings provide a testing platform for the data from the “Tianwen-4” mission. |
| format | Article |
| id | doaj-art-103412bc536e4fdd989cffa8a7cf5e4a |
| institution | Directory of Open Access Journals |
| issn | 1538-4357 |
| language | English |
| publishDate | 2025-01-01 |
| publisher | IOP Publishing |
| record_format | Article |
| spelling | doaj-art-103412bc536e4fdd989cffa8a7cf5e4a2025-10-14T04:23:54ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01992218610.3847/1538-4357/adfe65A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure ModelsKai Huang0https://orcid.org/0009-0001-4162-2792Yongzhang Yang1https://orcid.org/0000-0001-9202-7750Yuhao Chen2https://orcid.org/0000-0002-8077-094XYining Zhang3https://orcid.org/0000-0001-5933-5794Yuqiang Li4https://orcid.org/0000-0003-1022-8423Yunnan Observatories, Chinese Academy of Sciences , Kunming 650216, People’s Republic of China ; yang.yongzhang@ynao.ac.cn, lyq@ynao.ac.cn; University of Chinese Academy of Science , Beijing 100049, People’s Republic of ChinaYunnan Observatories, Chinese Academy of Sciences , Kunming 650216, People’s Republic of China ; yang.yongzhang@ynao.ac.cn, lyq@ynao.ac.cnYunnan Observatories, Chinese Academy of Sciences , Kunming 650216, People’s Republic of China ; yang.yongzhang@ynao.ac.cn, lyq@ynao.ac.cn; University of Chinese Academy of Science , Beijing 100049, People’s Republic of ChinaUniversity of Chinese Academy of Science , Beijing 100049, People’s Republic of China; National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of ChinaYunnan Observatories, Chinese Academy of Sciences , Kunming 650216, People’s Republic of China ; yang.yongzhang@ynao.ac.cn, lyq@ynao.ac.cn; Key Laboratory of Space Object and Debris Observation , PMO, CAS, Nanjing 210023, People’s Republic of ChinaChina is planning to launch the “Tianwen-4” mission around the year 2030, with its aim being the exploration of Jupiter and its moon, Callisto. Within the realm of deep space exploration, the accuracy of ephemerides is of great importance. Current ephemerides employ a simplified rotation model for Callisto, which this study addresses by proposing a novel dynamical model. This model enhances the existing orbital dynamics by integrating Callisto’s rotational motions influenced by gravitational torques from the Sun, Jupiter, and other Galilean moons within an inertial frame, capturing the intricate coupling between Callisto’s orbital and rotational dynamics. The study establishes a full dynamical model by deriving analytical expressions for this coupling and developing an adjustment model for data fitting using precise orbit determination methods. Furthermore, the influence of tidal effects on Callisto’s motion is investigated, considering its multilayered internal structure. Results demonstrate that the difference between the newly established full model and the model in current ephemerides is on the order of tens of meters. When calculating the impact of different internal structures of Callisto on its orbit, the influence of three-layered and two-layered structures is on the order of meters, suggesting that the development of a high-precision dynamical model requires additional constraints on the internal structure of Callisto. This research provides a novel alternative for a new generation of precise numerical ephemerides for Callisto. Additionally, these findings provide a testing platform for the data from the “Tianwen-4” mission.https://doi.org/10.3847/1538-4357/adfe65Celestial mechanicsAstrometryEphemeridesNatural satellite dynamicsJovian satellitesGalilean satellites |
| spellingShingle | Kai Huang Yongzhang Yang Yuhao Chen Yining Zhang Yuqiang Li A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure Models Celestial mechanics Astrometry Ephemerides Natural satellite dynamics Jovian satellites Galilean satellites |
| title | A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure Models |
| title_full | A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure Models |
| title_fullStr | A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure Models |
| title_full_unstemmed | A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure Models |
| title_short | A High-precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multilayer Internal Structure Models |
| title_sort | high precision dynamical model of callisto incorporating rotation effects within multilayer internal structure models |
| topic | Celestial mechanics Astrometry Ephemerides Natural satellite dynamics Jovian satellites Galilean satellites |
| url | https://doi.org/10.3847/1538-4357/adfe65 |
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