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...

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Published in:The Astrophysical Journal
Main Authors: Kai Huang, Yongzhang Yang, Yuhao Chen, Yining Zhang, Yuqiang Li
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adfe65
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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.
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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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