A Deep Learning-based Approach to 3D Reconstruction of Asteroids Using Ground-based Radar Data
The principal method employed for the three-dimensional(3D) reconstruction of asteroids is the optimisation method based on spherical harmonic functions. Nevertheless, this approach is inherently time-consuming and prone to local optima, which can lead to the emergence of distortions in the resulting 3D shapes. In order to address these issues, this paper puts forward a deep learning-based method for the reconstruction of asteroids in three dimensions. The dataset employed for the deep learning method comprises multi-angle range-Doppler images of asteroids consisting of a range of shapes. In order to demonstrate the robustness of this method, this paper presents the reconstruction of 3D models of asteroids with several different shapes. This paper provides a comparison of the reconstruction accuracy. The above analysis demonstrates that the proposed method is effective in reconstructing 3D models of asteroids. This paper improves the limitations of conventional methods.
Authors
- Ziyang Pan
- Zehua Dong (ORCID: https://orcid.org/0000-0002-2327-3824)
- Yan Chen (ORCID: https://orcid.org/0009-0005-0674-2675)
- Zhuangzhuang Tian (ORCID: https://orcid.org/0000-0002-3685-1742)
- Chunyi Zhou (ORCID: https://orcid.org/0009-0008-6524-8142)
- Zegang Ding
Institutions
- Beijing Institute of Technology (CN)
Publication Details
- Published
- 2024-11-22
- DOI
- https://doi.org/10.1109/icsidp62679.2024.10867950
- Primary Topic
- Astro and Planetary Science
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Natural Science Foundation of China
- Natural Science Foundation of Chongqing