Issue |
A&A
Volume 696, April 2025
|
|
---|---|---|
Article Number | A212 | |
Number of page(s) | 11 | |
Section | Planets, planetary systems, and small bodies | |
DOI | https://doi.org/10.1051/0004-6361/202452844 | |
Published online | 25 April 2025 |
Modeling the global shape and surface morphology of the Ryugu asteroid using an improved neural implicit method
1
Institute of Geodesy and Geoinformation Science, Technische Universität Berlin,
Berlin
10553,
Germany
2
Institute of Planetary Research, German Aerospace Center (DLR),
Berlin
12489,
Germany
3
Institute of Geological Sciences, Freie Universität Berlin,
Berlin
12249,
Germany
4
Institute of Space Technology & Space Applications (LRT 9.1), University of the Bundeswehr Munich,
Neubiberg
85577,
Germany
5
Instituto de Astrofísica de Andalucía (IAA-CSIC),
Granada
18008,
Spain
★ Corresponding authors: hao.chen.2@campus.tu-berlin.de; hxiao@iaa.es
Received:
1
November
2024
Accepted:
25
March
2025
Context. Detailed shape modeling is a fundamental task in the context of small body exploration aimed at supporting scientific research and mission operations. The neural implicit method (NIM) is a novel deep learning technique that models the shapes of small bodies from multi-view optical images. While it is able to generate models from a small set of images, it encounters challenges in accurately reconstructing small-scale or irregularly shaped boulders on Ryugu, which hinders the investigation of detailed surface morphology.
Aims. Our goal is to accurately reconstruct a high-resolution shape model with refined terrain details of Ryugu based on a limited number of images.
Methods. We propose an improved NIM that leverages multi-scale deformable grids to flexibly represent the complex geometric structures of various boulders. To enhance the surface accuracy, three-dimensional (3D) points derived from the Structure-from-Motion plus Multi-View Stereo (SfM-MVS) method were incorporated to provide explicit supervision during network training. We selected 131 Optical Navigation Camera Telescope images from two different mission phases at different spatial resolutions to reconstruct two Ryugu shape models for performance evaluation.
Results. The proposed method effectively addresses the challenges encountered by NIM and demonstrates an accurate reconstruction of high-resolution shape models of Ryugu. The volume and surface area of our NIM models are closely aligned with those of the prior shape model derived from the SfM-MVS method. However, despite utilizing fewer images, the proposed method achieves a higher resolution and refinement performance in polar regions and for irregularly shaped boulders, compared to the SfM-MVS model. The effectiveness of the method applied to Ryugu suggests that it holds significant potential for applications to other small bodies.
Key words: techniques: image processing / planets and satellites: surfaces / minor planets, asteroids: individual: Ryugu
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.