Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/111698
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dc.contributorResearch Centre for Deep Space Explorations-
dc.contributorDepartment of Land Surveying and Geo-Informatics-
dc.creatorChen, S-
dc.creatorWu, B-
dc.creatorLi, H-
dc.creatorLi, Z-
dc.creatorLiu, Y-
dc.date.accessioned2025-03-13T02:22:05Z-
dc.date.available2025-03-13T02:22:05Z-
dc.identifier.urihttp://hdl.handle.net/10397/111698-
dc.language.isoenen_US
dc.publisherEDP Sciencesen_US
dc.rights© The Authors 2024en_US
dc.rightsOpen 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.en_US
dc.rightsThe following publication Chen, S., Wu, B., Li, H., Li, Z., & Liu, Y. (2024). Asteroid-NeRF: A deep-learning method for 3D surface reconstruction of asteroids. A&A, 687, A278 is available at https://doi.org/10.1051/0004-6361/202450053.en_US
dc.subjectMinor planets, asteroids: generalen_US
dc.subjectPlanets and satellites: surfacesen_US
dc.subjectTechniques: image processingen_US
dc.titleAsteroid-NeRF : a deep-learning method for 3D surface reconstruction of asteroidsen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.volume687-
dc.identifier.doi10.1051/0004-6361/202450053-
dcterms.abstractContext. Asteroids preserve important information about the origin and evolution of the Solar System. Three-dimensional (3D) surface models of asteroids are essential for exploration missions and scientific research. Regular methods for 3D surface reconstruction of asteroids, such as stereo-photogrammetry (SPG), usually struggle to reconstruct textureless areas and can only generate sparse surface models. Stereo-photoclinometry (SPC) can reconstruct pixel-wise topographic details but its performance depends on the availability of images obtained under different illumination conditions and suffers from uncertainties related to surface reflectance and albedo.-
dcterms.abstractAims. This paper presents Asteroid-NeRF, a novel deep-learning method for 3D surface reconstruction of asteroids that is based on the state-of-the-art neural radiance field (NeRF) method.-
dcterms.abstractMethods. Asteroid-NeRF uses a signed distance field (SDF) to reconstruct a 3D surface model from multi-view posed images of an asteroid. In addition, Asteroid-NeRF incorporates appearance embedding to adapt to different illumination conditions and to maintain the geometric consistency of a reconstructed surface, allowing it to deal with the different solar angles and exposure conditions commonly seen in asteroid images. Moreover, Asteroid-NeRF incorporates multi-view photometric consistency to constrain the SDF, enabling optimised reconstruction.-
dcterms.abstractResults. Experimental evaluations using actual images of asteroids Itokawa and Bennu demonstrate the promising performance of Asteroid-NeRF, complementing traditional methods such as SPG and SPC. Furthermore, due to the global consistency and pixel-wise training of Asteroid-NeRF, it produces highly detailed surface reconstructions. Asteroid-NeRF offers a new and effective solution for high-resolution 3D surface reconstruction of asteroids that will aid future exploratory missions and scientific research on asteroids.-
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationAstronomy and astrophysics, July 2024, v. 687, A278-
dcterms.isPartOfAstronomy and astrophysics-
dcterms.issued2024-07-
dc.identifier.scopus2-s2.0-85199490015-
dc.identifier.eissn2331-7019-
dc.identifier.artnA278-
dc.description.validate202503 bcch-
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_Othersen_US
dc.description.fundingSourceRGCen_US
dc.description.pubStatusPublisheden_US
dc.description.oaCategoryCCen_US
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