Crater-MASN: A Multi-Scale Adaptive Semantic Network for Efficient Crater Detection.
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| Title: | Crater-MASN: A Multi-Scale Adaptive Semantic Network for Efficient Crater Detection. |
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| Authors: | Yu, Ruiqi1 (AUTHOR), Xu, Zhijing1 (AUTHOR) zjxu@shmtu.edu.cn |
| Source: | Remote Sensing. Sep2025, Vol. 17 Issue 18, p3139. 27p. |
| Subjects: | Lunar craters, Planetary science, Impact craters, Feature extraction, Semantic networks (Information theory), Software frameworks, Mechanical efficiency |
| Abstract: | Highlights: What are the main findings? A lightweight multi-scale framework, Crater-MASN, is proposed to balance high accuracy with computational efficiency. A novel training and post-processing pipeline enables robust detection in dense, nested regions and demonstrates an exceptional capability for discovering previously uncatalogued craters. What is the implication of the main finding? Crater-MASN provides a scalable and efficient tool for planetary scientists to perform large-scale, high-precision crater cataloging and planetary surface analysis. The model's proven ability to identify uncatalogued craters demonstrates its significant potential for scientific discovery and the completion of existing lunar databases. Automatic crater detection is crucial for planetary science, but still faces several long-standing challenges. The morphological characteristics of craters exhibit significant variability; combined with complex lighting conditions, this makes feature extraction difficult, especially for small or severely degraded features. These difficulties are further compounded by incomplete ground truth annotations, which limit the effectiveness of supervised learning. In addition, achieving a balance between detection accuracy and computational efficiency remains a critical bottleneck, especially in large-scale planetary surveys. Traditional postprocessing algorithms also often struggle to resolve complex spatial hierarchies in densely cratered regions, leading to substantial omissions and misclassifications. To address these interrelated challenges, we propose Crater-MASN, a lightweight adaptive detection framework specifically designed for lunar crater analysis. The architecture employs a compact GhostNet backbone to balance efficiency and accuracy, while enhancing multi-scale feature representation through a novel bidirectional integration and fusion module (BIFM) to better capture the morphological diversity of craters. To mitigate the impact of incomplete annotations, we introduce an adaptive semantic contrastive sampling (ASCS) mechanism which dynamically mines unlabeled craters through semantic clustering and contrastive learning. Additionally, we design the hierarchical soft NMS (H-SoftNMS) algorithm, a geometry-aware postprocessing method that selectively suppresses non-hierarchical overlaps to preserve nested craters, thereby achieving more accurate crater retention in dense regions. Experiments on a dedicated lunar crater dataset demonstrate the effectiveness of Crater-MASN. The model achieves an mAP50 of 91.0% with only 2.1 million parameters. When combined with H-SoftNMS, it achieves a recall rate of 95.0% and new discovery rate P NDR of 89.6%. These results highlight the potential of Crater-MASN as a scalable and reliable tool for high-precision crater cataloging and planetary surface analysis. [ABSTRACT FROM AUTHOR] |
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| Database: | Engineering Source |
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| Abstract: | Highlights: What are the main findings? A lightweight multi-scale framework, Crater-MASN, is proposed to balance high accuracy with computational efficiency. A novel training and post-processing pipeline enables robust detection in dense, nested regions and demonstrates an exceptional capability for discovering previously uncatalogued craters. What is the implication of the main finding? Crater-MASN provides a scalable and efficient tool for planetary scientists to perform large-scale, high-precision crater cataloging and planetary surface analysis. The model's proven ability to identify uncatalogued craters demonstrates its significant potential for scientific discovery and the completion of existing lunar databases. Automatic crater detection is crucial for planetary science, but still faces several long-standing challenges. The morphological characteristics of craters exhibit significant variability; combined with complex lighting conditions, this makes feature extraction difficult, especially for small or severely degraded features. These difficulties are further compounded by incomplete ground truth annotations, which limit the effectiveness of supervised learning. In addition, achieving a balance between detection accuracy and computational efficiency remains a critical bottleneck, especially in large-scale planetary surveys. Traditional postprocessing algorithms also often struggle to resolve complex spatial hierarchies in densely cratered regions, leading to substantial omissions and misclassifications. To address these interrelated challenges, we propose Crater-MASN, a lightweight adaptive detection framework specifically designed for lunar crater analysis. The architecture employs a compact GhostNet backbone to balance efficiency and accuracy, while enhancing multi-scale feature representation through a novel bidirectional integration and fusion module (BIFM) to better capture the morphological diversity of craters. To mitigate the impact of incomplete annotations, we introduce an adaptive semantic contrastive sampling (ASCS) mechanism which dynamically mines unlabeled craters through semantic clustering and contrastive learning. Additionally, we design the hierarchical soft NMS (H-SoftNMS) algorithm, a geometry-aware postprocessing method that selectively suppresses non-hierarchical overlaps to preserve nested craters, thereby achieving more accurate crater retention in dense regions. Experiments on a dedicated lunar crater dataset demonstrate the effectiveness of Crater-MASN. The model achieves an mAP50 of 91.0% with only 2.1 million parameters. When combined with H-SoftNMS, it achieves a recall rate of 95.0% and new discovery rate P NDR of 89.6%. These results highlight the potential of Crater-MASN as a scalable and reliable tool for high-precision crater cataloging and planetary surface analysis. [ABSTRACT FROM AUTHOR] |
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| ISSN: | 20724292 |
| DOI: | 10.3390/rs17183139 |
