{"title":"Precision in planetary exploration: Crater detection with residual U-Net34/50 and matching template algorithm","authors":"Ritik Raju Mohite , Sushil Kumar Janardan , Rekh Ram Janghel , Himanshu Govil","doi":"10.1016/j.pss.2024.106029","DOIUrl":null,"url":null,"abstract":"<div><div>Counting craters on celestial bodies such as the Moon is essential for understanding the Solar System's evolution and its dynamic past. The conventional crater recognition methods rely heavily on human observation, often paired with standard machine learning techniques. However, these methods face obstacles, like the absence of an objective criterion and challenges in achieving accurate recognition results for overlapping or smaller craters. To mitigate these issues, our proposed solution involves implementing a convolutional neural network known as the Residual U-Net-34 and Residual U-Net-50. These models are designed to effectively identify craters within lunar Digital Elevation Model (DEM) images. The initial step of our method involves the emphasizing of crater edges and suppressing the other surfaces within lunar DEM data. Following edge detection, we employ matching template algorithm to calculate the size and positions of craters within the lunar DEM data. In the Residual U-Net-34 and Residual U-Net-50 architectures, the framework extends the U-Net model by incorporating the residual convolution block, departing from conventional convolution methods. This hybridization leverages the strengths of both U-Net and residual networks. Remarkably, Residual U-Net-34 and Residual U-Net-50 maintains the input and output image sizes, simplifying the training process due to its use of residual units. This design also enables straightforward optimization of the proposed model. The approach focuses on crater rims and demonstrates the ability to identify overlapping craters. Within the domain of lunar crater recognition, our model demonstrates elevated performance with a recall of 77.22% and precision of 83.67% when operating on DEM data. Notably, the recall and precision outperform other deep learning methods. These experimental outcomes validate the feasibility of leveraging our network for crater recognition within lunar DEM datasets.</div></div>","PeriodicalId":20054,"journal":{"name":"Planetary and Space Science","volume":"255 ","pages":"Article 106029"},"PeriodicalIF":1.8000,"publicationDate":"2025-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Planetary and Space Science","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0032063324001934","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Counting craters on celestial bodies such as the Moon is essential for understanding the Solar System's evolution and its dynamic past. The conventional crater recognition methods rely heavily on human observation, often paired with standard machine learning techniques. However, these methods face obstacles, like the absence of an objective criterion and challenges in achieving accurate recognition results for overlapping or smaller craters. To mitigate these issues, our proposed solution involves implementing a convolutional neural network known as the Residual U-Net-34 and Residual U-Net-50. These models are designed to effectively identify craters within lunar Digital Elevation Model (DEM) images. The initial step of our method involves the emphasizing of crater edges and suppressing the other surfaces within lunar DEM data. Following edge detection, we employ matching template algorithm to calculate the size and positions of craters within the lunar DEM data. In the Residual U-Net-34 and Residual U-Net-50 architectures, the framework extends the U-Net model by incorporating the residual convolution block, departing from conventional convolution methods. This hybridization leverages the strengths of both U-Net and residual networks. Remarkably, Residual U-Net-34 and Residual U-Net-50 maintains the input and output image sizes, simplifying the training process due to its use of residual units. This design also enables straightforward optimization of the proposed model. The approach focuses on crater rims and demonstrates the ability to identify overlapping craters. Within the domain of lunar crater recognition, our model demonstrates elevated performance with a recall of 77.22% and precision of 83.67% when operating on DEM data. Notably, the recall and precision outperform other deep learning methods. These experimental outcomes validate the feasibility of leveraging our network for crater recognition within lunar DEM datasets.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research