Abstract

Impact cratering process is the major geologic activity on the surface of the Moon, and the spatial distribution and size-frequency distribution of lunar craters are indicative to the bombardment history of the Solar System. The substantial efforts on the development of automated crater detection algorithms (CDAs) have been carried out on the images from the remote sensing observations. Recently, CDAs via convolutional neural network (CNN) on digital elevation model (DEM) has been developed as it can combine the discrimination ability of CNN with the robust characteristic of the DEM data. However, most of the existing algorithms adopt a traditional two-stage detection pipeline including an edge segmentation and a template matching step. In this paper, we attempt to reduce the gap between the existing DEM-based CDAs and the advanced CNN methods for object detection, and propose a complete workflow including an end-to-end deep learning pipeline for lunar crater detection, in particular for craters smaller than 50 km in diameter. Based on the workflow, we benchmark nine representative CNN models involving three popular types of detection architectures. Moreover, we elaborate on the practical application of the proposed workflow, and provide an example method to demonstrate the performance advantage in terms of the precision (82.97%) and recall (79.39%). Furthermore, we develop a crater verification tool to manually validate the detection results, and the visualization results show that our detected craters are reasonable and can be used as a supplement to the existing hand-labeled datasets.

Highlights

  • Impact cratering process is the major geologic activity on the surface of the Moon, and the spatial distribution and size-frequency distribution of lunar craters are indicative to the bombardment history of the Solar System

  • For the crater information, we used the two released hand-labeled datasets, in which Povilaitis et al [5] annotated the craters with a diameter between 5 and 20 km based on the Lunar Reconnaisance Orbiter (LRO) Wide Angle Camera (WAC) digital elevation model (DEM) data [45] with a resolution of 303 pixels/degree, and Head et al [2] exploited the craters for a diameter larger than 20 km according to the Lunar Orbiter Laser Altimeter (LOLA) DEM data with a resolution of 64 pixels/degree

  • The value of the second hyper-parameter is associated with the real distribution of lunar craters with different degrees of overlaps, since it is used to remove the duplicate craters with geographical coordinates in a global DEM image

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Summary

Introduction

Impact cratering process is the major geologic activity on the surface of the Moon, and the spatial distribution and size-frequency distribution of lunar craters are indicative to the bombardment history of the Solar System. We attempt to reduce the gap between the existing DEM-based CDAs and the advanced CNN methods for object detection, and propose a complete workflow including an end-to-end deep learning pipeline for lunar crater detection, in particular for craters smaller than 50 km in diameter. As the bombardment flux of the Solar System decreases with the increases of time, the density and size-frequency distribution of craters over the lunar surface directly provide the critical information on the relative age of the mare units on the. The manual detection is very time-consuming and is difficult for exhaustive coverage, in particular for small or overlapping craters at specific geographic region [2,5]

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