Abstract

Lunar crater detection plays an important role in lunar exploration, while machine learning (ML) exhibits promising advantages in the field. However, previous ML works almost all used a single type of lunar map, such as an elevation map (DEM) or orthographic projection map (WAC), to extract crater features; the two types of images have individual limitations on reflecting the crater features, which lead to insufficient feature information, in turn influencing the detection performance. To address this limitation, we, in this work, propose feature complementary of the two types of images and accordingly explore an advanced dual-path convolutional neural network (Dual-Path) based on a U-NET structure to effectively conduct feature integration. Dual-Path consists of a contracting path, bridging path, and expanding path. The contracting path separately extracts features from DEM and WAC images by means of two independent input branches, while the bridging layer integrates the two types of features by 1 × 1 convolution. Finally, the expanding path, coupled with the attention mechanism, further learns and optimizes the feature information. In addition, a special deep convolution block with a residual module is introduced to avoid network degradation and gradient disappearance. The ablation experiment and the comparison of four competitive models only using DEM features confirm that the feature complementary can effectively improve the detection performance and speed. Our model is further verified by different regions of the whole moon, exhibiting high robustness and potential in practical applications.

Highlights

  • The moon is the first choice for human astronomical activities and space exploration activities, which are of great significance to human development

  • With the feature integration strategy, we explored a dual input convolutional neural network based on the U-NET structure, called

  • In order to validate the impact of the feature complementary of the digital elevation map (DEM) and Wide-Angle Camera (WAC)

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Summary

Introduction

The moon is the first choice for human astronomical activities and space exploration activities, which are of great significance to human development. Impact craters are the most obvious and main morphological features on the lunar surface, which could provide important clues for studying the evolutionary history of the moon and space exploration. Many efforts have been devoted to recognizing lunar impact craters, including artificial recognition [1,2,3,4], image transformation and segmentation [5,6,7], geoscience information analysis [8,9], and machine learning [10,11,12]. Artificial recognition is a method in which experts or other astronomers use telescopes to take pictures and mark impact craters manually in lunar images. The methods based on the image transformation and segmentation use different filtering and detection algorithms to recognize the image features of the lunar surface, while the method based on geoscience information analysis is to use the information from slopes, textures, and curvature of slopes

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