Abstract

This paper introduces a new GeoAI solution to support automated mapping of global craters on the Mars surface. Traditional crater detection algorithms suffer from the limitation of working only in a semiautomated or multi-stage manner, and most were developed to handle a specific dataset in a small subarea of Mars’ surface, hindering their transferability for global crater detection. As an alternative, we propose a GeoAI solution based on deep learning to tackle this problem effectively. Three innovative features are integrated into our object detection pipeline: (1) a feature pyramid network is leveraged to generate feature maps with rich semantics across multiple object scales; (2) prior geospatial knowledge based on the Hough transform is integrated to enable more accurate localization of potential craters; and (3) a scale-aware classifier is adopted to increase the prediction accuracy of both large and small crater instances. The results show that the proposed strategies bring a significant increase in crater detection performance than the popular Faster R-CNN model. The integration of geospatial domain knowledge into the data-driven analytics moves GeoAI research up to the next level to enable knowledge-driven GeoAI. This research can be applied to a wide variety of object detection and image analysis tasks.

Highlights

  • Leveraging the advantages of GeoAI, we developed a deep learning model that enables multi-scale learning and crater detection on Mars

  • All craters in the images are annotated with instance-level bounding boxes (BBOXes) utilizing the Martian impact crater database by Robbins and Hynek [14]

  • The Mars global mosaic [16] consists of 2001 Mars Odyssey Thermal Emission Imagining System (THEMIS) daytime infrared (DIR) data with 100 m spatial resolution and global coverage

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Summary

Introduction

Impact craters have been important in the development of our understanding of the geological history of the Solar System. Scientists observe the number, size, shape, distribution or the density of craters on planets to learn about the geological processes of those bodies without landing on the surfaces [1,2,3,4,5]. Crater counts are used to estimate the age of planetary surfaces [6,7], while crater characteristics such as distribution and size-density are leveraged to understand geological processes [8,9]. Over several decades of research, impact craters have been cataloged by various methods, including visual/infrared imagery and digital elevation models (DEMs) of a planet’s surface [12,13,14,15]

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