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Automatic Characterization of Boulders on Planetary Surfaces From High‐Resolution Satellite Images.

Authors :
Prieur, Nils C.
Amaro, Brian
Gonzalez, Emiliano
Kerner, Hannah
Medvedev, Sergei
Rubanenko, Lior
Werner, Stephanie C.
Xiao, Zhiyong
Zastrozhnov, Dmitry
Lapôtre, Mathieu G. A.
Source :
Journal of Geophysical Research. Planets; Nov2023, Vol. 128 Issue 11, p1-22, 22p
Publication Year :
2023

Abstract

Boulders form from a variety of geological processes, which their size, shape, and orientation may help us better understand. Furthermore, they represent potential hazards to spacecraft landing that need to be characterized. However, mapping individual boulders across vast areas is extremely labor‐intensive, often limiting the extent over which they are characterized and the statistical robustness of obtained boulder morphometrics. To automate boulder characterization, we use an instance segmentation neural network, Mask R‐CNN, to detect and outline boulders in high‐resolution satellite and aerial images. Our neural network, BoulderNet, was trained from a data set of >33,000 boulders in >750 image tiles from Earth, the Moon, and Mars. BoulderNet not only correctly detects the majority of boulders in images but also identifies the outline of boulders with high fidelity, achieving average precision and recall values of 72% and 64% relative to manually digitized boulders from the test data set, when only detections with intersection‐over‐union ratios >50% are considered valid. These values are similar to those obtained from human mappers. On Earth, equivalent boulder diameters, aspect ratios, and orientations extracted from predictions were benchmarked against ground measurements and yield values within ±15%, ±0.20, and ±20° of their ground‐truth values, respectively. BoulderNet achieves better boulder detection and characterization performance relative to existing methods, providing a versatile open‐source tool to characterize entire boulder fields on planetary surfaces. Plain Language Summary: Boulders are one of the most abundant features on the surfaces of solid planetary bodies. Measuring their size, shape, and orientation can tell us about how they formed as well as help select landing sites that minimize hazard to spacecraft. However, mapping boulders across large areas is a labor‐intensive task that often limits the scope and robustness of boulder studies. To overcome this challenge, we trained a machine‐learning algorithm to automatically outline boulders on a variety of planetary surfaces using a database of over 30,000 boulders manually mapped from aerial or satellite images of Earth, the Moon, and Mars. Our algorithm, BoulderNet, performs as well as human mappers and outperforms existing automated tools. BoulderNet is made available to the community. Key Points: We describe BoulderNet, a Mask R‐CNN instance segmentation model trained to characterize boulders on the surfaces of solid planetary bodiesBoulderNet achieves robust performance on Earth, the Moon, and Mars, outlining boulders with high fidelityBoulderNet achieves better boulder detection and morphometric characterization performances than other existing methods [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
21699097
Volume :
128
Issue :
11
Database :
Complementary Index
Journal :
Journal of Geophysical Research. Planets
Publication Type :
Academic Journal
Accession number :
173892975
Full Text :
https://doi.org/10.1029/2023JE008013