This investigation further gauged the Beta-Variational Autoencoder's ability to locate anomalous surface features, successfully recovering two places of interest and numerous landed technological assets at a statistically significant rate.
Abstract
The Lunar Reconnaissance Orbiter (LRO) has been collecting high-resolution images (at around 0.5-2 meters per pixel linearly with its Narrow Angle Camera) of the Moon since 2009, amassing a large dataset of images and offering researchers the opportunity to study the surface of the Moon at unprecedented scale. Here, we aim to test the abilities of the Beta-Variational Autoencoder (VAE) created by Lesnikowski et al. (2024), an unsupervised learning model which identifies anomalous features across the Moon's surface, locating not only scientifically useful geologic formations such as rockfall deposits, fresh impact craters, irregular mare patches, or volcanic pits/collapsed lava tubes, but also artificial objects such as landed spacecraft. This investigation further gauged the model's ability to locate anomalous surface features, successfully recovering two places of interest (Plaskett Crater and Paracelsus C Crater) and numerous landed technological assets at a statistically significant rate.
Lunarfm is introduced, a multimodal foundation model that learns a general representation of the lunar surface from diverse orbital measurements, and demonstrates that this embedding space supports a diverse range of downstream applications, enabling efficient scientific investigation and resource-oriented analysis.
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Identified as the planetary science top highest-priority objective for the next NASA decadal survey, the exploration of the Uranian planetary system requires advanced multispectral instrumentation to characterize the geomorphology and composition of its icy moons, Uranus’ rings and atmosphere. This paper presents the c...
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The potentially hazardous asteroid (153814) 2001 WN$_5$ will pass inside the lunar distance on June 26, 2028, offering a rare opportunity to characterize a kilometer-scale near-Earth asteroid at high angular resolution. We aim to constrain the rotation state, shape, visible colors, geometric albedo, and taxonomy of 200...
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A novel unsupervised framework based on Variational Autoencoders (VAEs) to automatically sift through the XSA, which provides a scalable screening tool for multi-band light curves generated by the EPIC-pn Pipeline Processing System (PPS).
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The compact atmospheric microwave sounder (CAMS) aboard the commercial TianYan-16 satellite is a cross-track scanning radiometer with two separate cold-space view on its left and right sides. During on-orbit operation, the Moon regularly intrudes into one deep-space view (DSV), producing abnormal cold-space counts and...
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