NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Multimodal-Multiresolution Foundation Model for Lunar Remote SensingWe present a multimodal foundation model for lunar remote sensing, pretrained from scratch on SomBench, a co-registered corpus of nearly two million tile bundles spanning 11 modalities at two spatial scales (i.e., 1 m/pixel and 100 m/pixel). The dataset is geographically partitioned to prevent leakage across train, validation, and test splits. The model adapts the TerraMind masked-token architecture to the lunar setting with two extensions: per-tile acquisition geometry (i.e., illumination angles, solar-frame anchors, tile footprint) is provided as explicit contextual information rather than requiring the model to infer it implicitly from image content; and tiles anchored at meter and hundred-meter scale are trained jointly in a mixed-batch regime so that a single set of weights covers both resolution families. A FlexiViT patch-embedding scheme allows the same pretrained checkpoint to be reused at different working patch sizes without backbone retraining, and modality-wise tokenization lets downstream users drop or add modalities at fine-tuning time. Qualitative generation experiments indicate that the model captures meaningful cross-modal correspondences (i.e., terrain derivatives from elevation, illumination-consistent reflectance from geometry, and coarse spatial pattern across co-registered modality sets). Evaluated across four downstream benchmarks (i.e., crater detection at 100 m/pixel and NAC 1 m/pixel imagery, irregular mare patch segmentation, and polar ice prospectivity regression) using TerraTorch, the pretrained model matches or outperforms ImageNet-pretrained baselines and an architecturally identical random-initialization control. On multimodal ice prospectivity regression at the poles, the pretrained model variants (i.e., full finetuning, Low-Rank Adaptation (LoRA) and frozen) outperform all baselines by margins that exceed run-to-run variability, with the randomly initialized version of our model that beats all but one baselines. This indicates that part of the gain comes from our architecture’s native token-level multimodal processing rather than from pretraining alone. Label efficiency is particularly pronounced for crater detection: at 50% training data on crater detection at 100 m/pixel, the pretrained model already exceeds the strongest ImageNet baseline trained on the full dataset. Among adaptation strategies, LoRA matches or surpasses full fine-tuning on crater detection and irregular mare patches segmentation, using a small fraction of the trainable parameters with lower run-to-run variance. Full fine-tuning remains best on ice-prospectivity regression, with LoRA that however still beats all baselines. We release the pretrained checkpoint, fine-tuning code, and benchmark datasets to support reproducibility and community reuse.
Document ID
20260008697
Acquisition Source
Marshall Space Flight Center
Document Type
White Paper
Authors
Paolo Fraccaro
(IBM Research - Zurich Rüschlikon, Switzerland)
Gabrielle Nyirjesy
(IBM Research - Thomas J. Watson Research Center Yorktown Heights, United States)
Daniela Szwarcman
(IBM Research - Zurich Rüschlikon, Switzerland)
Himanshu Patil
(The University of Alabama in Huntsville (UAH) Huntsville, AL, United States)
Vishal Gaur
(University of Alabama in Huntsville Huntsville, United States)
Rohit Lal
(University of Alabama in Huntsville Huntsville, United States)
Rachel A Slank
(Universities Space Research Association Columbia, United States)
Geoffrey Dawson
(IBM Research - Thomas J. Watson Research Center Yorktown Heights, United States)
Hiyam Debary
(IBM Research - Thomas J. Watson Research Center Yorktown Heights, United States)
Michael K Barker
(Goddard Space Flight Center Greenbelt, United States)
Andrew Annex
(SETI Institute Mountain View, California, United States)
Vishnu Viswanathan
(University of Maryland, Baltimore County (UMBC) Baltimore, MD, United States)
Zachary Morse
(Howard Univ. Washington, DC United States)
Ethan I Schaefer
(SETI Institute Mountain View, California, United States)
Nikolaos Dionelis
(University of Alabama in Huntsville Huntsville, United States)
Ankur Kumar
(University of Alabama in Huntsville Huntsville, United States)
Campbell D Watson
(IBM Research - Thomas J. Watson Research Center Yorktown Heights, United States)
Manil Maskey
(Marshall Space Flight Center Redstone Arsenal, United States)
Rebekah I Dawson-Rigas
(National Aeronautics and Space Administration Washington, United States)
Juan Bernabe-Moreno
(IBM Research - Ireland Dublin, Ireland)
Rahul Ramachandran
(Marshall Space Flight Center Redstone Arsenal, United States)
Sujit Roy
(University of Alabama in Huntsville Huntsville, United States)
Date Acquired
September 9, 2026
Publication Date
September 23, 2026
Publication Information
Subject Category
Earth Resources and Remote Sensing
Funding Number(s)
CONTRACT_GRANT: 80MSFC25M0084
CONTRACT_GRANT: 80MSFC22M0004
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
Single Expert
No Preview Available