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A new preprint from the Impact AI team at NASA’s Marshall Space Flight Center in Huntsville, Alabama, and IBM Research presents early results in the process to build a foundation model for the Martian atmosphere, combining data-driven learning with novel algorithmic approaches for sparse planetary data.

The arXiv preprint paper submitted on May 16, 2026 lays out the design and algorithmic roadmap for a Mars atmospheric Foundation Model. “Towards a Foundation Model for the Martian Atmosphere” describes how a single model with physics-informed pretraining and data assimilation can represent, forecast, and detect distinct phenomena within the Martian atmosphere.

Building such a model is not straightforward. General circulation models can simulate Martian atmospheric behavior, but they grow computationally expensive at resolutions needed to capture mesoscale features. The observational record compounds the difficulty as these observations are sparse, short, and fragmented across instrument generations.

To work within those constraints, the team characterized available data sources, including OpenMARS reanalysis, orbital retrievals, and Mars Global Climate Model (GCM) outputs. They then evaluated three architectures: a Mars-adapted GraphCast (graph neural network), a Mars-adapted Prithvi Weather and Climate (vision transformer), and a Spectral-LS transformer trained on OpenMARS surface variables. They also explored pretraining based on partial differential equations as a strategy to improve model skill in data-limited settings.

The Spectral-LS transformer outperforms persistence for wind and surface pressure forecasts over 24-hour horizons, an encouraging early result. Dust column opacity remains challenging across all three architectures and is an open problem the team continues to tackle. Beyond forecasting, the paper surveys AI-based data assimilation approaches as a path toward ingesting sparse orbital observations directly into the model state, a critical capability given that observational records of Mars are fragmented.

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Four rows of graphs show the zonal and meridional wind speed from Mars Year 35, and the Spectral-LS model predictions that go along with them. The predictions are very close to the ground truth. Redder areas represent faster wind speeds, while bluer areas represent slower speeds.
Zonal (u) and meridional (v) wind forecast evolution using the Spectral-LS model, for a test sample from Mars Year 35 at Ls = 71.7° (northern spring). Each column shows a different forecast lead time from +2h to +24h. For each variable, the top row shows the model prediction and the bottom row shows the corresponding ground truth from OpenMARS reanalysis. The model captures the large-scale zonal jet structure and meridional circulation patterns throughout the 24-hour rollout, with errors growing gradually at smaller spatial scales. Grid resolution is 5° × 5° (36 × 72). Image credit: NASA Impact AI team

The work may lead to better Martian weather forecasting and could support future planetary surface operations, aligning with NASA’s Science Mission Directorate planetary science objectives.

Learn more about NASA’s AI for Science efforts: science.nasa.gov/artificial-intelligence-science