LLMs in dynamical (and general) astronomy
How large language models are transforming astronomical research in celestial mechanics and dynamical astronomy.
Smirnov, Evgeny & Carruba, Valerio (2026)
Benchmark shows multimodal LLMs can classify orbital resonances from images with high accuracy without fine-tuning.
The study introduces reproducible benchmarks for testing multimodal LLMs on classifying mean-motion and secular resonances from plots of resonant arguments. Commercial models achieved perfect scores on unambiguous cases and up to 94% F1 on a harder three-class dataset, while open-source models approached commercial performance on the full binary benchmark. The main weakness was identifying transient and resonance-sticking behavior, but the results indicate that even untuned, locally runnable models can be useful for dynamical-astronomy classification.
Benchmarking multimodal commercial and open-source LLMs on image-based classification of dynamical resonance behavior.
Basic knowledge of orbital dynamics, mean-motion and secular resonances, and machine-learning evaluation metrics.
How large language models are transforming astronomical research in celestial mechanics and dynamical astronomy.
A companion collection for the ACM 2026 talk by Valerio Carruba
Have no resources to use the commercial models? Use OSS! You can even launch them on your laptop. And they ARE good.
— ES