philippbaumeister/ExoMDN
Rapid characterization of exoplanet interiors with Mixture Density Networks
Quickly determine the internal composition of low-mass exoplanets from observational data. You provide the exoplanet's mass, radius, and equilibrium temperature, and it outputs a full inference of its interior structure. This tool is designed for astronomers and planetary scientists studying exoplanet characteristics.
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Use this if you need rapid, detailed insights into exoplanet interiors without running complex, time-consuming dedicated models.
Not ideal if you are studying exoplanets outside the low-mass range or require a full-physics simulation for interior modeling.
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11
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3
Language
Jupyter Notebook
License
MIT
Category
Last pushed
Aug 07, 2025
Commits (30d)
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