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Stanford's STEHM model helps astronomers screen exoplanets for atmosphere retention and habitability

By

Samantha Mathewson

2d ago· 4 min readenNews

Summary

Stanford researchers have developed a new planetary habitability model called STEHM (Smaller Than Earth Habitability Model) that helps astronomers efficiently screen exoplanets for their ability to build and retain atmospheres over billions of years. The model allows scientists to quickly identify rocky worlds unlikely to sustain life-supporting atmospheres before committing valuable telescope time to detailed observations, potentially making the search for extraterrestrial life more targeted and efficient.

Source

Twitter / XStanford's STEHM model helps astronomers screen exoplanets for atmosphere retention and habitabilityspace.com

Key quotes

· 2 pulled
The software, called the Smaller Than Earth Habitability Model (STEHM), allows astronomers to screen exoplanets before committing valuable telescope time to detailed observations.
Developed by researchers at Stanford University, the model assesses whether a rocky planet can build and retain an atmosphere over billions of years — a prerequisite for life as we know it.
Snippet from the RSS feed
A new exoplanet model screens rocky worlds by their ability to retain atmospheres over geologic timescales, helping narrow the search for potentially habitable planets beyond Earth.

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