JWST Detects Exoplanet Atmospheres
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87% Informative
Direct imaging of exoplanets is rare due to the extreme contrast between stars and their planets.
The brightness difference between a star and its orbiting exoplanet can be enormous, often exceeding a factor of a billion .
By studying these objects, researchers can test theories about how gas giants like Jupiter and Saturn formed.
The JWST , with its ability to detect infrared light, can observe much cooler and smaller planets than ever before.
By directly imaging exoplanets, scientists can better understand their atmospheric properties, formation history, and potential for habitability.
These discoveries bring us closer to answering fundamental questions about the diversity of planetary systems.
JWST continues to refine its capabilities, with astronomers exploring new observation techniques to push the boundaries of what can be detected.
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