Astronomy & Space

SPHEREx discovers brown dwarfs with water and methane in their atmospheres

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NASA's SPHEREx space telescope has detected atmospheric water and methane in brown dwarfs, celestial objects that exist between stars and planets in terms of mass and characteristics. The research, published in The Astrophysical Journal, reveals that these dim objects possess chemically complex atmospheres similar to gas giant planets in our solar system. This discovery provides new insights into the atmospheric composition of brown dwarfs, which have been difficult to study due to their faint emissions.


Understanding brown dwarf atmospheres helps bridge our knowledge between stellar and planetary science, potentially informing exoplanet atmospheric studies. The detection of water and methane signatures demonstrates SPHEREx's capability to characterize faint celestial objects, which may improve our ability to study similar chemical compositions in distant exoplanets.


NASA’s SPHEREx (Spectro-Photometer for the History of the universe, Epoch of Reionization, and ices Explorer) space telescope is shedding light on brown dwarfs, celestial objects that blur the line between stars and exoplanets. New findings published in The Astrophysical Journal show that these dark and cloudy worlds have chemically rich atmospheres not unlike the giant planets in our own solar system.

Source: SPHEREx spots menagerie of brown dwarfs with atmospheric water and methane