Page 3: Research news on Brown dwarfs

Brown dwarf research is a subfield of astrophysics focused on objects with masses between the heaviest gas giant planets and the lightest stars, insufficient to sustain stable hydrogen fusion. This research area investigates their formation pathways, atmospheric chemistry and dynamics, internal structure, cooling and evolutionary tracks, and spectral classification (e.g., L, T, and Y types). It leverages multiwavelength observations, high-resolution spectroscopy, and theoretical modeling to constrain substellar mass functions, metallicities, cloud physics, and magnetic activity, and to calibrate brown dwarfs as analogs for exoplanet atmospheres and as benchmarks for testing low-temperature equation-of-state and radiative-transfer models.

Ancient brown dwarf reveals cloud chemistry secrets

Deep in space, an ancient brown dwarf nicknamed "The Accident" has revealed the first-ever detection of a molecule that scientists have been searching for in planetary atmospheres for decades.

Methane detected in the atmosphere of the nearest T dwarf

Using the 10.4-m Gran Telescopio Canarias (GTC), European astronomers have detected methane in the atmosphere of WISEA J181006.18−101000.5—the closest T dwarf to Earth. The finding was reported in a research paper published ...

Two new brown dwarfs discovered with TESS

An international team of astronomers reports the detection of two new brown dwarfs orbiting distant stars using NASA's Transiting Exoplanet Survey Satellite (TESS). The newfound objects are about 30 times more massive than ...

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