Teide 1, found in the Pleiades cluster, was confirmed in 1995 as the first bona fide brown dwarf — a substellar object with a mass below the roughly 0.08 solar-mass threshold needed to sustain ordinary hydrogen fusion, resolving a decade of unconfirmed brown-dwarf candidates. It was identified using the Spanish Nordic Optical Telescope.
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Teide 1, found in the Pleiades cluster, was confirmed in 1995 as the first bona fide brown dwarf — a substellar object with a mass below the roughly 0.08 solar-mass threshold needed to sustain ordinary hydrogen fusion, resolving a decade of unconfirmed brown-dwarf candidates. It was identified using the Spanish Nordic Optical Telescope.
The year a substellar object was first confirmed to be a genuine brown dwarf (too massive to be a planet, too low-mass to sustain hydrogen fusion).
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Permanent ID limitsregistry.com/limits/LR-FIRST-CONFIRMED-BROWN-DWARF
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Limits Registry. LR-FIRST-CONFIRMED-BROWN-DWARF. First confirmed brown dwarf. 2026.