Gliese 229B: the first confirmed brown dwarf (1995)
A Caltech team using Palomar Observatory imaged a faint companion beside the star Gliese 229. Its spectrum showed methane absorption, a sign of a cool atmosphere, confirming it as an object too small to fuse hydrogen in its core.
Gliese 229B became the first directly confirmed brown dwarf, validating a theoretical class of objects.
It established brown dwarfs as a distinct population bridging planets and stars, and made them accessible targets for atmospheric study.
It launched the field this study continues: using brown dwarfs as laboratories for giant-planet atmospheric physics that are bright enough to observe directly.
