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Updated: Aug 15, 2026

Infrared Degenerate Four-wave Mixing with Upconversion Detection for Quantitative Gas Sensing
Published on: March 22, 2019
Infrared spectrum of the cool brown dwarf Gl 229B
B R Oppenheimer1, S R Kulkarni, K Matthews
1Palomar Observatory, California Institute of Technology, Pasadena 91125, USA.
Abstract:
Spectroscopic measurements of a cool brown dwarf, Gl 229B, reveal absorption features attributable to methane in the near infrared much like those of Jupiter. These features are not seen in any star. The presence of methane indicates that the surface temperature of Gl 229B is below 1000 kelvin. Features attributed to water vapor also indicate that Gl 229B is much cooler than any known star.
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