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Science 1 December 1995: Vol. 270. no. 5241, pp. 1478 - 1479 DOI: 10.1126/science.270.5241.1478
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Reports
Infrared Spectrum of the Cool Brown Dwarf Gl 229B
B. R. Oppenheimer,
S. R. Kulkarni (1),
K. Matthews,
T. Nakajima
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.
Palomar Observatory 105-24, California Institute of Technology,
Pasadena, CA 91125, USA.
(1) To whom correspondence should be addressed.
THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
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282, 1095-1097
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- Brown Dwarfs: A Possible Missing Link Between Stars and Planets.
- S. R. Kulkarni (1997)
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276, 1350-1354
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