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brown dwarf
(redirected from Brown dwarf star)

   Also found in: Encyclopedia, Wikipedia 0.01 sec.
brown dwarf
n.
A celestial body with insufficient mass to sustain the nuclear fusion that produces radiant energy in normal stars, believed to have formed with enough mass to start nuclear fusion in its core, but without enough for the fusion to become self-sustaining.

brown dwarf
n
(Astronomy) a type of celestial body midway in mass between a large planet and a small star

brown dwarf
A celestial body with insufficient mass to sustain the nuclear fusion that produces radiant energy in normal stars. It is believed that a brown dwarf is formed with enough mass to start nuclear fusion in its core, but without enough for the fusion to become self-sustaining. Theory suggests that a body with about one percent of the mass of the Sunor ten times the mass of Jupitercan generate this initial fusion, but that it needs at least eight percent of the Sun's mass to sustain the fusion. After the fusion ends, the dwarf still glows for a period from radiating heat, with a surface temperature of about 2,500°K (4,532°F) or less. See Note at dwarf star.


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Alan Boss, an exoplanet expert at the Carnegie Institution of Washington, and Lisa Kaltenegger, a Harvard exoplanet hunter, both said more study was needed to confirm the new set of photos were those of proven planets and not just brown dwarf stars.
who improved on methods of assessing the age of brown dwarf stars from their near-infrared spectra.
JSA Scattered among the galaxy are brown dwarf stars, capable of producing energy to heat colonizing stations and power starships.
 
 
 
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