brown dwarf

American  

[broun dwawrf] / ˈbraʊn ˈdwɔrf /

noun

Astronomy.

1. a celestial object smaller than a small star but larger than a giant planet: believed to form as stars do, from collapsing clouds of gas and dust, brown dwarfs are sometimes called failed stars as they are not dense enough to initiate nuclear fusion, leaving them much dimmer and cooler than stars.

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brown dwarf British  

noun

1. a type of celestial body midway in mass between a large planet and a small star

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brown dwarf Scientific  

1. 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 Sun—or ten times the mass of Jupiter—can 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.

2. See Note at dwarf star

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Etymology

Origin of brown dwarf

First recorded in 1975–80

Example Sentences

It could be a giant planet, a brown dwarf, or an extremely low-mass star.

From Science Daily

With a mass similar to Saturn, the researchers suggest that it most likely formed within a planetary system rather than developing on its own like a small star or brown dwarf.

From Science Daily

Astronomers working with the Subaru Telescope in Hawaiʻi have identified two remarkable objects circling distant stars: a giant planet and a brown dwarf.

From Science Daily

The second object, HIP 71618 B, is a brown dwarf with a mass about 60 times that of Jupiter.

From Science Daily

Its host star is bright, the brown dwarf sits at an ideal position, and at the Roman Coronagraph's operating wavelengths it will appear faint enough relative to its star to properly evaluate the new technology.

From Science Daily