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Brown dwarf - Wikipedia
Brown dwarfs are substellar objects that have more mass than the biggest gas giant planets, but less than the least massive main-sequence stars. Their mass is approximately 13 to 80 times that of Jupiter (MJ) —not big enough to sustain nuclear fusion of ordinary hydrogen ( H) into helium in their cores, but … See more
Early theorizing
The objects now called "brown dwarfs" were theorized by Shiv S. Kumar in the 1960s to exist and were originally called black dwarfs, … See moreClassification of brown dwarfs
Spectral class M
These are brown dwarfs with a spectral class of M5.5 or … See moreThe earliest stage of brown dwarf formation is called proto- or pre-brown dwarf. Proto-brown dwarfs are low-mass equivalents of protostars (class 0/I objects). Additionally Very Low Luminosity Objects (VeLLOs) that have Lint ≤0.1-0.2 L☉ are … See more
The standard mechanism for star birth is through the gravitational collapse of a cold interstellar cloud of gas and dust. As the cloud contracts, it … See more
Brown dwarf–brown dwarf binaries
Brown dwarfs binaries of type M, L, and T are less common with a lower mass of the primary. L-dwarfs have a binary fraction of about 24+6 −2% and … See moreAccording to the IAU working definition (from August 2018) an exoplanet can orbit a brown dwarf. It requires a mass below 13 MJ and a mass ratio … See more
• Fusor (astronomy)
• Brown-dwarf desert – Theorized range of orbits around a star within which brown dwarfs cannot exist as companion objects
• Blue dwarf (red-dwarf stage) – Hypothetical class of star that develops from a red dwarf See moreWikipedia text under CC-BY-SA license - bing.com › videosWatch full videoWatch full video
Star Life and Death - National Radio Astronomy Observatory
Brown Dwarfs: Celestial Objects That Are Neither …
Sep 14, 1995 · Brown dwarfs are called “failed stars” because they do not reach the stage of thermonuclear fusion of hydrogen in their cores. Objects from stellar disks become true stars when they finally ignite by fusing hydrogen to helium …
Brown dwarf | Astronomy, Formation & Characteristics …
Dec 27, 2024 · brown dwarf, astronomical object that is intermediate between a planet and a star. Brown dwarfs usually have a mass less than 0.075 that of the Sun, or roughly 75 times that of Jupiter. (This maximum mass is a little higher …
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Brown dwarfs: The stars that 'fail' - Space.com
Dec 20, 2024 · Brown dwarfs are curious celestial bodies that appear to straddle the mass divide between stars and planets. Often referred to as "failed stars," brown dwarfs form in isolation from a...
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Brown Dwarf: Definition, Temperature, Size And Other …
Jun 2, 2024 · Brown dwarfs are sub-stellar objects that are something between stars and planets. They are formed like regular stars, but fail to gain enough mass to sustain a fusion reaction.
Life Cycle of a Star: Types of Stars by Life Cycle
Stars below 10 Mj (Mj-mass of Jupiter) are called sub-brown dwarfs and sometimes they are referred to as rogue planets. The main sequence stars create a nuclear fusion reaction of hydrogen atoms to helium atoms in its core and …
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A Brown Dwarf Prevented a Regular Star from Going Through its …
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