Brown Dwarf

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Introduction1

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Encyclopedia

Brown dwarfs are substellar objects that are not massive enough to sustain nuclear fusion of ordinary hydrogen (1H) into helium in their cores, unlike a main-sequence star. Instead, they have a mass between the most massive gas giant planets and the least massive stars, approximately 13 to 80 times that of Jupiter (MJ). However, they can fuse deuterium (2H), and the most massive ones (> 65 MJ) can fuse lithium (7Li). Astronomers classify self-luminous objects by spectral class, a distinction intimately tied to the surface temperature, and brown dwarfs occupy types M, L, T, and Y. As brown dwarfs do not undergo stable hydrogen fusion, they cool down over time, progressively passing through later spectral types as they age. Despite their name, to the naked eye, brown dwarfs would appear in different colors depending on their temperature. The warmest ones are possibly orange or red, while cooler brown dwarfs would likely appear magenta to the human eye. Brown dwarfs may be fully convective, with no layers or chemical differentiation by depth. — Wikipedia

Brown Dwarf (Encyclopædia Britannica)

Brown Dwarf (COSMOS: The SAO Encyclopedia of Astronomy)

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Innovation

Science

NASASpaceNews (YouTube Channel)

Brown Dwarfs: Space’s Strangely Important Oddballs (SciShow Space, YouTube Video)

What is a Brown Dwarf? (JPL/NASA)

Brown Dwarf (Wolfram Alpha)

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Preservation

History

The objects now called “brown dwarfs” were theorized by Shiv S. Kumar in the 1960s to exist and were originally called black dwarfs, a classification for dark substellar objects floating freely in space that were not massive enough to sustain hydrogen fusion. However, (a) the term black dwarf was already in use to refer to a cold white dwarf; (b) red dwarfs fuse hydrogen; and (c) these objects may be luminous at visible wavelengths early in their lives. Because of this, alternative names for these objects were proposed, including planetar and substar. In 1975, Jill Tarter suggested the term “brown dwarf”, using “brown” as an approximate color. — Wikipedia

Library

DDC: 523.88 Brown Dwarf Stars (Library Thing)
Subject: Brown Dwarf Stars (Library Thing)

Subject: Brown Dwarf Stars (Open Library)

LCC: QB 843.B77 Brown Dwarf Stars (Library of Congress)
Subject: Brown Dwarf Stars (Library of Congress)

Subject: Brown Dwarf Stars (WorldCat)

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Participation

Education

Brown Dwarfs (Crash Course Astronomy, YouTube Video)

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Community

News

Brown Dwarfs (Nova Research Highlights, American Astronomical Society)
Brown Dwarf (Astronomy Magazine)
Brown Dwarf (JSTOR)
Brown Dwarf (Phys.org)


Recent News from Phys.org …

  • TESS discovers a rare brown dwarf orbiting a...
    on August 13, 2026 at 9:00 pm

    For decades, astronomers lumped brown dwarfs into a single category defined by mass alone—too big to be classified as planets but too small to become stars. However, this definition ignores the two very different mechanisms that can form them: the direct collapse of gas clouds and formation within the accretion disks of massive stars.

  • Charting the galaxy: Milky Way Mapper survey...
    on August 6, 2026 at 10:30 pm

    The Sloan Digital Sky Survey V (SDSS-V) has announced its 20th public data release (DR20), delivering a dramatic expansion of the Milky Way Mapper (MWM) scientific survey—the most detailed spectroscopic map yet assembled of stars in and around our home galaxy.

  • Spacecraft observations may conceal how particles...
    on August 6, 2026 at 1:20 pm

    High-energy particles in Earth's radiation belt can appear to spread out randomly, even when they are moving in a "predictable" way. This is because spacecraft observations naturally blur the fine-scale structure of the particle population, a new study reveals.

  • A 21-hour dip could help explain Tabby's star's...
    on August 3, 2026 at 12:00 pm

    Since 2016, an ordinary-looking F-type star called KIC 8462852, nicknamed Tabby's star, has behaved anything but ordinarily. In a new study published in the Monthly Notices of the Royal Astronomical Society on July 6, researchers revisited this star to find out what is really causing its irregular dimming.

  • Tabby's star may be orbited by a planetary-mass...
    on July 28, 2026 at 2:00 pm

    By analyzing data from NASA's Transiting Exoplanet Survey Satellite (TESS) and conducting new radial velocity measurements, U.K. and French astronomers have found evidence that the mysterious Tabby's star may be orbited by an object about nine times more massive than Jupiter. The new findings are published on the preprint server arXiv.

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Related

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Notes

1.   The resources on this page are are organized by a classification scheme developed exclusively for Cosma.