Brown Dwarf

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Introduction1

Astronomic (YouTube Channel)
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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)

MERLOT: Multimedia Educational Resource for Learning and Online Teaching
OER Commons: Open Educational Resources

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 …

  • The largest survey of exoplanet spins confirms a...
    on April 5, 2026 at 3:00 pm

    For some time, astronomers have theorized that there is a connection between planetary mass and rotation. In the solar system, Jupiter and Saturn both rotate rapidly, completing a rotation in roughly ten hours, while accounting for a significant fraction of the solar system's rotational energy. Using the W.M. Keck Observatory on Maunakea, Hawai'i, a team of astronomers tested this predicted relationship by studying 32 gas giants and brown dwarfs in distant star systems—6 giant planets larger […]

  • ZTF discovers a new mass-transferring brown dwarf...
    on March 29, 2026 at 7:00 pm

    Astronomers from the California Institute of Technology (Caltech) and elsewhere report the discovery of a binary system consisting of two brown dwarfs undergoing stable mass transfer. The detection of the system, designated ZTF J1239+8347, was made with the Zwicky Transient Facility (ZTF) and is detailed in a paper published March 18 in The Astrophysical Journal Letters.

  • Saturday Citations: Merging brown dwarfs, ancient...
    on March 21, 2026 at 12:30 pm

    This week, among a lot of other important findings, we learned that emperor cichlid fish have gaze sensitivity and dislike it if you look at them—or especially their children. England is looking for a solution to its 5-billion-liter water deficit. And a high-fiber diet isn't only healthy for you—it also benefits your parasitic tapeworms!

  • How two dim stars came together to shine brightly
    on March 18, 2026 at 7:40 pm

    Brown dwarfs get a bad rap in the stellar world, often labeled as "failed stars" for their inability to sustain nuclear fusion at their cores. The mass of these objects falls between planets and stars, ranging from 13 to 80 times the mass of Jupiter. Because they aren't massive enough to sustain fusion, they are far fainter and cooler than their stellar comrades.

  • Clearest evidence yet that giant planets spin...
    on March 18, 2026 at 2:00 pm

    For decades, astronomers have struggled to differentiate giant planets from brown dwarfs, a class of objects more massive than planets but too small to ignite nuclear fusion like true stars. Through a telescope, these cosmic lookalikes can have overlapping brightness, temperatures, and even atmospheric fingerprints. The striking similarity leaves astronomers unsure if they have observed an oversized planet or an undersized star. Now, a Northwestern University-led team has uncovered a crucial […]

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Related

Here are links to pages about closely related subjects.

Knowledge Realm

Physical

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Planetary System Star, Brown Dwarf, Planet, Moon

Our Neighborhood
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Terrestrial Planet Mercury, Venus, Earth (Moon), Mars
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Trans-Neptunian Object
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Scattered Disc Eris, Sedna, Planet X
Oort Cloud Etc. Scholz’s Star
Small Body Comet, Centaur, Asteroid

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Notes

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