Cosma / Communication / Knowledge / Realm / Physical / Universe / Planetary System / Brown Dwarf
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Introduction1
Astronomic (YouTube Channel)
Astronomic (Facebook)
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)
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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 …
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Studying exoplanets has given astronomers insights into the characteristics that could help them find life beyond Earth. For years, astronomers thought an exoplanet's location in a star's habitable zone was enough to make it an Earth-like world. But some stars are more active than our sun, exposing planets in their habitable zones to far more radiation than Earth receives. Astronomers have increasingly recognized that a planet's magnetic field, which shields Earth from harmful radiation, could […]
- A world 20 light-years away reveals surprisingly...on September 16, 2026 at 7:00 am
Scientists from Trinity College Dublin have developed a way to unravel changing weather patterns on distant worlds. Using this approach, they discovered that the weather on a well-studied brown dwarf, SIMP 0136, previously linked to northern lights-like phenomena, is largely shaped by just two dominant processes: changes in temperature and the vertical structure of its clouds.
- Webb reveals dynamic panorama of star formation,...on September 15, 2026 at 9:20 pm
This starry view of the nearby star-forming region IC 348 is one of the largest images released to date from NASA's James Webb Space Telescope. Using Webb, astronomers searched IC 348 for brown dwarfs, which are less massive than the smallest stars. The researchers discovered brown dwarfs just twice the mass of Jupiter, bringing the study of these curious objects into a new mass range and revealing new insights about the star-formation process.
- 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.
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Related
Here are links to pages about closely related subjects.
“Fundamentals”
Law (Constant) Relativity
Force Gravity, Electromagnetism (Light, Color)
Matter (Microscope) Molecule, Atom (Periodic Table), Particle
“Space”
Universe (Astronomical Instrument)
Galaxy Milky Way, Andromeda
Planetary System Star, Brown Dwarf, Planet, Moon
Our Neighborhood
Solar System Sun
Terrestrial Planet Mercury, Venus, Earth (Moon), Mars
Asteroid Belt Ceres, Vesta
Jovian Planet Jupiter, Saturn, Uranus, Neptune
Trans-Neptunian Object
Kuiper Belt Pluto, Haumea, Makemake
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.





