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 …
- Jupiter-mass 'exomoon' orbiting brown dwarf...on July 22, 2026 at 3:00 pm
Observations made with the European Southern Observatory's Very Large Telescope (ESO's VLT) have revealed evidence for a moon-like object in the CD-35 2722 system. Unlike moons in our solar system, the newly found object does not orbit a planet, raising questions about what to name it. Instead, it circles a brown dwarf, an object larger than a planet, that orbits the CD-35 2722 star. If confirmed, this could be the first "moon" discovered outside our solar system.
- Webb telescope discovers hidden planet in famous...on July 16, 2026 at 2:40 pm
Astronomers using NASA's James Webb Space Telescope have discovered a giant planet outside our solar system, called an exoplanet, hiding within one of the most intensely studied planetary systems in the Milky Way galaxy.
- Astronomers characterize 'improbable' system...on July 6, 2026 at 4:00 pm
In the course of studying planets beyond our solar system (6,316 confirmed exoplanets and counting), scientists have discovered some very interesting systems. Consider TOI-201, a compact system populated by three bodies, including a brown dwarf, orbiting on the same plane. The system was recently observed by an international team led by the European Southern Observatory (ESO) and the National Institute for Astrophysics (INAF) using data from NASA's Transiting Exoplanet Survey Satellite (TESS).
- What makes a star a star? A strange...on July 2, 2026 at 4:40 pm
A star called TOI-2155 lies around 1,350 light-years (839 trillion miles) from Earth. It is a little bigger, heavier and hotter than the sun, and it is not particularly interesting or unusual in itself.
- Euclid captures 60 million stars in sharpest...on June 24, 2026 at 4:40 pm
For just one day, our dark universe detective, Euclid, turned its gaze toward the light: the extremely bright inner region of our Milky Way galaxy, known as the galactic bulge. This special request came from astronomers who were after what Euclid does best: capturing huge areas of the sky in crisp detail.
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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.





