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Red dwarfs
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Red dwarfs

Red dwarfs are tiny, cool stars making up over 70% of our galaxy. If the Sun were a bright high-beam headlight, a red dwarf would be like a dim candle with a temperature around 3,000 K. They have only 8–50% of the Sun's mass, but through full convection, they mix fuel like a giant cauldron and burn hydrogen extremely slowly.

While the Sun will die in billions of years, these "space marathoners" can shine for trillions of years. They are often orbited by planets, but due to low luminosity, these worlds must be much closer than Earth is to the Sun to stay warm, exposing them to intense flares.
  • Percentage of Red dwarfs within 98.5 light years: 70.79 % (6741 from 9522 stars)
  • Average mass of Red dwarfs: 7.5-50% solar mass
  • Average radius of Red dwarfs: 10-60% solar radius
  • Average temperature of Red dwarfs: 2400-3900 K

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Latest news from Red dwarfs

Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b
iconToday
iconStars | Exoplanets | Red dwarfs | Super-Earths | Planetary atmospheres | TESS
Image: Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b
TOI-2257 b represents a unique case in planetary science due to its 35-day orbital period and high eccentricity, which describes how much an orbit deviates from a perfect circle. Located in a sparsely populated region of planetary parameter space, it sits at a critical threshold where the combined effects of stellar radiation and tidal forces - gravitational stresses caused by the host star - begin to lose their influence over the planet. Simulations show that the planet remains near this transi...
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Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class
icon6. 10. 2026
iconStars | Exoplanets | Red dwarfs | James Webb Space Telescope | Planetary atmospheres | Ocean plane
Image: Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class
Analysis of sub-Neptune planets around Red dwarf stars using JWST data reveals a new category of hybrid worlds. These planets have atmospheric compositions that do not align with traditional gas dwarf or water world definitions. Study highlights include TOI-776 c....
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Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere
icon3. 10. 2026
iconStars | Exoplanets | Red dwarfs | James Webb Space Telescope | Planetary atmosphere
Image: Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere
Analysis of four transit observations of TRAPPIST-1 c shows the planet is likely airless. By using a new method to account for stellar activity, researchers ruled out thick carbon dioxide and nitrogen atmospheres for this rocky exoplanet....
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Cold sub-Neptune TOI-6981 b discovered orbiting near the water ice line
icon30. 9. 2026
iconStars | Exoplanets | TESS | Red dwarf
Image: Cold sub-Neptune TOI-6981 b discovered orbiting near the water ice line
TOI-6981 b is a cold sub-Neptune planet discovered orbiting its Red dwarf host star at the water ice line. With a temperature of 170 K and a 60.8-day orbit, it stands as a key target for future atmospheric studies using the James Webb Space Telescope....
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Temperate sub-Neptune planet orbiting the red dwarf star TOI-210 confirmed
icon29. 9. 2026
iconStars | Exoplanets | Red dwarfs | TESS
Image: Temperate sub-Neptune planet orbiting the red dwarf star TOI-210 confirmed
A temperate sub-Neptune planet, TOI-210 b, has been confirmed orbiting the red dwarf TOI-210. With 6.75 times Earth's mass, the planet is likely a water-rich world or a gas dwarf. Evidence also points to two additional planets in the system....
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