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Enanas rojas
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Enanas rojas

Las enanas rojas son estrellas pequeñas y frías que representan más del 70% de nuestra galaxia. Si el Sol fuera un faro brillante, una enana roja sería como una vela tenue con una temperatura de unos 3.000 K. Tienen solo el 8-50% de la masa del Sol, pero mediante convección total, mezclan su combustible como en un gran caldero y queman hidrógeno muy lentamente. 

Mientras que el Sol morirá en miles de millones de años, estos "maratonistas espaciales" pueden brillar durante billones de años. Suelen tener planetas, pero debido a su bajo brillo, estos mundos deben estar mucho más cerca que la Tierra del Sol para no congelarse, exponiéndolos a fuertes erupciones.
  • Percentage of Enanas rojas within 97.4 años luz: 71.92 % (6612 from 9194 stars)
  • Average masa of Enanas rojas: 7.5-50% solar mass
  • Average radius of Enanas rojas: 10-60% solar radius
  • Average temperatura of Enanas rojas: 2400-3900 K

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Aligned orbits found in double M dwarf system and trends across planets, brown dwarfs, and binaries
icon12. 4. 2026
iconEstrellas | Exoplanetas | Enanas roj
Image: Aligned orbits found in double M dwarf system and trends across planets, brown dwarfs, and binaries
A new study has measured the alignment between the spin of an M dwarf star and the orbit of its very-low-mass stellar companion, marking the first such measurement for a double M dwarf system. Using the Rossiter-McLaughlin effect, researchers found that the two stars are well aligned, meaning the companion orbits in the same direction as the primary star spins. This suggests the system either formed aligned or was later realigned by tidal forces. The study also compared the alignment, or obli...
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The newly discovered Earth-like exoplanet TOI-4552 b has a year that lasts only 8 hours
icon21. 3. 2026
iconEstrellas | Exoplanetas | TESS | Enanas roj
Image: The newly discovered Earth-like exoplanet TOI-4552 b has a year that lasts only 8 hours
TOI-4552 b, a dense Earth-sized planet with a 0.3-day orbit around a quiet red dwarf, is confirmed and stands out as a top target for JWST studies....
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JWST reveals a low-metallicity atmosphere for giant planet TOI-5293 A b around a variable red dwarf
icon18. 3. 2026
iconEstrellas | Exoplanetas | Telescopio espacial James Webb | Atmósferas planetarias | Enanas roj
Image: JWST reveals a low-metallicity atmosphere for giant planet TOI-5293 A b around a variable red dwarf
JWST reveals TOI-5293 A b’s low-metallicity atmosphere and inflated radius, highlighting the challenges of studying planets around variable red dwarfs....
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TOI-672 b is confirmed as a hot super-Neptune, shedding light on the Neptunian desert around red dwarfs
icon16. 3. 2026
iconEstrellas | Exoplanetas | TESS | Enanas roj
Image: TOI-672 b is confirmed as a hot super-Neptune, shedding light on the Neptunian desert around red dwarfs
TOI-672 b, a hot super-Neptune orbiting a red dwarf, is confirmed and helps refine our understanding of the Neptunian desert’s boundaries around different stars....
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Earth-sized planet found orbiting a nearby red dwarf LP 466-156 (TOI-4616)
icon12. 3. 2026
iconEstrellas | Exoplanetas | TESS | Enanas roj
Image: Earth-sized planet found orbiting a nearby red dwarf LP 466-156 (TOI-4616)
TOI-4616 b, an Earth-sized planet orbiting a nearby red dwarf, has been confirmed and offers a valuable target for studying rocky worlds and their atmospheres....
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