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Lista de Enanas rojas
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Estrellas 121-140
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Nombre de la estrella Mass Distance

Gliese 831
Wolf 922, HIC 106255, HIP 106255, LFT 163, LTT 8556, NLTT 51428, LHS 511, BB Cap, BLA 9, BB Capricornus
 M4.5 V 0.22 M☉ 24.3 ly

HU Delphini
HU Del, Gliese 791.2, CCDM J20298+0941AB, LHS 3556, G 144-8, G 24-16, AST 2, HU Del, 2E 4369, LTT 15983, JP11 5099, TIC 374416052, UBV 17774, USNO 78
 M4.5V 0.24 M☉ 24.4 ly

Gaia DR2 6702242043883732864
 - 24.6 ly

Gaia DR2 6702242043877655936
TIC 349898518, 2MASS J18180608-5124366
 - 24.6 ly

Gliese 3991
G 203-47, HIP 83945, USNO 752
 M3.5V 0.2 M☉ 24.8 ly

G 141-36
2MASS J18481752+0741210
 M5V 0.13 M☉ 24.8 ly

Gliese 514
Ross 490, LHS 352, BD+11 2576, G 63-34, LTT 13925, NLTT 34287, LFT 1012, HIP 65859, HIC 65859, MCC 143, 2MASS J13295979+1022376, TYC 895-317-1 , Gl 514
 M1Ve 0.51 M☉ 24.9 ly

Gliese 4053
LP 71-165, G 258-33, LHS 3376, PLX 4228.11, USNO 554
 M4.5VC 0.16 M☉ 24.9 ly

Gliese 4248
Luyten 499-56, L 499-56, LHS 3746, LP 983-71, LTT 8811
 M3V 0.2 M☉ 25 ly

Mu Cassiopeiae B
 M 0.17 M☉ 25 ly

Fomalhaut C
LP 876-10, Fomalhaut C, 2MASS J22480446-2422075, NLTT 54872, GSC 06964-01226
 M4V 0.18 M☉ 25 ly

Gliese 109
Ross 556, V VX Ari, VX Arietis, V* VX Ari, HIC 12781, HIP 12781, Ci 20 180, Ci 20 180, LHS 1439, LTT 10897
 M3V 0.3 M☉ 25.1 ly

AN Sextantis
Gliese 382, HIP 49986, HIC 49986, G 162-25, G 53-29, LTT 3734, V* AN Sex, BD-03 2870, NLTT 23680, MCC 569, 2MASS J10121768-0344441
 M2 V 0.56 M☉ 25.1 ly

SIPS J1259-4336
2MASS J12590470-4336243, TIC 248223026, WISEA J125905.84-433627.2
 M8: - 25.2 ly

Gliese 2005
LHS 1070, LP 881-64, LEI 1, 2MASS J00244419-2708242
 M6V 0.15 M☉ 25.2 ly

Gliese 2005 B
 M8.5Ve 0.08 M☉ 25.2 ly

Gliese 2005 C
 M9.2V 0.07 M☉ 25.2 ly

Gliese 2005 D
 MV 0.09 M☉ 25.2 ly

Gliese 3378
Luyten 1813-21, G 192-13, LHS 1805, GJ 3378
 M3.5V 0.26 M☉ 25.2 ly

Gliese 701
Luyten 991-14, LHS 3356, HD 165222, LFT 1389, HIP 88574, G 21-1, G 20-22, NLTT 45883, MCC 176, 2MASS J18050755-0301523, LTT 7180
 M2 V 0.49 M☉ 25.2 ly
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Enanas rojas noticias

Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b
icon15. 10. 2026
iconEstrellas | Exoplanetas | Enanas rojas | Supertierras | Atmósferas planetarias | 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
iconEstrellas | Exoplanetas | Enanas rojas | Telescopio espacial James Webb | Atmósferas planetarias | Planetas océano
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
iconEstrellas | Exoplanetas | Enanas rojas | Telescopio espacial James Webb | Atmósferas planetari
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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study iconResearch in Enanas rojas

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Explore los últimos estudios científicos sobre estrellas y exoplanetas en nuestra galaxia. Descubra las últimas investigaciones sobre astrofísica y astronomía estelar.
La investigación actual

 WISE 0855-0714
7.3 ly
 study icon Water Cloud and Chemical Modulations in the Coldest Brown Dwarf
17. 10. 2026

WASP 94
687 ly
 study icon A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum
16. 10. 2026

KELT-2
439 ly
 study icon Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity
15. 10. 2026

TOI-2257
189 ly
 study icon The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b
15. 10. 2026

KELT-18
1032 ly
 study icon High-resolution transmission spectroscopy of KELT-18b Metastable helium detection at 1083 nm
14. 10. 2026
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Publicaciones más antiguas

Frequently Asked Questions about nearby stars

What is the nearest star?

Nearest star is Proxima Centauri, located approximately 4.24 light-years (1.30 parsecs) from the Sun. It is part of the Alpha Centauri star system, which also includes Alpha Centauri A and Alpha Centauri B.

What are the nearest stars to Earth?

Nearest stars to Earth include the Alpha Centauri system (Alpha Centauri A, Alpha Centauri B, and Proxima Centauri), Barnard's Star, and Wolf 359. There are also brown dwarfs Luhman 16 and WISE 0855−0714.

What is the solar neighborhood?

Solar neighborhood (also Local Interstellar Cloud) is the region of interstellar space that surrounds the Sun with diameter about 15 light years. Stellar Catalog database includes all stars contained within this region.

How do astronomers measure distances to stars?

Astronomers use methods like parallax, standard candles, and redshift to measure distances to stars. Parallax is especially useful for nearby stars in our solar neighborhood, while other techniques help map the universe beyond.

Are there any exoplanets orbiting the nearest stars?

Yes, several exoplanets have been discovered orbiting the nearest stars. For example, Proxima Centauri has an exoplanet called Proxima Centauri b, which is located in the star's habitable zone and is the closest known exoplanet to Earth.

Why are the nearest stars important for astronomy and physics?

The nearest stars provide valuable laboratories for studying stellar evolution, space environments, and the fundamental physics of stars. Observing these stars helps astronomers understand the structure of our galaxy and the broader universe.
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exoplanet iconStellarGuide: Estrellas

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Estrellas
Las estrellas son enormes esferas de gas caliente que brillan al generar energía mediante fusión nuclear en sus núcleos. La mayoría de las estrellas están compuestas principalmente de hidrógeno y helio. En el centro de una estrella, la alta presión y temperatura hacen que los átomos de hidrógeno se fusionen en helio, liberando una enorme cantidad de energía en forma de luz y calor.
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Posición de la estrellaLuminosidadTemperatura de la estrellaMasa estelarTamaño de la estrellaEdad de las estrellas

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