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Lista de Enanas rojas

        
    
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Estrellas 321-340
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Nombre de la estrella Mass Distance

Gliese 3119
G 159-3, G 271-166, LHS 1302, NLTT 6192, 2MASS J01510405-0607047
M4.5 Ve 0 M☉ 34.4 ly

LP 647-13
LP 647-013, NLTT 3868, 2MASS J01095117-0343264, TIC 248350761
M9 Ve 0 M☉ 34.5 ly

HD 209290
LHS 3745, DO 7683, G 18-16, G 27-5, G 26-44, G 93-66, GJ 846, Gliese 846, HIC 108782, HIP 108782, LFT 1678, LTT 16435, 2MASS J22021026+0124006, TIC 292987389, TYC 558-1540-1, WISEA J220209.96+012358.0, Wolf 1340
M0.5V - 34.5 ly

LP 775-31
CRC 47A, Karmn J04352-161, 2MASS J04351612-1606574, 2MUCD 10302, NLTT 13580, SIPS J0435-1607, TIC 117733581, WISE J043516.24-160653.9
M8Ve - 34.5 ly

Gliese 1235
LHS 476, G 185-18, GJ 1235, LFT 1471, L 1355-129, L 1355-12, LP 452-1, LTT 15660, 2MASS J19213867+2052028, NLTT 47717, TIC 385368233, UBV M 42690
M4.0Ve - 34.6 ly

G 68-8
LHS 543, GJ 4333, Gliese 4333, HIC 115332, HIP 115332, LFT 1785, L 1295-31, LP 462-27, 2MASS J23213752+1717284, LTT 16862, NLTT 56616, TIC 435198528, TYC 1713-313-1, WISEA J232137.05+171710.9
M3.5Ve 0.3 M☉ 34.6 ly

LP 860-41
LHS 5303, DENIS J155244.6-262313, 2MASS J15524460-2623134, NLTT 41379, TIC 23997017, WISEA J155244.77-262318.4
M6.0V - 34.6 ly

L 98-59
2MASS J08180763-6818468, NLTT 19357, TIC 307210830, TYC 9193-2365-1, WISEA J081807.80-681850.2, TOI-175, RAVE J081807.6-681847, Luyten 98-59
M3V C 0.32 M☉ 34.6 ly

G 107-48
G 107-48, GJ 3426, Gliese 3426, 2MASS J07073776+4841138, NLTT 17418, TIC 252947361, WISEA J070737.71+484110.3
M4.35 - 34.6 ly

LP 867-15
EPIC 215818496, 2MASS J18421107-2328582, NLTT 46868, TIC 3882477
M3.5 - 34.6 ly

G 22-26
M4V - 34.6 ly

G 261-6
LHS 3461, GJ 1238, Gliese 1238, LP 25-636, 2MASS J19241634+7533121, NLTT 47831, TIC 420130591, WISEA J192417.32+753318.0
M6V 0.13 M☉ 34.7 ly

Ross 165
GJ 766 A, Gliese 766, WDS J19458+2710A, KUI 95, KPR 95, HIC 97237, HIP 97237, LFT 1491, LHS 478, LTT 15768, NLTT 48208, 2MASS J19454548+2707318, TIC 451852919, TYC 2147-1374-1, WISEA J194545.48+270719.0
M4V - 34.7 ly

Ross 165B
M4V - 34.7 ly

HD 111631
G 14-6, G 60-41, GJ 488, Gliese 488, HIC 62687, HIP 62687, LTT 4913, 2MASS J12504357-0046047, MCC 675, NLTT 32069, TIC 53280272, TYC 4950-67-1, WISEA J125043.52-004609.2, YZ 90 3469
M0V - 34.8 ly

Gliese 4154
LHS 3583, GJ 4154, L 23-30, LFT 1559, LTT 8178, NLTT 49675, 2MASS J20463725-8143141, TIC 401667290, WISEA J204639.66-814319.2
M3e 0.38 M☉ 34.8 ly

TVLM 513-46
TVLM 513-46546, 2MASS J15010818+2250020, 2MASSI J1501081+225001, 2MUCD 20596, SDSS J150108.17+225001.8, TIC 311188315, WISEP J150108.17+225001.4
M8.5V C 0.09 M☉ 35 ly

Gliese 669
GJ 669 A, Gliese 669, G 170-35, HIC 84794, HIP 84794, LTT 15139, NLTT 44616, 2MASS J17195422+2630030, RBS 1637, SDSS J171954.30+262957.9, TIC 257798327, TYC 2082-2076-1, V* V647 Her, WISEA J171954.02+263006.7, Ross 868
M3.5V - 35.1 ly

Gliese 669 B
Ross 867, GJ 669 B, WISE J171952.80+263006.3, 2MASS J17195298+2630026
M4.5V - 35.1 ly

V* V857 Cen
GJ 431, Gliese 431, HIC 56244, HIP 56244, LFT 821, LHS 2423, L 396-7, LTT 4255, NLTT 27672, 2MASS J11314655-4102473, TIC 181015118, TYC 7744-1540-1, ISEA J113145.82-410245.2
M3.5 0.3 M☉ 35.1 ly
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Enanas rojas noticias

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A
iconToday
iconEstrellas | Exoplanetas | Enanas rojas | TESS
Image: Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A
A small planet candidate has been identified in the binary star system known as Gliese 774. The object, which is smaller than the Earth, orbits its host star approximately every 4.2 days. Observations from the Transiting Exoplanet Survey Satellite (TESS) captured the planet as it passed in front of its star, briefly blocking a tiny fraction of the starlight. This periodic dimming event allowed for the identification of the candidate despite the complex environment of a binary system, where two s...
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Ammonia and hydrogen may separate inside Uranus and Neptune
iconToday
iconEstrellas | Exoplanetas | Enanas roj
Image: Ammonia and hydrogen may separate inside Uranus and Neptune
Uranus and Neptune may be experiencing ammonia rain: simulations show their expected temperature profiles cross the boundary where ammonia and hydrogen separate. In warmer sub-Neptune TOI-270 d, the two are likely to mix in all proportions....
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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
The exoplanet TOI-2257 b orbits its star once every 35 days with a high eccentricity. New models suggest its atmospheric and orbital fate depends on whether it is a gas-rich mini-Neptune or a rocky super-Earth. Higher eccentricity would confirm a gaseous nature....
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study iconResearch in Enanas rojas

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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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