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Lista de Enanas rojas

        
    
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Estrellas 281-300
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Nombre de la estrella Mass Distance

Gliese 609
LHS 411, G 168-25, GJ 609, G 137-78, LFT 1243, L 1346-53, L 1345-70, LTT 14773, TIC 229575381, USNO 55, 2MASS J16025098+2035218
M4V - 32.7 ly

G 195-59
LHS 2232, LFT 697, L 1761-5, LP 92-48, 2MASS J10123481+5703495, NLTT 23649, TIC 137958028, WISEA J101234.33+570343.5
M3.5Ve - 32.8 ly

APMPM J0237-5928
2MASS J02363244-5928057, TIC 201878287, WISEA J023633.27-592800.6, RAVE J023632.5-592806
M4.5V - 32.8 ly

Gliese 1134
LHS 287, G 146-58, GJ 1134, LFT 732, L 1545-14, LP 263-15, LTT 12850, 2MASS J10413809+3736397, NLTT 25073, TIC 17299996, WISEA J104136.57+373635.2
M4.0Ve - 32.8 ly

L 480-69
GJ 590, Gliese 590, LHS 3092, DENIS J153634.5-375422, LFT 1212, LTT 6228, 2MASS J15363450-3754223, NLTT 40644, TIC 172278724, WISEA J153634.19-375431.1
M5e - 32.9 ly

Gliese 1119
G 115-42, GJ 1119, LFT 626, LHS 2092, L 1684-5, LP 165-10, LTT 12354, NLTT 20711, 2MASS J09003254+4635117, TIC 29168887, USNO 430
M4.5V - 32.9 ly

HD 223889
L 26-27, CD-76 1182, DENIS J235349.8-753756, HIC 117828, HIP 117828, LTT 9759, 2MASS J23535017-7537575, NLTT 58294, TIC 402104884, TYC 9477-617-1, WISEA J235350.77-753800.5
M3 - 33 ly

Gliese 678.1
BD+05 3409, G 139-43, WOR 25, GJ 9592, HIC 85665, HIP 85665, LTT 15197, NLTT 44915, MCC 321, 2MASS J17302272+0532547, Wolf 751
M1 Ve 0 M☉ 33 ly

G 97-15
GJ 3326, Gliese 3326, LTT 17736, 2MASS J05041476+1103238, NLTT 14445, TIC 415508270, WISEA J050414.71+110325.9
M5V - 33.2 ly

Gliese 660
GJ 660, G 19-15, LPM 629, HIC 84123, HIP 84123, LFT 1324, LHS 3269, L 989-20, LPM 629, LP 627-9, LTT 6854, NLTT 44323, 2MASS J17115234-0151057, TIC 142948307, TYC 5065-23-1, WISEA J171152.00-015108.8
M3V - 33.2 ly

Gliese 660 B
- 33.2 ly

Gliese 487
G 237-78, GJ 487, DEL 4, AC +66 3955, HIC 62556, HIP 62556, JP11 5150, LSPM J1249+6606, LTT 13665, NLTT 32013, 2MASS J12490273+6606366, TIC 341687654, TYC 4168-824-1, V* DP Dra, WISEA J124902.00+660635.8, Gaia DR2 1677568527365572224
M3V - 33.3 ly

Gliese 203
HIP 25578, Ross 41, GJ 203, LHS 1761, LFT 411, G 102-3, G 97-42, LTT 11651, NLTT 15107, 2MASS J05280015+0938382
M3.5Ve 0.22 M☉ 33.3 ly

Gaia EDR3 5264749303457104384
Alpha Mensae B
- 33.3 ly

UCAC4 175-092532
2MASS J12455254-5506502, SCR J1245-5506, TIC 419692115, WISEA J124552.96-550651.6
M5e - 33.3 ly

Gliese 1265
GJ 1265, L 788-37, LHS 3776, LFT 1695, LP 819-52, LTT 8915, 2MASS J22134277-1741081, NLTT 53236, WISEA J221343.49-174111.9
dM4.5 C 0.18 M☉ 33.4 ly

Gliese 3049
LHS 1134, LFT 69, 2MASS J00432603-4117337, L 363-38, LTT 400, LP 989-140, NLTT 2382, GJ 3049
M5 0.21 M☉ 33.4 ly

L 273-106
LHS 5341, LFT 1428, L 273-106, LTT 7416, NLTT 46865, 2MASS J18430697-5436481, TIC 120395704, WISEA J184306.81-543653.4
M5 - 33.4 ly

Gliese 1083
G 100-28, GJ 1083, WNO 45, LTT 17846, NLTT 15441, TIC 75326630, V* V780 Tau, 2MASS J05402570+2448090, USNO 307, WISEA J054025.79+244804.2
M7V - 33.4 ly

2MASS J0419+4233
2MASS J04195212+4233304, TIC 347994537, WISEA J041952.62+423315.4, LSPM J0419+4233, LSR J0419+4233
M8/9V - 33.5 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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