Enanas rojas | Stellar Catalog

	Mass	Distance
Gliese 190 L 737-9, LHS 203, HIC 23932, HIP 23932, LFT 391, LP 777-36, LTT 2179, NLTT 14559, 2MASS J05083500-1810178	M3.5 V	0 M☉	30.1 ly
Gliese 3325 LHS 1731, L 736-49, L 736-44, LP 776-46, LTT 2153, HIC 23512, HIP 23512, NLTT 14433, 2MASS J05032009-1722245	M3 V	0.29 M☉	30.1 ly
Gliese 3128 LHS 1326, LSPM J0202+1020, USNO-B1.0 1003-00018076, 2MASS J02021620+1020136, USNO 693, LP 469-67, NLTT 6802	M5.5 V	0 M☉	30.1 ly
Gliese 1103 Luyten 961-1, G 112-50, LFT 553, LP 603-1, LP 603-2, LHS 1951, LHS 1952, LTT 12077, NLTT 18546	M4.5V	0.1 M☉	30.2 ly
66 G. Centauri B HD 102365B, LHS 313, VB 5, NLTT 28513	M4 V	0 M☉	30.4 ly
2MASS J0011+5908 GAT 1367, Karmn J00115+591, LSPM J0011+5908, LSR J0011+5908, 2MASS J00113182+5908400, PM J00115+5908, TIC 452882423	M6.0V	-	30.4 ly
Gliese 84 HIP 9724, LHS 149, LTT 1092, G 272-148, BD-18 359	M2.5 V	0.4 M☉	30.4 ly
Ross 837 LHS 2830, Ci 20 824, GALEX 3870529557103646973, G 65-19, GJ 3817, Gliese 3817, LFT 1053, LTT 14082, 2MASS J13581392+1234438, NLTT 35837, TIC 387009593	M3.5V	-	30.5 ly
Gliese 3135 LHS 1339, CD-30 731, HIC 9786, HIP 9786, LFT 180, L 511-7, LTT 1101, NLTT 7002, 2MASS J02054859-3010361, GJ 3135	M2.5 V	0 M☉	30.6 ly
Wolf 1062 AST 1, ASCC 1159413, Ci 20 1136, G 22-18, Gliese 748, GJ 748, HIC 94349, HIP 94349, LFT 1455, LHS 472, LSPM J1912+0253, LTT 15619, 2MASS J19121455+0253111, NLTT 47511, TIC 228846172, TYC 467-4992-1	M3.5V	0.37 M☉	30.7 ly
Wolf 1062 B		0.17 M☉	30.7 ly
Gliese 367 GJ 367, CD-45 5378, LHS 2182, HIC 47780, HIP 47780, LFT 682, LPM 328, LTT 3579, NLTT 22506, 2MASS J09442986-4546351, TOI 731, TIC 34068865, WISEA J094429.37-454641.4	M1.0V	0.45 M☉	30.7 ly
Gliese 3192 C	M	0.16 M☉	30.7 ly
Gliese 357 TOI 562, L 678-39, LHS 2157, LFT 661, LPM 321, LP 788-6, LTT 3534, NLTT 22154, 2MASS J09360161-2139371, HIP 47103, HIC 47103, GJ 357	M2.5 V	0.36 M☉	30.8 ly
1RXS J115928.5-524717	M9Ve	-	30.9 ly
Gliese 226 LHS 215, G 222-11, HIC 29277, HIP 29277, LFT 445, LTT 11765, NLTT 15960, 2MASS J06101978+8206256, AC+82 1111	M2.5 V	0 M☉	30.9 ly
UCAC4 379-100760 Karmn J18057-143, 2MASS J18054470-1422425, PM J18057-1422, TIC 362144730	M5.5V	-	30.9 ly
Gliese 176 Ross 33, BD+18° 683, BD+18 683, HD 285968, HIP 21932, LHS 196, G 85-9, G 83-32, G 8-55, LFT 372, LTT 11495, 2MASS J04425581+1857285, NLTT 13785, MCC 107, GJ 176	M2 V	0.5 M☉	30.9 ly
Gliese 479 CD-51 6859, LHS 336, HIC 61629, HIP 61629, LFT 930, L 255-20, LPM 438, LTT 4806, NLTT 31327, 2MASS J12375231-5200055	M3 V	0.43 M☉	31 ly
Gliese 3512 LHS 252, G 234-45, LP 90-18, NLTT 20004, 2MASS J08412013+5929505, WISEA J084119.76+592937.0, GJ 3512	M5.70	0.12 M☉	31 ly

Nombre de la estrella

Mass

Distance

Gliese 190

L 737-9, LHS 203, HIC 23932, HIP 23932, LFT 391, LP 777-36, LTT 2179, NLTT 14559, 2MASS J05083500-1810178

M3.5 V

0 M☉

30.1 ly

Gliese 3325

LHS 1731, L 736-49, L 736-44, LP 776-46, LTT 2153, HIC 23512, HIP 23512, NLTT 14433, 2MASS J05032009-1722245

M3 V

0.29 M☉

30.1 ly

Gliese 3128

LHS 1326, LSPM J0202+1020, USNO-B1.0 1003-00018076, 2MASS J02021620+1020136, USNO 693, LP 469-67, NLTT 6802

M5.5 V

0 M☉

30.1 ly

Gliese 1103

Luyten 961-1, G 112-50, LFT 553, LP 603-1, LP 603-2, LHS 1951, LHS 1952, LTT 12077, NLTT 18546

M4.5V

0.1 M☉

30.2 ly

66 G. Centauri B

HD 102365B, LHS 313, VB 5, NLTT 28513

M4 V

0 M☉

30.4 ly

2MASS J0011+5908

GAT 1367, Karmn J00115+591, LSPM J0011+5908, LSR J0011+5908, 2MASS J00113182+5908400, PM J00115+5908, TIC 452882423

M6.0V

30.4 ly

Gliese 84

HIP 9724, LHS 149, LTT 1092, G 272-148, BD-18 359

M2.5 V

0.4 M☉

30.4 ly

Ross 837

LHS 2830, Ci 20 824, GALEX 3870529557103646973, G 65-19, GJ 3817, Gliese 3817, LFT 1053, LTT 14082, 2MASS J13581392+1234438, NLTT 35837, TIC 387009593

M3.5V

30.5 ly

Gliese 3135

LHS 1339, CD-30 731, HIC 9786, HIP 9786, LFT 180, L 511-7, LTT 1101, NLTT 7002, 2MASS J02054859-3010361, GJ 3135

M2.5 V

0 M☉

30.6 ly

Wolf 1062

AST 1, ASCC 1159413, Ci 20 1136, G 22-18, Gliese 748, GJ 748, HIC 94349, HIP 94349, LFT 1455, LHS 472, LSPM J1912+0253, LTT 15619, 2MASS J19121455+0253111, NLTT 47511, TIC 228846172, TYC 467-4992-1

M3.5V

0.37 M☉

30.7 ly

Wolf 1062 B

0.17 M☉

30.7 ly

Gliese 367

GJ 367, CD-45 5378, LHS 2182, HIC 47780, HIP 47780, LFT 682, LPM 328, LTT 3579, NLTT 22506, 2MASS J09442986-4546351, TOI 731, TIC 34068865, WISEA J094429.37-454641.4

M1.0V

0.45 M☉

30.7 ly

Gliese 3192 C

0.16 M☉

30.7 ly

Gliese 357

TOI 562, L 678-39, LHS 2157, LFT 661, LPM 321, LP 788-6, LTT 3534, NLTT 22154, 2MASS J09360161-2139371, HIP 47103, HIC 47103, GJ 357

M2.5 V

0.36 M☉

30.8 ly

1RXS J115928.5-524717

M9Ve

30.9 ly

Gliese 226

LHS 215, G 222-11, HIC 29277, HIP 29277, LFT 445, LTT 11765, NLTT 15960, 2MASS J06101978+8206256, AC+82 1111

M2.5 V

0 M☉

30.9 ly

UCAC4 379-100760

Karmn J18057-143, 2MASS J18054470-1422425, PM J18057-1422, TIC 362144730

M5.5V

30.9 ly

Gliese 176

Ross 33, BD+18° 683, BD+18 683, HD 285968, HIP 21932, LHS 196, G 85-9, G 83-32, G 8-55, LFT 372, LTT 11495, 2MASS J04425581+1857285, NLTT 13785, MCC 107, GJ 176

M2 V

0.5 M☉

30.9 ly

Gliese 479

CD-51 6859, LHS 336, HIC 61629, HIP 61629, LFT 930, L 255-20, LPM 438, LTT 4806, NLTT 31327, 2MASS J12375231-5200055

M3 V

0.43 M☉

31 ly

Gliese 3512

LHS 252, G 234-45, LP 90-18, NLTT 20004, 2MASS J08412013+5929505, WISEA J084119.76+592937.0, GJ 3512

M5.70

0.12 M☉

31 ly

Enanas rojas noticias

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A

Today

Estrellas | 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...

Read article

Ammonia and hydrogen may separate inside Uranus and Neptune

Today

Estrellas | 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....

Read article

Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

15. 10. 2026

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....

Read article

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.

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.

More about Estrellas

Random terms

Posición de la estrella Luminosidad Temperatura de la estrella Masa estelar Tamaño de la estrella Edad de las estrellas

TOI 431 106 ly		Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey today
L 115-21 41.9 ly		A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274) today
TOI-3686 841 ly		TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance today
HD 112485 5881 ly		Ensemble pulsational characteristics of eclipsing binaries containing β Cep stars observed by the TESS mission 19. 10. 2026
TOI-5322 1560 ly	+1	A Sample of Thick-Disk Stars Hosting Hot Jupiters 17. 10. 2026

Lista de Enanas rojas

Enanas rojas noticias

Research in Enanas rojas

Frequently Asked Questions about nearby stars

What is the nearest star?

What are the nearest stars to Earth?

What is the solar neighborhood?

How do astronomers measure distances to stars?

Are there any exoplanets orbiting the nearest stars?

Why are the nearest stars important for astronomy and physics?

StellarGuide: Estrellas