Enanas rojas | Stellar Catalog

	Mass	Distance
Mu Herculis C	M3.5 V	0.39 M☉	27.1 ly
Gliese 747 B	M3 V	-	27.1 ly
Gliese 747 G 207-16, KUI 90, LFT 1451, LHS 471, L 1499-28, LP 336-6, LTT 15603, NLTT 47437	M3 V	-	27.1 ly
Mu Herculis Ab	M4 V	0.32 M☉	27.2 ly
Mu Herculis B mu.02 Her	M3.5 V	0.44 M☉	27.2 ly
Gliese 1227 LHS 465, G 227-29, LP 103-305, NLTT 46427, 2MASS J18222719+6203025	M4 V	-	27.2 ly
Gliese 1289 G 130-4, LHS 4003, 2MASS J23430628+3632132, NLTT 57748, G 190-43, GJ 1289, TIC 352593978, WISEA J234307.14+363211.5	M4.5 V	0.21 M☉	27.3 ly
2MASS J18352–3123 2MASS J18352154–3123385, 1RXS J183520.9−312327	M6.5V	0 M☉	27.3 ly
2MASS J18352–3123 B 2MASS J18352205−3123421	M8 V	-	27.3 ly
SCR 1138-7721 2MASS J11381671-7721484, WISEA J113810.11-772142.2, SCR J1138-7721	M5 V	0.18 M☉	27.3 ly
2MASS J1546-5534 2MASS J15464185-5534468, DENIS J154641.8-553446, SCR J1546-5534, WISEA J154640.78-553446.0	M7.5	0.2 M☉	27.4 ly
Gliese 185 B		0.37 M☉	27.4 ly
TYC 3980-1081-1 IRAS 21500+5903, 2MASS J21513828+5917383	M3.9	0.2 M☉	27.6 ly
Gliese 232 Ross 64, JP11 5117, LHS 1846, LFT 467, G 104-37, LTT 11838, Ci 20 385	M4 V	0 M☉	27.7 ly
Gliese 618 B LHS 416, LFT 1267, L 482-31, LTT 6509	M5	0 M☉	27.7 ly
Gliese 618 CD-37 10765, LHS 415, LDS 6312, L 482-30, LFT 1266, LTT 6508, NLTT 42493, 2MASS J16200353-3731449, TYC 7853-670-1	M3 V	-	27.8 ly
Gliese 493.1 Wolf 461, V* FN Vir, G 60-55, G 62-5, LFT 962, LHS 2664, LTT 13750, NLTT 32583, 2MASS J13003350+0541081	M4.5 Ve	0 M☉	27.9 ly
Gliese 3454 LTT 17993, G 89-32, Nl 654, HEN 3, 2MASS J07362513+0704431, NLTT 18152	M4.5 V	0.15 M☉	28 ly
Gliese 3454 B	M4 V	0.13 M☉	28 ly
Gliese 877 HIP 113229, LHS 531, L 49-19, Ci 20 1389, GJ 877, HIC 113229, LFT 1747, 2MASS J22554532-7527320, NLTT 55234, Gaia DR2 6378584028690858496	M3 V	0 M☉	28 ly

Nombre de la estrella

Mass

Distance

Mu Herculis C

M3.5 V

0.39 M☉

27.1 ly

Gliese 747 B

M3 V

27.1 ly

Gliese 747

G 207-16, KUI 90, LFT 1451, LHS 471, L 1499-28, LP 336-6, LTT 15603, NLTT 47437

M3 V

27.1 ly

Mu Herculis Ab

M4 V

0.32 M☉

27.2 ly

Mu Herculis B

mu.02 Her

M3.5 V

0.44 M☉

27.2 ly

Gliese 1227

LHS 465, G 227-29, LP 103-305, NLTT 46427, 2MASS J18222719+6203025

M4 V

27.2 ly

Gliese 1289

G 130-4, LHS 4003, 2MASS J23430628+3632132, NLTT 57748, G 190-43, GJ 1289, TIC 352593978, WISEA J234307.14+363211.5

M4.5 V

0.21 M☉

27.3 ly

2MASS J18352–3123

2MASS J18352154–3123385, 1RXS J183520.9−312327

M6.5V

0 M☉

27.3 ly

2MASS J18352–3123 B

2MASS J18352205−3123421

M8 V

27.3 ly

SCR 1138-7721

2MASS J11381671-7721484, WISEA J113810.11-772142.2, SCR J1138-7721

M5 V

0.18 M☉

27.3 ly

2MASS J1546-5534

2MASS J15464185-5534468, DENIS J154641.8-553446, SCR J1546-5534, WISEA J154640.78-553446.0

M7.5

0.2 M☉

27.4 ly

Gliese 185 B

0.37 M☉

27.4 ly

TYC 3980-1081-1

IRAS 21500+5903, 2MASS J21513828+5917383

M3.9

0.2 M☉

27.6 ly

Gliese 232

Ross 64, JP11 5117, LHS 1846, LFT 467, G 104-37, LTT 11838, Ci 20 385

M4 V

0 M☉

27.7 ly

Gliese 618 B

LHS 416, LFT 1267, L 482-31, LTT 6509

0 M☉

27.7 ly

Gliese 618

CD-37 10765, LHS 415, LDS 6312, L 482-30, LFT 1266, LTT 6508, NLTT 42493, 2MASS J16200353-3731449, TYC 7853-670-1

M3 V

27.8 ly

Gliese 493.1

Wolf 461, V* FN Vir, G 60-55, G 62-5, LFT 962, LHS 2664, LTT 13750, NLTT 32583, 2MASS J13003350+0541081

M4.5 Ve

0 M☉

27.9 ly

Gliese 3454

LTT 17993, G 89-32, Nl 654, HEN 3, 2MASS J07362513+0704431, NLTT 18152

M4.5 V

0.15 M☉

28 ly

Gliese 3454 B

M4 V

0.13 M☉

28 ly

Gliese 877

HIP 113229, LHS 531, L 49-19, Ci 20 1389, GJ 877, HIC 113229, LFT 1747, 2MASS J22554532-7527320, NLTT 55234, Gaia DR2 6378584028690858496

M3 V

0 M☉

28 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...

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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....

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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....

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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.

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