Enanas rojas | Stellar Catalog

	Mass	Distance
2MASS J15345704-1418486 TIC 386928810, WISEA J153456.27-141852.6	M8.6V	-	35.7 ly
LP 851-346 DENIS J115542.9-222458, 2MASS J11554286-2224586, SIPS J1155-2224, TIC 5630425, WISEA J115542.56-222500.7	M7.5V	-	35.7 ly
LP 271-25 GJ 3849, Gliese 3849, FS 134, LHS 2924, 2MASS J14284323+3310391, NLTT 37480, SDSS J142843.13+331036.8, TIC 286963145, WISEA J142842.93+331031.7	M9Ve	-	35.8 ly
CD-45 1184 LTT 1678, CF 1005, GJ 145, Gliese 145, HIC 16536, HIP 16536, NLTT 11234, 2MASS J03325585-4442070, TIC 79568861, TYC 7574-455-1, UCAC4 227-003357	M2.5V	0.34 M☉	35.8 ly
LP 853-12		-	35.8 ly
Gliese 1129 LHS 273, L 750-52, GJ 1129, LFT 681, LP 788-30, LTT 3578, 2MASS J09444731-1812489, NLTT 22505, TIC 418096656	M3.5Ve	-	35.8 ly
HD 115404 B	M0.5 V	0.54 M☉	35.9 ly
Gliese 438 CD-51 5974, LFT 839, LHS 2447, CF 9268, L 252-28, LTT 4348, NLTT 28348, 2MASS J11431977-5150255, GJ 438, PLX 2709, TIC 93716498, TYC 8227-1613-1	M1 D	0.4 M☉	35.9 ly
Ross 1003 Gaia DR2 772430527947893632, GJ 1148, Gliese 1148, LTT 13210, 2MASS J11414471+4245072, LHS 2443, G 122-40, HIP 57050, HIC 57050, LFT 836, LTT 13210, NLTT 28266, TIC 115869504, TYC 3016-1877-1, WISEA J114144.08+424506.2	M4.0Ve	0.34 M☉	36 ly
Wolf 1561 GJ 852 A, LDS 782A, DENIS J221719.0-084811, EPIC 206262336, LFT 1699, LHS 3787, LTT 8938, 2MASS J22171899-0848122, NLTT 53397, V* FG Aqr, Zkh 329, WDS J22173-0847A	M4V	-	36 ly
HD 11507 G 272-114, G 274-109, GJ 79, Gliese 79, HIC 8768, HIP 8768, LFT 168, LHS 1307, LTT 1005, NLTT 6302, 2MASS J01524908-2226055, TIC 266680951, TYC 5858-74-1, WISEA J015249.82-222605.4	M0V	-	36.1 ly
LP 993-115 IDS 02414-4409 A, LTT 1339, 2MASS J02451070-4344319, NLTT 8911, PM J02451-4344, TIC 142305549, WISEA J024510.75-434436.0	M4	-	36.2 ly
CD-56 1032	M3Ve	-	36.2 ly
CD-56 1032B	M4Ve	-	36.2 ly
LSR J1826+3014	M8.5V	-	36.2 ly
Gliese 740 GJ 740, LHS 470, HD 176029, HIC 93101, BD+05 3993, NLTT 47240, LTT 15568, LFT 1443	M1.0Ve	0.58 M☉	36.2 ly
Gliese 3069 G 218-20, GJ 3069, 2MASS J01015952+5410577, NLTT 3373, TIC 252110114, WISEA J010159.12+541056.4	M5	-	36.2 ly
SCR J0838-5855 DENIS J083802.2-585558, 2MASS J08380224-5855583, TIC 44984200, WISEA J083802.10-585601.7	M6e	-	36.2 ly
MCC 188 GJ 735, Gliese 735, AC +08 142-393, 2E 4160, GCRV 68818, HIC 92871, HIP 92871, IRAS 18530+0820, JP11 5167, 2MASS J18552740+0824090, TIC 102107794, TYC 1039-1079-1, V* V1285 Aql, VVO 105	M3Ve	-	36.3 ly
SCR J0717-0501 2MASS J07171706-0501031, SCR J0717-0500	M3.5V	-	36.3 ly

Nombre de la estrella

Mass

Distance

2MASS J15345704-1418486

TIC 386928810, WISEA J153456.27-141852.6

M8.6V

35.7 ly

LP 851-346

DENIS J115542.9-222458, 2MASS J11554286-2224586, SIPS J1155-2224, TIC 5630425, WISEA J115542.56-222500.7

M7.5V

35.7 ly

LP 271-25

GJ 3849, Gliese 3849, FS 134, LHS 2924, 2MASS J14284323+3310391, NLTT 37480, SDSS J142843.13+331036.8, TIC 286963145, WISEA J142842.93+331031.7

M9Ve

35.8 ly

CD-45 1184

LTT 1678, CF 1005, GJ 145, Gliese 145, HIC 16536, HIP 16536, NLTT 11234, 2MASS J03325585-4442070, TIC 79568861, TYC 7574-455-1, UCAC4 227-003357

M2.5V

0.34 M☉

35.8 ly

LP 853-12

35.8 ly

Gliese 1129

LHS 273, L 750-52, GJ 1129, LFT 681, LP 788-30, LTT 3578, 2MASS J09444731-1812489, NLTT 22505, TIC 418096656

M3.5Ve

35.8 ly

HD 115404 B

M0.5 V

0.54 M☉

35.9 ly

Gliese 438

CD-51 5974, LFT 839, LHS 2447, CF 9268, L 252-28, LTT 4348, NLTT 28348, 2MASS J11431977-5150255, GJ 438, PLX 2709, TIC 93716498, TYC 8227-1613-1

M1 D

0.4 M☉

35.9 ly

Ross 1003

Gaia DR2 772430527947893632, GJ 1148, Gliese 1148, LTT 13210, 2MASS J11414471+4245072, LHS 2443, G 122-40, HIP 57050, HIC 57050, LFT 836, LTT 13210, NLTT 28266, TIC 115869504, TYC 3016-1877-1, WISEA J114144.08+424506.2

M4.0Ve

0.34 M☉

36 ly

Wolf 1561

GJ 852 A, LDS 782A, DENIS J221719.0-084811, EPIC 206262336, LFT 1699, LHS 3787, LTT 8938, 2MASS J22171899-0848122, NLTT 53397, V* FG Aqr, Zkh 329, WDS J22173-0847A

M4V

36 ly

HD 11507

G 272-114, G 274-109, GJ 79, Gliese 79, HIC 8768, HIP 8768, LFT 168, LHS 1307, LTT 1005, NLTT 6302, 2MASS J01524908-2226055, TIC 266680951, TYC 5858-74-1, WISEA J015249.82-222605.4

M0V

36.1 ly

LP 993-115

IDS 02414-4409 A, LTT 1339, 2MASS J02451070-4344319, NLTT 8911, PM J02451-4344, TIC 142305549, WISEA J024510.75-434436.0

36.2 ly

CD-56 1032

M3Ve

36.2 ly

CD-56 1032B

M4Ve

36.2 ly

LSR J1826+3014

M8.5V

36.2 ly

Gliese 740

GJ 740, LHS 470, HD 176029, HIC 93101, BD+05 3993, NLTT 47240, LTT 15568, LFT 1443

M1.0Ve

0.58 M☉

36.2 ly

Gliese 3069

G 218-20, GJ 3069, 2MASS J01015952+5410577, NLTT 3373, TIC 252110114, WISEA J010159.12+541056.4

36.2 ly

SCR J0838-5855

DENIS J083802.2-585558, 2MASS J08380224-5855583, TIC 44984200, WISEA J083802.10-585601.7

M6e

36.2 ly

MCC 188

GJ 735, Gliese 735, AC +08 142-393, 2E 4160, GCRV 68818, HIC 92871, HIP 92871, IRAS 18530+0820, JP11 5167, 2MASS J18552740+0824090, TIC 102107794, TYC 1039-1079-1, V* V1285 Aql, VVO 105

M3Ve

36.3 ly

SCR J0717-0501

2MASS J07171706-0501031, SCR J0717-0500

M3.5V

36.3 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

	TIC 220432308 1129 ly			Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields today
	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

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