Enanas rojas | Stellar Catalog

	Mass	Distance
LSPM J0510+2714 LSR J0510+2713, 2MASS J05102012+2714032, TIC 69850453, WISEA J051019.92+271355.3, USNO-B1.0 1172-00096972	M7V	-	33.5 ly
Gliese 1232 LHS 3438, CRC 32A, G 185-9, G 142-11, GJ 1232, Gliese 1232, JP11 5097, LFT 1454, L 1283-23, LP 452-2, LTT 15611, 2MASS J19095098+1740074, NLTT 47484, TIC 395665737, Gaia DR2 4514347014274847744	M4V	-	33.5 ly
Gliese 3147 LP 245-10, GJ 3147, LHS 1378, NLTT 7516, TIC 63781635, 2MASS J02170993+3526330, WISEA J021710.48+352629.7	M7V C	-	33.7 ly
Gliese 1277 LHS 532, LTT 928-1, LFT 1750, L 167-14, NLTT 55304, 2MASS J22562466-6003490	M4.5 V	0 M☉	33.9 ly
Gliese 649 LHS 3257, ASCC 694128, BD+25 3173, Ci 20 1014, GCRV 9782, G 169-38, G 170-6, GJ 649, Gliese 649, HIC 83043, HIP 83043, IRAS 16560+2549, LFT 1313, LTT 15016, 2MASS J16580884+2544392, MCC 785, NLTT 43922, Ross 860, TIC 236743275, TYC 2063-479-1, Zkh 239	M1V	0.51 M☉	33.9 ly
LSPM J2044+1517 2MASS J20443743+1517352, TIC 341162242, WISEA J204437.70+151733.1	M8	-	33.9 ly
LP 848-50 2MASS J10424135-2416050, NLTT 25128, SIPS J1042-2416, TIC 188035578		-	33.9 ly
HD 122303 LHS 2842, BD-01 2892, DO 3431, G 64-35, GJ 536, Gliese 536, HIC 68469, HIP 68469, LFT 1061, L 979-36, LPM 504, LTT 5470, 2MASS J14010324-0239180, NLTT 35989, TIC 119147875, TYC 4978-501-1, WISEA J140102.63-023911.1	M0V	0.53 M☉	34 ly
SCR J0533-4257 SYU 7, 2MASS J05332802-4257205, RAVE J053328.0-425721, RBS 661, 1RXS J053328.4-425713, TIC 302962949, WDS J05335-4257AB	M4.5	-	34 ly
Gliese 341 LHS 2128, CD-59 2351, HD 304636, HIC 45908, HIP 45908, LFT 643, L 140-9, LTT 3453, 2MASS J09213761-6016551, NLTT 21618, TOI 741	M1V	0.52 M☉	34.1 ly
Gliese 3459 LP 783-1, LHS 1935, GJ 3459, HIC 37217, HIP 37217, LFT 540, L 672-9, LP 783-1, LTT 2906, NLTT 18223, 2MASS J07384089-2113276, TIC 415085843, TYC 5992-530-1	M3.0	-	34.1 ly
Gliese 654 BD-04 4226, GJ 654, HD 154363B, G 19-14, HIC 83599, HIP 83599, LFT 1317, NC 42, WISEA J170513.16-050550.7	M1.5V	0.48 M☉	34.1 ly
LP 169-22 LHS 2395, 2MASS J11193058+4641437, NLTT 26984, TIC 148673115, UCAC2 47535582, USNO-B1.0 1366-00221246	M5.5	-	34.1 ly
Gliese 3976 G 169-29, NLTT 43674, 2MASS J16505794+2227058, LSPM J1650+2227	M5 V	0 M☉	34.1 ly
L 140-289 LHS 5156, LFT 677, L 140-289, LTT 3567, 2MASS J09424960-6337560, NLTT 22459, TIC 362253884, WISEA J094250.40-633755.2	M4.5V	-	34.2 ly
2MASS J0330+5413 LSPM J0330+5413, TIC 316627328, USNO-B1.0 1442-00105844, WISEA J033048.70+541355.0, 2MASS J03304890+5413551	M7V	-	34.3 ly
Gliese 754.1 B LDS 678B, CSI-07-19179 2, GJ 754.1 B, L 923-22	M5V	-	34.3 ly
BD+02 348	M1V	-	34.3 ly
Gliese 373 LHS 2211, G 235-49, G 236-7, GJ 373, BD+63 869, BD+63 869, HIC 48714, HIP 48714, LFT 688, L 1869-6, LSPM J0956+6247, LTT 12638, 2MASS J09560868+6247185, MCC 121, NLTT 22923, TIC 287165117, TYC 4140-922-1, VVO 170	M0.5Ve	-	34.3 ly
Wolf 44 LHS 1176, GJ 47, Gliese 47, LFT 90, G 243-50, 2MASS J01012006+6121560, NLTT 3322, TIC 256316623, TYC 4017-558-1, WISEA J010120.55+612148.4	M2.0Ve	0.37 M☉	34.3 ly

Nombre de la estrella

Mass

Distance

LSR J0510+2713, 2MASS J05102012+2714032, TIC 69850453, WISEA J051019.92+271355.3, USNO-B1.0 1172-00096972

M7V

33.5 ly

LHS 3438, CRC 32A, G 185-9, G 142-11, GJ 1232, Gliese 1232, JP11 5097, LFT 1454, L 1283-23, LP 452-2, LTT 15611, 2MASS J19095098+1740074, NLTT 47484, TIC 395665737, Gaia DR2 4514347014274847744

M4V

33.5 ly

Gliese 3147

LP 245-10, GJ 3147, LHS 1378, NLTT 7516, TIC 63781635, 2MASS J02170993+3526330, WISEA J021710.48+352629.7

M7V C

33.7 ly

Gliese 1277

LHS 532, LTT 928-1, LFT 1750, L 167-14, NLTT 55304, 2MASS J22562466-6003490

M4.5 V

0 M☉

33.9 ly

Gliese 649

LHS 3257, ASCC 694128, BD+25 3173, Ci 20 1014, GCRV 9782, G 169-38, G 170-6, GJ 649, Gliese 649, HIC 83043, HIP 83043, IRAS 16560+2549, LFT 1313, LTT 15016, 2MASS J16580884+2544392, MCC 785, NLTT 43922, Ross 860, TIC 236743275, TYC 2063-479-1, Zkh 239

M1V

0.51 M☉

33.9 ly

LSPM J2044+1517

2MASS J20443743+1517352, TIC 341162242, WISEA J204437.70+151733.1

33.9 ly

LP 848-50

2MASS J10424135-2416050, NLTT 25128, SIPS J1042-2416, TIC 188035578

33.9 ly

HD 122303

LHS 2842, BD-01 2892, DO 3431, G 64-35, GJ 536, Gliese 536, HIC 68469, HIP 68469, LFT 1061, L 979-36, LPM 504, LTT 5470, 2MASS J14010324-0239180, NLTT 35989, TIC 119147875, TYC 4978-501-1, WISEA J140102.63-023911.1

M0V

0.53 M☉

34 ly

SCR J0533-4257

SYU 7, 2MASS J05332802-4257205, RAVE J053328.0-425721, RBS 661, 1RXS J053328.4-425713, TIC 302962949, WDS J05335-4257AB

M4.5

34 ly

Gliese 341

LHS 2128, CD-59 2351, HD 304636, HIC 45908, HIP 45908, LFT 643, L 140-9, LTT 3453, 2MASS J09213761-6016551, NLTT 21618, TOI 741

M1V

0.52 M☉

34.1 ly

Gliese 3459

LP 783-1, LHS 1935, GJ 3459, HIC 37217, HIP 37217, LFT 540, L 672-9, LP 783-1, LTT 2906, NLTT 18223, 2MASS J07384089-2113276, TIC 415085843, TYC 5992-530-1

M3.0

34.1 ly

Gliese 654

BD-04 4226, GJ 654, HD 154363B, G 19-14, HIC 83599, HIP 83599, LFT 1317, NC 42, WISEA J170513.16-050550.7

M1.5V

0.48 M☉

34.1 ly

LP 169-22

LHS 2395, 2MASS J11193058+4641437, NLTT 26984, TIC 148673115, UCAC2 47535582, USNO-B1.0 1366-00221246

M5.5

34.1 ly

Gliese 3976

G 169-29, NLTT 43674, 2MASS J16505794+2227058, LSPM J1650+2227

M5 V

0 M☉

34.1 ly

L 140-289

LHS 5156, LFT 677, L 140-289, LTT 3567, 2MASS J09424960-6337560, NLTT 22459, TIC 362253884, WISEA J094250.40-633755.2

M4.5V

34.2 ly

2MASS J0330+5413

LSPM J0330+5413, TIC 316627328, USNO-B1.0 1442-00105844, WISEA J033048.70+541355.0, 2MASS J03304890+5413551

M7V

34.3 ly

Gliese 754.1 B

LDS 678B, CSI-07-19179 2, GJ 754.1 B, L 923-22

M5V

34.3 ly

BD+02 348

M1V

34.3 ly

Gliese 373

LHS 2211, G 235-49, G 236-7, GJ 373, BD+63 869, BD+63 869, HIC 48714, HIP 48714, LFT 688, L 1869-6, LSPM J0956+6247, LTT 12638, 2MASS J09560868+6247185, MCC 121, NLTT 22923, TIC 287165117, TYC 4140-922-1, VVO 170

M0.5Ve

34.3 ly

Wolf 44

LHS 1176, GJ 47, Gliese 47, LFT 90, G 243-50, 2MASS J01012006+6121560, NLTT 3322, TIC 256316623, TYC 4017-558-1, WISEA J010120.55+612148.4

M2.0Ve

0.37 M☉

34.3 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