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Lista de estrellas

        Nuestra galaxia, la Vía Láctea, contiene miles de millones de estrellas, desde estrellas masivas y brillantes hasta pequeños y tenues remanentes estelares. Algunas estrellas existen de forma independiente, mientras que muchas forman parte de sistemas binarios o múltiples. Esta página presenta una lista de las estrellas más cercanas al Sistema Solar, lo que ayuda a mapear nuestro vecindario estelar local y a comprender la diversidad de estrellas más cercanas a nosotros.

La lista se puede filtrar por categoría estelar, lo que permite explorar tipos específicos de estrellas, como enanas rojas, estrellas similares al Sol, enanas blancas o enanas marrones. Esta vista flexible facilita la comparación de diferentes poblaciones estelares y permite centrarse en objetos de interés. Si bien el enfoque principal se centra en las estrellas cercanas, el catálogo también se extiende más allá del vecindario inmediato, ofreciendo una perspectiva más amplia sobre los tipos de estrellas dentro de nuestra galaxia.
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Estrellas 381-400
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Nombre de la estrella Mass Distance

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

ULAS J133553.45+113005.2
WISEP J133553.41+113004.7
 T9 0.02 M☉ 33.7 ly

Pollux
β Geminorum, 78 Geminorum, BD+28°1463, GCTP 1826.00, Gliese 286, GJ 286, HD 62509, HIP 37826, HR 2990, LFT 548, LHS 1945, LTT 12065, SAO 79666, * bet Gem
 K0IIIb 1.9 M☉ 33.8 ly

32 G. Eridani
LWR 4A, BD-13 544, Ci 20 190, 2E 674, GJ 117, Gliese 117, HIC 13402, HIP 13402, HR 857, JP11 713, LTT 1372, 2MASS J02523210-1246109, NLTT 9195, NSV 975, RBS 367, TD1 1733, TIC 30016911, TYC 5292-897-1, V* EP Eri, HD 17925
 K1V 0.88 M☉ 33.8 ly

CFBDS J213926+022023
2MUCD 20912, WISEP J213927.09+022023.7, 2MASS J21392676+0220226, SIMP J01365662+0933473
 T1.5 0.04 M☉ 33.8 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

CPD-69 177
WD 0310-688
 DA3.0 0.66 M☉ 33.9 ly

LP 848-50
2MASS J10424135-2416050, NLTT 25128, SIPS J1042-2416, TIC 188035578
 - 33.9 ly

2MASS J1237+6526
SDSS J123738.88+652613.5, TIC 147681982, 2MASS 1237+6526, 2MASS J12373919+6526148
 T6.5 0.04 M☉ 33.9 ly

WISE J154214.00+223005.2
WISEA J154214.00+223005.2, WISE J154214.00+223005.2, EQ J1542+2230
 T9.5 - 34 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

2MASS J09083803+5032088
2MUCD 10802, SDSS J090837.91+503207.5, TIC 150171368, WISEA J090837.55+503203.3
 L8 - 34 ly

LP 852-7
WD 1202-232, 2MASS J12052666-2333125, NLTT 29555, TIC 398243520
 DA5.7 - 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 653
HD 154363, GJ 653, LHS 431, LFT 1316, TIC 142456308, LDS 585, BD-04 4225, GC 23043, G 19-13, HIC 83591, HIP 83591, LTT 6822, 2MASS J17050345-0503584, MCC 787, TYC 5072-408-1, WISEA J170502.78-050410.9, Wolf 635
 K4/5V - 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
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Estrellas 381-400
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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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Random terms
Posición de la estrellaLuminosidadTemperatura de la estrellaMasa estelarTamaño de la estrellaEdad de las estrellas

Evolución estelar

Stars are born and die in various ways depending on their mass, composition, and other factors. The most common life cycle for stars like our Sun involves several key stages.
Stellar evolution visualisation

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