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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 421-440
>
Nombre de la estrella Mass Distance

LP 867-15
EPIC 215818496, 2MASS J18421107-2328582, NLTT 46868, TIC 3882477
 M3.5 - 34.6 ly

G 22-26
 M4V - 34.6 ly

Gaia EDR3 3489874340630661248
 - 34.6 ly

G 261-6
LHS 3461, GJ 1238, Gliese 1238, LP 25-636, 2MASS J19241634+7533121, NLTT 47831, TIC 420130591, WISEA J192417.32+753318.0
 M6V 0.13 M☉ 34.7 ly

DENIS J145407.8-660447
2MASS J14540797-6604476, TIC 259315924, WISEA J145408.80-660451.2
 L3.5 - 34.7 ly

Ross 165
GJ 766 A, Gliese 766, WDS J19458+2710A, KUI 95, KPR 95, HIC 97237, HIP 97237, LFT 1491, LHS 478, LTT 15768, NLTT 48208, 2MASS J19454548+2707318, TIC 451852919, TYC 2147-1374-1, WISEA J194545.48+270719.0
 M4V - 34.7 ly

HD 111631
G 14-6, G 60-41, GJ 488, Gliese 488, HIC 62687, HIP 62687, LTT 4913, 2MASS J12504357-0046047, MCC 675, NLTT 32069, TIC 53280272, TYC 4950-67-1, WISEA J125043.52-004609.2, YZ 90 3469
 M0V - 34.8 ly

Gliese 4154
LHS 3583, GJ 4154, L 23-30, LFT 1559, LTT 8178, NLTT 49675, 2MASS J20463725-8143141, TIC 401667290, WISEA J204639.66-814319.2
 M3e 0.38 M☉ 34.8 ly

SCR J0821-6703
WD 0821-669, 2MASS J08212670-6703201, SCR J0821-6703, TIC 307363368, WD 0820-668, WISEA J082125.99-670313.0
 DA10.0 - 34.8 ly

2MASS J0243−2453
2MASSI J0243137-245329, 2MASS J02431371−2453298
 T6.0 0.03 M☉ 34.8 ly

Zeta Herculis
ζ Her, 40 Her, ADS 10157 AB, BD+31 2884, GJ 635, HD 150680, HIP 81693, HR 6212, LHS 3234, LTT 14952, SAO 65485, WDS J16413+3136AB, zet Her
 F9 IV 1.5 M☉ 35 ly

TVLM 513-46
TVLM 513-46546, 2MASS J15010818+2250020, 2MASSI J1501081+225001, 2MUCD 20596, SDSS J150108.17+225001.8, TIC 311188315, WISEP J150108.17+225001.4
 M8.5V C 0.09 M☉ 35 ly

Gliese 669
GJ 669 A, Gliese 669, G 170-35, HIC 84794, HIP 84794, LTT 15139, NLTT 44616, 2MASS J17195422+2630030, RBS 1637, SDSS J171954.30+262957.9, TIC 257798327, TYC 2082-2076-1, V* V647 Her, WISEA J171954.02+263006.7, Ross 868
 M3.5V - 35.1 ly

V* V857 Cen
GJ 431, Gliese 431, HIC 56244, HIP 56244, LFT 821, LHS 2423, L 396-7, LTT 4255, NLTT 27672, 2MASS J11314655-4102473, TIC 181015118, TYC 7744-1540-1, ISEA J113145.82-410245.2
 M3.5 0.3 M☉ 35.1 ly

Gliese 86
Gl 86, GJ 86, CD−51°532, HD 13445, HIP 10138, HR 637, SAO 232658, WDS J02104-5049A, LHS 13, ESG 1A, GSC 08048-01022, LFT 186, LPM 103, LTT 1130, 2MASS J02102587-5049258, N30 446, NLTT 7238, TIC 220017951, TYC 8048-1022-1, WISEA J021028.31-504918.3,
K1V 0.88 M☉ 35.1 ly

1RXS J121408.0-234516
2MASS J12140866-2345172, SCR J1214-2345, TIC 429354344, RX J1214.1-2345
 M4.5 - 35.1 ly

Gliese 617
LHS 3175, G 257-32, GJ 617 A, HIC 79755, HIP 79755, LFT 1263, LTT 14863, HD 147379, 2MASS J16164280+6714196, NLTT 42488, SAO 17026, TIC 230073581, TYC 4195-721-1, WISEA J161641.85+671420.6
 M0Ve 0.6 M☉ 35.1 ly

Gliese 9349
CD-23 9765, LHS 2358, GJ 413.1, GJ 9349, HIC 54532, HIP 54532, LFT 764, L 683-112, LPM 368, LTT 4108, 2MASS J11093138-2435548, NLTT 26464, TIC 20325431, TYC 6640-765-1, WISEA J110930.72-243559.6
 M2V 0.45 M☉ 35.1 ly

UCAC4 444-118477
2MASS J20091824-0113377, TIC 243800364, WISEA J200918.21-011342.2, SCR J2009-0113
M5.0V - 35.2 ly

Ross 145
 M2V - 35.2 ly
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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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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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