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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 361-380
>
Nombre de la estrella Mass Distance

WISE 1322-2340
 T8 - 32.9 ly

HD 223889
L 26-27, CD-76 1182, DENIS J235349.8-753756, HIC 117828, HIP 117828, LTT 9759, 2MASS J23535017-7537575, NLTT 58294, TIC 402104884, TYC 9477-617-1, WISEA J235350.77-753800.5
 M3 - 33 ly

Gliese 678.1
BD+05 3409, G 139-43, WOR 25, GJ 9592, HIC 85665, HIP 85665, LTT 15197, NLTT 44915, MCC 321, 2MASS J17302272+0532547, Wolf 751
 M1 Ve 0 M☉ 33 ly

WISE J081117.81-805141.3
 T9.5 - 33.1 ly

Gliese 453
LHS 319, GC 16365, GJ 453, HD 103932, HIC 58345, HIP 58345, LFT 865, LTT 4450, 2MASS J11575619-2742251, TIC 403802333, TYC 6674-576-1, Zkh 175
 K4+V - 33.2 ly

G 97-15
GJ 3326, Gliese 3326, LTT 17736, 2MASS J05041476+1103238, NLTT 14445, TIC 415508270, WISEA J050414.71+110325.9
 M5V - 33.2 ly

WISE 1614+1739
WISE J161441.46+173935.5, CNS5 3987, WISEA J161441.47+173935.4
 T9 - 33.2 ly

Gliese 660
GJ 660, G 19-15, LPM 629, HIC 84123, HIP 84123, LFT 1324, LHS 3269, L 989-20, LPM 629, LP 627-9, LTT 6854, NLTT 44323, 2MASS J17115234-0151057, TIC 142948307, TYC 5065-23-1, WISEA J171152.00-015108.8
 M3V - 33.2 ly

Alpha Mensae
Alf Men, Alp Men, CD−74° 294, FK5 239, GJ 231, Gliese 231, HD 43834, HIP 29271, HR 2261, SAO 256274, LTT 2490
 G7 V 1.1 M☉ 33.3 ly

Gliese 487
G 237-78, GJ 487, DEL 4, AC +66 3955, HIC 62556, HIP 62556, JP11 5150, LSPM J1249+6606, LTT 13665, NLTT 32013, 2MASS J12490273+6606366, TIC 341687654, TYC 4168-824-1, V* DP Dra, WISEA J124902.00+660635.8, Gaia DR2 1677568527365572224
 M3V - 33.3 ly

Gliese 203
HIP 25578, Ross 41, GJ 203, LHS 1761, LFT 411, G 102-3, G 97-42, LTT 11651, NLTT 15107, 2MASS J05280015+0938382
 M3.5Ve 0.22 M☉ 33.3 ly

UCAC4 175-092532
2MASS J12455254-5506502, SCR J1245-5506, TIC 419692115, WISEA J124552.96-550651.6
 M5e - 33.3 ly

Gliese 1265
GJ 1265, L 788-37, LHS 3776, LFT 1695, LP 819-52, LTT 8915, 2MASS J22134277-1741081, NLTT 53236, WISEA J221343.49-174111.9
 dM4.5 C 0.18 M☉ 33.4 ly

Gliese 3049
LHS 1134, LFT 69, 2MASS J00432603-4117337, L 363-38, LTT 400, LP 989-140, NLTT 2382, GJ 3049
 M5 0.21 M☉ 33.4 ly

L 273-106
LHS 5341, LFT 1428, L 273-106, LTT 7416, NLTT 46865, 2MASS J18430697-5436481, TIC 120395704, WISEA J184306.81-543653.4
 M5 - 33.4 ly

Gliese 1083
G 100-28, GJ 1083, WNO 45, LTT 17846, NLTT 15441, TIC 75326630, V* V780 Tau, 2MASS J05402570+2448090, USNO 307, WISEA J054025.79+244804.2
 M7V - 33.4 ly

2MASS J0419+4233
2MASS J04195212+4233304, TIC 347994537, WISEA J041952.62+423315.4, LSPM J0419+4233, LSR J0419+4233
 M8/9V - 33.5 ly

Gliese 339.1
EGGR 250, EGGR 250, G 195-19, LHS 262, NLTT 21302, SDSS J091555.98+532522.8, TIC 251080865, WD 0912+536, 2MASS J09155623+5325249, WISEA J091554.79+532512.0
 DCP7 - 33.5 ly

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
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Estrellas 361-380
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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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