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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 481-500
>
Nombre de la estrella Mass Distance

EGGR 148
GJ 836.5, Gliese 836.5, G 145-63, G 126-27, LFT 1655, LHS 3703, L 1363-3, LP 458-64, LTT 16348, NLTT 51906, 2MASS J21424099+2059582, SDSS J214240.92+205954.9, TIC 354568302, WD 2140+207, WISEA J214240.83+205951.2
 DQ6 - 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

HD 166620
BD+38°3095, GJ 706, Gliese 706, HD 166620, HIP 88972, HR 6806, SAO 66700, LHS 3363, LHS 3363, G 205-5, IRAS 18079+3826, LAL 33439, LFT 1396, LTT 15374, 2MASS J18093745+3827288, NLTT 46046, TIC 75946144, TYC 3102-1975-1, WISEA J180937.13+382723.0
 K2V 0.79 M☉ 36.2 ly

LSR J1826+3014
 M8.5V - 36.2 ly

OGLE BLG-ECL-216148
Gaia DR2 4042278603157583616
 - 36.2 ly

54 Piscium
54 Psc, NSV 245, BD+20°85, FK5 276, Gliese 27, HD 3651, HIP 3093, HR 166, SAO 74175, LHS 1116, LTT 10224
 K0 V 0.76 M☉ 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

Theta Persei
* tet Per, θ Per, BD+48°746, GJ 107, Gliese 107, CCDM J02441+4913, IDS 02374+4848, WDS J02442+4914, 13 Persei, HR 799, HD 16895, HIP 12777, FK5 93, GC 3277, PPM 45428, SAO 38288
 F8V 1.1 M☉ 36.4 ly

BD+47 2112
LHS 2849, ADS 9090 A, G 200-16A, GJ 537 A, Gliese 537, LFT 1065, LTT 14107, 2MASS J14023312+4620239, NLTT 36091, TIC 198151134, TYC 3465-617-1
 M2V - 36.4 ly

Gamma Serpentis
LHS 408, 41 Ser, * gam Ser, Ainalhai, 41 Serpentis, BD+16° 2849, FK5 591, GCTP 3604.00, HD 142860, HIP 78072, HR 5933, LHS 408, SAO 101826, TIC 377415363, TYC 1496-2119-1, WISEA J155627.41+153928.7, NLTT 41572, N30 3579, GJ 603, Gliese 603
 F6V 1.3 M☉ 36.4 ly

UPM J0812-3529
WD 0810-353, TIC 145863747, 2MASS J08122707-3529433
 DAH 0.63 M☉ 36.4 ly

L 380-8
LHS 1831, GJ 1088, Gliese 1088, LFT 460, LTT 2480, NLTT 16205, 2MASS J06105288-4324178, TIC 231917352, WISEA J061053.00-432410.0
 M4e - 36.5 ly

HD 74576
LTT 3225, GJ 320, Gliese 320, HIC 42808, HIP 42808, 2MASS J08431805-3852569, NLTT 20139, SAO 199544, TIC 181273463, TYC 7675-3469-1
 K3V 0.65 M☉ 36.5 ly
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Estrellas 481-500
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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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