Lista de estrellas más cercanas | Catálogo de estrellas

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.

	Mass	Distance
55 Cancri Copernicus, LHS 2062, LDS 6219A, GJ 324 A, Gliese 324, HD 75732, Rho1 Cancri, 55 Cnc, BD+28°1660, HIC 43587, HIP 43587, HR 3522, SAO 80585, rho01 Cnc, LFT 609, LTT 12310, NLTT 20414, TIC 332064670, TOI-1773, TYC 1949-2012-1, WISEA J085235.41+281948.5	G8V	1 M☉	41.1 ly
L 207-41	M4	-	41.1 ly
Gliese 1132 GJ 1132, LHS 281, L 320-124, GCRV 26265, LFT 707, LTT 3758, 2MASS J10145184-4709244, NLTT 23819, TIC 101955023, WISE J101450.69-470919.8	M4 D	0.18 M☉	41.1 ly
LAWD 10	DA+D1	-	41.2 ly
Gaia EDR3 1800808220172866048		-	41.2 ly
1RXS J0635-0403 1RXS J063531.2-040314	M5.5V	-	41.2 ly
Gliese 1072 G 85-19, GJ 1072, LHS 1706, NLTT 14034, 2MASS J04505083+2207224, TIC 18685916, WISEA J045051.40+220717.1	M5V	-	41.3 ly
SIPS J0539-0059 2MASS J05395200-0059019, SDSS J053951.99-005902.0, WISEA J053952.11-005858.1	L5V	-	41.3 ly
Wolf 1056	M2.5V	0.4 M☉	41.3 ly
Gliese 422 HD 304043, LHS 40, GJ 422, HIP 55042, HIC 55042, LFT 784, L 192-72, LTT 4167, 2MASS J11160018-5732513, Innes star, NLTT 26836, TIC 450545735, TYC 8624-3387-1, WISEA J111557.03-573239.3	M3.5 D	0.35 M☉	41.3 ly
PM J22114+4059	M5.5V	-	41.4 ly
HD 190007 V1654 Aql, V1654 Aquilae, BD+02° 4076, GJ 775, Gliese 775, HD 190007, HIC 98698, HIP 98698, SAO 125379, GC 27782, 2MASS J20024703+0319344, SAO 125379, TIC 345217789, TYC 498-2720-1, USNO-B1.0 0933-00588224, WISE J200246.98+031935.5	K5V B	0.68 M☉	41.5 ly
UCAC4 026-011435 2MASS J23303802-8455189, TIC 401834404, PM J23306-8455		-	41.5 ly
Wolf 1555	M0	-	41.5 ly
G 236-34	M4V	-	41.5 ly
LP 560-35	M6V	-	41.5 ly
2MASS J0523-1403 2MASS J05233822−1403022, 2MUCD 10390, B2006 J052338.2−140302, 2MASSI J0523382−140302, USNO-B1.0 0759−00062850, TIC 442929628, WISEA J052338.30-140300.3	L2.5V	0.06 M☉	41.5 ly
L 21-3	M4e	-	41.5 ly
2MASS J0144-0716 2MASS J01443536-0716142	L6.5	-	41.5 ly
LDS 390 GJ 3708, Gliese 3708, L 758-108	dM3.0	0.35 M☉	41.6 ly

Nombre de la estrella

Mass

Distance

55 Cancri

Copernicus, LHS 2062, LDS 6219A, GJ 324 A, Gliese 324, HD 75732, Rho1 Cancri, 55 Cnc, BD+28°1660, HIC 43587, HIP 43587, HR 3522, SAO 80585, rho01 Cnc, LFT 609, LTT 12310, NLTT 20414, TIC 332064670, TOI-1773, TYC 1949-2012-1, WISEA J085235.41+281948.5

G8V

1 M☉

41.1 ly

L 207-41

41.1 ly

Gliese 1132

GJ 1132, LHS 281, L 320-124, GCRV 26265, LFT 707, LTT 3758, 2MASS J10145184-4709244, NLTT 23819, TIC 101955023, WISE J101450.69-470919.8

M4 D

0.18 M☉

41.1 ly

LAWD 10

DA+D1

41.2 ly

Gaia EDR3 1800808220172866048

41.2 ly

1RXS J0635-0403

1RXS J063531.2-040314

M5.5V

41.2 ly

Gliese 1072

G 85-19, GJ 1072, LHS 1706, NLTT 14034, 2MASS J04505083+2207224, TIC 18685916, WISEA J045051.40+220717.1

M5V

41.3 ly

SIPS J0539-0059

2MASS J05395200-0059019, SDSS J053951.99-005902.0, WISEA J053952.11-005858.1

L5V

41.3 ly

Wolf 1056

M2.5V

0.4 M☉

41.3 ly

Gliese 422

HD 304043, LHS 40, GJ 422, HIP 55042, HIC 55042, LFT 784, L 192-72, LTT 4167, 2MASS J11160018-5732513, Innes star, NLTT 26836, TIC 450545735, TYC 8624-3387-1, WISEA J111557.03-573239.3

M3.5 D

0.35 M☉

41.3 ly

PM J22114+4059

M5.5V

41.4 ly

HD 190007

V1654 Aql, V1654 Aquilae, BD+02° 4076, GJ 775, Gliese 775, HD 190007, HIC 98698, HIP 98698, SAO 125379, GC 27782, 2MASS J20024703+0319344, SAO 125379, TIC 345217789, TYC 498-2720-1, USNO-B1.0 0933-00588224, WISE J200246.98+031935.5

K5V B

0.68 M☉

41.5 ly

UCAC4 026-011435

2MASS J23303802-8455189, TIC 401834404, PM J23306-8455

41.5 ly

Wolf 1555

41.5 ly

G 236-34

M4V

41.5 ly

LP 560-35

M6V

41.5 ly

2MASS J0523-1403

2MASS J05233822−1403022, 2MUCD 10390, B2006 J052338.2−140302, 2MASSI J0523382−140302, USNO-B1.0 0759−00062850, TIC 442929628, WISEA J052338.30-140300.3

L2.5V

0.06 M☉

41.5 ly

L 21-3

M4e

41.5 ly

2MASS J0144-0716

2MASS J01443536-0716142

L6.5

41.5 ly

LDS 390

GJ 3708, Gliese 3708, L 758-108

dM3.0

0.35 M☉

41.6 ly

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

Lista de estrellas

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

Evolución estelar