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
Gliese 493.1 Wolf 461, V* FN Vir, G 60-55, G 62-5, LFT 962, LHS 2664, LTT 13750, NLTT 32583, 2MASS J13003350+0541081	M4.5 Ve	0 M☉	27.9 ly
Gliese 3454 LTT 17993, G 89-32, Nl 654, HEN 3, 2MASS J07362513+0704431, NLTT 18152	M4.5 V	0.15 M☉	28 ly
Gliese 877 HIP 113229, LHS 531, L 49-19, Ci 20 1389, GJ 877, HIC 113229, LFT 1747, 2MASS J22554532-7527320, NLTT 55234, Gaia DR2 6378584028690858496	M3 V	0 M☉	28 ly
CD Ceti Gliese 1057, LHS 168, NLTT 10256, G 77-31, CD Cet, V* CD Cet	M4.5 V	0.16 M☉	28.1 ly
Zeta Tucanae FK5 10, GCTP 54, Gliese 17, GJ 17, HD 1581, HIP 1599, HR 77, LHS 5, LTT 167, SAO 248163, GC 401	F9.5V	0.99 M☉	28.1 ly
LP 502-56 Karmn J15305+094, LSPM J1530+0926, 2MASS J15303032+0926014, NLTT 40406, PM J15305+0926, TIC 393018418, Gaia DR2 1165479168642900992	M5.5V	-	28.1 ly
Gliese 3517 LHS 2065, LP 666-9, 2MUCD 10776, NLTT 20475, PLX 2122.01, 2MASS J08533619-0329321, TIC 7975441, WISEA J085335.79-032934.3	M9 V	0.07 M☉	28.2 ly
AP Columbae V* AP Col, LTT 2449, L 523-55, LP 949-15, 2MASS J06045215-3433360	M5 V	0.25 M☉	28.3 ly
PM J11413-3624 SIPS J1141-3624	M5	-	28.3 ly
Chi1 Orionis 54 Ori, Gliese 222, GJ 222, HR 2047, BD+20° 1162, HD 39587, LTT 11743, GCTP 1354.00, SAO 77705, HIC 27913, HIP 27913	G0 V	1 M☉	28.4 ly
Gliese 1207 G 19-7, L 988-42, LP 686-27, LTT 6767, LHS 3255, LFT 1312, NLTT 43858	M3.5 Ve	0 M☉	28.4 ly
LP 991-84	M4.5V	-	28.5 ly
2MASS 0036+1821 LSPM J0036+1821, 2MASS J00361617+1821104, 2MASSW J0036159+182110, USNO-B1.0 1083-00010105, Gaia DR3 2794735086363871360, BNA 1A, 2MASSW J0036162+182110, WDS J00363+1821A, Gaia DR2 2794735086363871360, CNS5 175, 2MUCD 20029, WISEA J003616.79+182111.6, TIC 426959594	L3.5	-	28.5 ly
Gliese 250 88 G. Monocerotis, BD -05°1844, GCTP 1606.00, HD 50281, HIP 32984, LFT 494, LHS 1875, LTT 2662, SAO 133805	K3.5 V	0.8 M☉	28.5 ly
Gliese 450 HIP 57802, G 148-13, MCC 135, NLTT 28756, HIC 57802, HIP 57802, NGP 36 11, 2MASS J11510737+3516188, BD+36 2119, MCC 135	M1.5 V	0.49 M☉	28.6 ly
41 G. Arae 41 Arae, CD-46° 11370, Gliese 666, GJ 666, HD 156274, HIP 84720, HR 6416, LHS 444, LTT 6886, SAO 227816, LPM 636, LFT 1334, * 41 Ara	G8V	0.81 M☉	28.7 ly
5 G. Capricorni HD 192310, CD-27° 14659, GCTP 4804.00, Gliese 785, HIP 99825, LHS 488, LTT 8009, NSV 12933, SAO 189065, HR 7722	K2 V	0.78 M☉	28.7 ly
Gliese 849 BD-05 5715, GCRV 13921, HIP 109388, LFT 1689, LHS 517, LPM 814, LTT 8889, NLTT 53078, GJ 849	M3.5 V	0.45 M☉	28.8 ly
Gliese 745 HIP 93873, HIP 93899, LHS 3432, LHS 3433, Ross 730, GJ 745	M1 V	0.35 M☉	28.8 ly
Xi Ursae Majoris Aa Alula Australis, ξ Ursae Majoris, ξ UMa, Xi UMa, 53 Ursae Majoris, BD+32°2132, CCDM J11182+3132, GC 15537, HIP 55203, IDS 11128+3206, SAO 62484, WDS J11182+3132	F8.5 V	0.97 M☉	28.8 ly

Nombre de la estrella

Mass

Distance

Gliese 493.1

Wolf 461, V* FN Vir, G 60-55, G 62-5, LFT 962, LHS 2664, LTT 13750, NLTT 32583, 2MASS J13003350+0541081

M4.5 Ve

0 M☉

27.9 ly

Gliese 3454

LTT 17993, G 89-32, Nl 654, HEN 3, 2MASS J07362513+0704431, NLTT 18152

M4.5 V

0.15 M☉

28 ly

Gliese 877

HIP 113229, LHS 531, L 49-19, Ci 20 1389, GJ 877, HIC 113229, LFT 1747, 2MASS J22554532-7527320, NLTT 55234, Gaia DR2 6378584028690858496

M3 V

0 M☉

28 ly

CD Ceti

Gliese 1057, LHS 168, NLTT 10256, G 77-31, CD Cet, V* CD Cet

M4.5 V

0.16 M☉

28.1 ly

Zeta Tucanae

FK5 10, GCTP 54, Gliese 17, GJ 17, HD 1581, HIP 1599, HR 77, LHS 5, LTT 167, SAO 248163, GC 401

F9.5V

0.99 M☉

28.1 ly

LP 502-56

Karmn J15305+094, LSPM J1530+0926, 2MASS J15303032+0926014, NLTT 40406, PM J15305+0926, TIC 393018418, Gaia DR2 1165479168642900992

M5.5V

28.1 ly

Gliese 3517

LHS 2065, LP 666-9, 2MUCD 10776, NLTT 20475, PLX 2122.01, 2MASS J08533619-0329321, TIC 7975441, WISEA J085335.79-032934.3

M9 V

0.07 M☉

28.2 ly

AP Columbae

V* AP Col, LTT 2449, L 523-55, LP 949-15, 2MASS J06045215-3433360

M5 V

0.25 M☉

28.3 ly

PM J11413-3624

SIPS J1141-3624

28.3 ly

Chi1 Orionis

54 Ori, Gliese 222, GJ 222, HR 2047, BD+20° 1162, HD 39587, LTT 11743, GCTP 1354.00, SAO 77705, HIC 27913, HIP 27913

G0 V

1 M☉

28.4 ly

Gliese 1207

G 19-7, L 988-42, LP 686-27, LTT 6767, LHS 3255, LFT 1312, NLTT 43858

M3.5 Ve

0 M☉

28.4 ly

LP 991-84

M4.5V

28.5 ly

2MASS 0036+1821

LSPM J0036+1821, 2MASS J00361617+1821104, 2MASSW J0036159+182110, USNO-B1.0 1083-00010105, Gaia DR3 2794735086363871360, BNA 1A, 2MASSW J0036162+182110, WDS J00363+1821A, Gaia DR2 2794735086363871360, CNS5 175, 2MUCD 20029, WISEA J003616.79+182111.6, TIC 426959594

L3.5

28.5 ly

Gliese 250

88 G. Monocerotis, BD -05°1844, GCTP 1606.00, HD 50281, HIP 32984, LFT 494, LHS 1875, LTT 2662, SAO 133805

K3.5 V

0.8 M☉

28.5 ly

Gliese 450

HIP 57802, G 148-13, MCC 135, NLTT 28756, HIC 57802, HIP 57802, NGP 36 11, 2MASS J11510737+3516188, BD+36 2119, MCC 135

M1.5 V

0.49 M☉

28.6 ly

41 G. Arae

41 Arae, CD-46° 11370, Gliese 666, GJ 666, HD 156274, HIP 84720, HR 6416, LHS 444, LTT 6886, SAO 227816, LPM 636, LFT 1334, * 41 Ara

G8V

0.81 M☉

28.7 ly

5 G. Capricorni

HD 192310, CD-27° 14659, GCTP 4804.00, Gliese 785, HIP 99825, LHS 488, LTT 8009, NSV 12933, SAO 189065, HR 7722

K2 V

0.78 M☉

28.7 ly

Gliese 849

BD-05 5715, GCRV 13921, HIP 109388, LFT 1689, LHS 517, LPM 814, LTT 8889, NLTT 53078, GJ 849

M3.5 V

0.45 M☉

28.8 ly

Gliese 745

HIP 93873, HIP 93899, LHS 3432, LHS 3433, Ross 730, GJ 745

M1 V

0.35 M☉

28.8 ly

Xi Ursae Majoris Aa

Alula Australis, ξ Ursae Majoris, ξ UMa, Xi UMa, 53 Ursae Majoris, BD+32°2132, CCDM J11182+3132, GC 15537, HIP 55203, IDS 11128+3206, SAO 62484, WDS J11182+3132

F8.5 V

0.97 M☉

28.8 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