Enanas rojas | Stellar Catalog

	Mass	Distance
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
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
Chi1 Orionis B	M6	0.15 M☉	28.3 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
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
Gliese 250 B HD 50281B	M2.5 V	0.5 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
Gliese 1103 B	M V	0.06 M☉	28.6 ly
41 G. Arae C		-	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
HU Delphini B	M3V	0.11 M☉	28.8 ly
41 G. Arae B * 41 Ara B	M0V	0.52 M☉	28.8 ly
Gliese 745 B ROSS 731	M1 V	0.35 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
LDS 169B L 32-8, NLTT 16774, HIC 31292, 2MASS J06334690-7537301, HIP 31292, GSC 09379-01149, IDS 06371-7533 B, TIC 142086813, TYC 9379-1149-1, WDS J06337-7538B	M3 V	0.4 M☉	28.8 ly
LDS 169 L 32-9 A, LTT 2602, HIP 31293, IRAS 06355-7535, EXO 063528-7535.1	M2 V	0 M☉	28.8 ly
Gliese 1105 HIP 38956, LHS 1963, G 111-47, NLTT 18699, HIC 38956, LSPM J0758+4118, TYC 2968-1142-1	M3.5 V	0.25 M☉	28.9 ly

Nombre de la estrella

Mass

Distance

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

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

Chi1 Orionis B

0.15 M☉

28.3 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

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

Gliese 250 B

HD 50281B

M2.5 V

0.5 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

Gliese 1103 B

M V

0.06 M☉

28.6 ly

41 G. Arae C

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

HU Delphini B

M3V

0.11 M☉

28.8 ly

41 G. Arae B

* 41 Ara B

M0V

0.52 M☉

28.8 ly

Gliese 745 B

ROSS 731

M1 V

0.35 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

LDS 169B

L 32-8, NLTT 16774, HIC 31292, 2MASS J06334690-7537301, HIP 31292, GSC 09379-01149, IDS 06371-7533 B, TIC 142086813, TYC 9379-1149-1, WDS J06337-7538B

M3 V

0.4 M☉

28.8 ly

LDS 169

L 32-9 A, LTT 2602, HIP 31293, IRAS 06355-7535, EXO 063528-7535.1

M2 V

0 M☉

28.8 ly

Gliese 1105

HIP 38956, LHS 1963, G 111-47, NLTT 18699, HIC 38956, LSPM J0758+4118, TYC 2968-1142-1

M3.5 V

0.25 M☉

28.9 ly

Enanas rojas noticias

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A

Today

Estrellas | Exoplanetas | Enanas rojas | TESS

Image: Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A

A small planet candidate has been identified in the binary star system known as Gliese 774. The object, which is smaller than the Earth, orbits its host star approximately every 4.2 days. Observations from the Transiting Exoplanet Survey Satellite (TESS) captured the planet as it passed in front of its star, briefly blocking a tiny fraction of the starlight. This periodic dimming event allowed for the identification of the candidate despite the complex environment of a binary system, where two s...

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Ammonia and hydrogen may separate inside Uranus and Neptune

Today

Estrellas | Exoplanetas | Enanas roj

Image: Ammonia and hydrogen may separate inside Uranus and Neptune

Uranus and Neptune may be experiencing ammonia rain: simulations show their expected temperature profiles cross the boundary where ammonia and hydrogen separate. In warmer sub-Neptune TOI-270 d, the two are likely to mix in all proportions....

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Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

15. 10. 2026

Image: Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

The exoplanet TOI-2257 b orbits its star once every 35 days with a high eccentricity. New models suggest its atmospheric and orbital fate depends on whether it is a gas-rich mini-Neptune or a rocky super-Earth. Higher eccentricity would confirm a gaseous nature....

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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.

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

TOI 431 106 ly		Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey today
L 115-21 41.9 ly		A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274) today
TOI-3686 841 ly		TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance today
HD 112485 5881 ly		Ensemble pulsational characteristics of eclipsing binaries containing β Cep stars observed by the TESS mission 19. 10. 2026
TOI-5322 1560 ly	+1	A Sample of Thick-Disk Stars Hosting Hot Jupiters 17. 10. 2026

Lista de Enanas rojas

Enanas rojas noticias

Research in Enanas rojas

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