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Lista de Enanas rojas

        
    
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Estrellas 261-280
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Nombre de la estrella Mass Distance

Gliese 49
LHS 1179, BD+61 195, HIC 4872, HIP 4872, LFT 94, WNO 51A, G 244-7, NLTT 3392, LTT 10363, 2MASS J01023895+6220422, Wolf 46, GJ 49
M1.5 V 0.52 M☉ 32.2 ly

V388 Cassiopeiae
V388 Cas, Gliese 51, Wolf 47, WNO 51B, LFT 95, LHS 1183, LTT 10364, BD+61 195B, NLTT 3445, G 243-55, 2MASS J01031971+6221557, TIC 52183206, Zkh 21, WISEA J010320.94+622156.8
M5 V 0.52 M☉ 32.2 ly

Gliese 22
MCY 1, VYS 2A, ADS 433 AC, GJ 22 A, LFT 47, LHS 114, LTT 10178, 2MASS J00322970+6714080, NLTT 1707, TIC 420470817, TYC 4027-803-1, V547 Cas, WDS J00321+6715Aa, Gliese 22, V547 Cassiopeiae, BD+66 34A, ADS 440
M2V 0.38 M☉ 32.3 ly

Gliese 22 C
0.14 M☉ 32.3 ly

UPM J0815-2344
UCAC3 133-99469, 2MASS J08151117-2344157, TIC 437229644, UCAC4 332-044363
- 32.3 ly

Gliese 3988
G 203-42, LHS 3262, NLTT 44121, 2MASS J17032384+5124219, GJ 3988, Karmn J17033+514
M4.5 V 0.18 M☉ 32.3 ly

HD 232979
HD 232979, TYC 3732-542-1, HIP 21553
M0.5V - 32.3 ly

Gliese 1125
G 48-20, LHS 2149, HIC 46655, HIP 46655, LFT 653, L 1038-28, LP 607-58, LTT 12513, NLTT 21945, 2MASS J09304457+0019214
M3.5 V 0 M☉ 32.3 ly

AT Microscopii
V* AT Mic A, AT Mic, CD−32°16135, GJ 799, HD 196982, HIP 102141, SAO 212355, WDS J20452-3120BC, CD-32 1613, HIC 102141, RBS 1692, TIC 441398770, 2MASS J20415111-3226073, IRAS 20387-3236
M4.5Ve 0.25 M☉ 32.4 ly

Gliese 1065
G 160-28, LHS 183, NLTT 11991, 2MASS J03504432-0605400
M3 V 0 M☉ 32.4 ly

Gliese 1230
LP 319-2, G 184-19, GJ 1230, LHS 3405, TIC 317177585, NLTT 46862, LDS 6330
M4.5V 0.24 M☉ 32.4 ly

Gliese 1230 C
0.13 M☉ 32.4 ly

L 403-31
LHS 5264, PM J14038-4241, 2MASS J14035157-4241528, NLTT 36110, Gaia DR2 6109610086872510592
M5e - 32.4 ly

Gliese 1230 B
G 184-19B
M4.5V 0.3 M☉ 32.4 ly

CE Bootis
Gliese 569, HIC 72944, HIP 72944, G 136-28, BD+16 2708, FRT 1, V* CE Boo, GJ 569
M2.5 V 0.35 M☉ 32.4 ly

Gliese 22 B
LHS 115, VYS 2B, ADS 433 B, GJ 22 B, Gliese 22 B, LFT 48, LTT 10179, NLTT 1708, 2MASS J00322979+6714043, TIC 420470815, TYC 4027-802-1, Zkh 11, BD+66 34B
M3V 0 M☉ 32.5 ly

Gliese 3855
LP 98-79, LHS 2930, NLTT 37621, 2MASS J14303787+5943249, 2MASS J1430+5943
M6.5V 0.2 M☉ 32.5 ly

Gliese 102
L 1305-10, LP 354-46, CSI+24-02307, LSPM J0233+2455, LTT 10844, G 36-24, JP11 5108, LFT 215, LHS 1417, PLX 514, NLTT 8312, 2MASS J02333717+2455392, USNO 408
M3.5 V - 32.6 ly

Gliese 239
LHS 1858, BD+17 1320, G 110-5, G 104-49, HD 260655, HIC 31635, HIP 31635, JP11 53, LFT 477, LTT 11880, NLTT 16743, 2MASS J06371092+1733526, Wolf 287, TOI-4599
M0 Ve 0.44 M☉ 32.6 ly

Ross 440
GJ 352, Gliese 352, KPR 41, KUI 41, HIC 46706, HIP 46706, LFT 656, LHS 2151, LTT 3500, 2MASS J09311936-1329192, MCC 26, NLTT 21974, TIC 293521985, TYC 5472-348-1, UBV M 5362
M3V - 32.7 ly
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Enanas rojas noticias

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A
iconToday
iconEstrellas | 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
iconToday
iconEstrellas | 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
icon15. 10. 2026
iconEstrellas | Exoplanetas | Enanas rojas | Supertierras | Atmósferas planetarias | TESS
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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study iconResearch in Enanas rojas

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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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