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Lista de Enanas rojas

        
    
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Estrellas 341-360
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Nombre de la estrella Mass Distance

Gliese 617 B
EW Draconis, EW Dra, Gliese 617 B, Gl 617 B, GJ 617 B, HIP 79762, TYC 4195-1167-1, 2MASS J16164537+6715224, WDS J16167+6714 B
M3.0Ve 0.4 M☉ 35.1 ly

1RXS J121408.0-234516
2MASS J12140866-2345172, SCR J1214-2345, TIC 429354344, RX J1214.1-2345
M4.5 - 35.1 ly

Gliese 617
LHS 3175, G 257-32, GJ 617 A, HIC 79755, HIP 79755, LFT 1263, LTT 14863, HD 147379, 2MASS J16164280+6714196, NLTT 42488, SAO 17026, TIC 230073581, TYC 4195-721-1, WISEA J161641.85+671420.6
M0Ve 0.6 M☉ 35.1 ly

Gliese 9349
CD-23 9765, LHS 2358, GJ 413.1, GJ 9349, HIC 54532, HIP 54532, LFT 764, L 683-112, LPM 368, LTT 4108, 2MASS J11093138-2435548, NLTT 26464, TIC 20325431, TYC 6640-765-1, WISEA J110930.72-243559.6
M2V 0.45 M☉ 35.1 ly

UCAC4 444-118477
2MASS J20091824-0113377, TIC 243800364, WISEA J200918.21-011342.2, SCR J2009-0113
M5.0V - 35.2 ly

Ross 145
M2V - 35.2 ly

Gliese 3820
LHS 2836, L 763-63, LP 799-7, LTT 5455, NLTT 35884, 2MASS J13591045-1950034
M4.5 V - 35.3 ly

Gliese 1050
LHS 157, GCRV 26217, GJ 1050, L 513-23, LFT 221, LP 941-142, LTT 1304, 2MASS J02395066-3407557, NLTT 8645, TIC 122574885, WISEA J023951.16-340815.1
M3 - 35.5 ly

Wolf 1478
LHS 2932, GJ 553.1, GJ 9484, Gliese 9484, HIC 70975, HIP 70975, LTT 5734, TIC 297175954, 2MASS J14310120-1217451, NLTT 37557, TIC 297175954, TYC 5571-551-1, WISEA J143100.88-121749.9
dM3.5 0.3 M☉ 35.5 ly

Ross 594
GJ 170, Gliese 170, G 81-21, JP11 5112, LFT 355, LHS 1674, LTT 11440, LTT 10440, NLTT 13380, 2MASS J04302527+3951000, TIC 238865036, V* V546 Per, WISEA J043025.53+395053.5
M5V - 35.5 ly

Gliese 4281
GJ 4281, LP 760-3, EPIC 206050032, LHS 523, 2MASS J22285440-1325178, NLTT 53958, WISEA J222854.11-132530.5
M6.5V - 35.5 ly

L 34-26
NLTT 18592, 2MASS J07491271-7642065, TIC 272232401, TYC 9381-1809-1, USNO-B1.0 0132-00043434, COCONUTS-2A
M3Ve 0.3 M☉ 35.5 ly

Gliese 4063
LP 229-17, NLTT 46690, 2MASS J18343664+4007266
M4 V 0 M☉ 35.5 ly

HR 9038 B
M2 - 35.5 ly

LP 847-48
HIC 48659, HIP 48659, NLTT 22957, 2MASS J09552387-2715405, TIC 22147322, TYC 6612-5-1
M3V - 35.6 ly

Gliese 228
GJ 228, BD+10 1032, G 102-53, G 105-16, HIC 29316, HIP 29316, LFT 458, LHS 1830, LTT 11799, NLTT 16165, 2MASS J06105481+1019056, Ross 79, TIC 229264027, WISEA J061054.84+101856.0
M2.5V - 35.6 ly

Gliese 228 B
- 35.6 ly

Gliese 3412
G 250-29, GJ 3412, HEI 334, HIC 33142, HIP 33142, LFT 493, LHS 221, L 1815-5, LP 87-237, LTT 11937, NLTT 17099, 2MASS J06540419+6052191, TIC 88334764, TYC 4110-2079-1, WISEA J065404.98+605208.1
M3.0Ve - 35.6 ly

Gliese 9492
G 239-25, GKI 4A, HIC 71898, HIP 71898, LTT 14363, NLTT 38229, MCC 723, 2MASS J14422164+6603208, GJ 9492
M3 V 0.41 M☉ 35.7 ly

V* V816 Her
GJ 4071, Gliese 4071, G 141-29, JNN 280A, L 1209-6, LP 510-15, LTT 15516, NLTT 46898, 2MASS J18424498+1354168, TIC 230345672, USNO-B1.0 1039-00345551
M5V - 35.7 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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