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List of nearest Red dwarfs

        This page highlights red dwarfs near the Solar System, which are key targets in the study of nearby stars and planetary systems. Their abundance and long-lived stability make them especially interesting for exoplanet searches, including exoplanets in the habitable zone. Understanding nearby red dwarfs helps place our Sun in context and provides important clues about where habitable planets and potential life might be found.
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Star name Mass Distance

EQ Pegasi B
BD+19 5116B
 M4.0Ve 0.17 M☉ 20.4 ly

EQ Pegasi
Gliese 896, GJ 896, EQ Peg, BD+19° 5116, HIP 116132, WDS J23317+1956AB, G 68-24, G 129-19, G 128-71, LFT 1799, LHS 3965, LTT 16919, NLTT 57135
 M3.5 0.44 M☉ 20.4 ly

Gliese 581
Wolf 562, HO Librae, HO Lib, BD−07°4003, GJ 581, HIP 74995, LFT 1195, LHS 394, LPM 564, LTT 6112, NLTT 39886, TYC 5594-1093-1, BD-07 4003, Gl 581
 M3 V 0.31 M☉ 20.5 ly

Gliese 338 B
HD 79211, LFT 635, LHS 261, LTT 12426, HIC 120005, HIP 120005
 M0V 0.64 M☉ 20.7 ly

LHS 2090
LP 368-128, NLTT 20726, 2MASS J09002359+2150054
 M6.5V 0.09 M☉ 20.7 ly

V1054 Ophiuchi
V1054 Oph, Gliese 644, GJ 644, Wolf 630, VanBiesbroeck 8, HD 152751, HIP 82817, SAO 141439
 M3V 0.19 M☉ 21.1 ly

V1054 Ophiuchi Ba
 M4 Ve 0.35 M☉ 21.1 ly

V1054 Ophiuchi Bb
 M4 Ve 0.31 M☉ 21.1 ly

GL Virginis
GL Vir, Gliese 1156, Luyten 1190-34, G 12-30, LHS 324, LTT 13440, GCTP 2835.0, LP 494-77, 2MASS J12185939+1107338
 M4.5 Ve 0.12 M☉ 21.1 ly

Gliese 625
G 202-48, HIC 80459, PLX 3740.03, PM J16254+5418
 M1.5V 0.37 M☉ 21.1 ly

V1054 Ophiuchi C
VB 8
 M7.0 V 0.08 M☉ 21.2 ly

Gliese 643
Wolf 629, LHS 427, LDS 573C, HIC 82809, HIP 82809, PLX 3844, TIC 181589885, LTT 6750, LFT 1311
 M3.5 V 0.19 M☉ 21.2 ly

Gliese 1128
Luyten 100-115, L 100-115, LFT 680, LHS 271, LTT 3572, NLTT 22480, GSC 09209-00444, 2MASS J09424635-6853060, DENIS J094246.3-685309, GJ 1128
 M4.0V 0.17 M☉ 21.2 ly

Gliese 3737
L 471-42, LHS 337, LTT 4818, NLTT 31382, PM 12362-3805, 2MASS J12384914-3822527
 M4.5V 0.18 M☉ 21.7 ly

Gliese 829 B
 M3.5V 0.27 M☉ 21.9 ly

Gliese 408
Ross 104, HIP 53767, HIC 53767, LTT 12942, LHS 6193, G 58-32, 2MASS J11000432+2249592, G 119-49, GJ 408, WEB 9740, TIC 97472519, TYC 1978-1286-1
 M2.5V 0.41 M☉ 22 ly

Gliese 299
Ross 619, LHS 35, G 52-2, G 50-22, LTT 12146
 M4.5Ve 0.16 M☉ 22.1 ly

Gliese 3522
LHS 6158, G 41-14, LTT 12352, DEL 2, NLTT 20670, 2MASS J08585633+0828259, NN 3522
 M3.5 V 0.2 M☉ 22.1 ly

Gliese 3522 B
 M3.5 V 0.17 M☉ 22.1 ly

Gliese 3522 C
 M3.5 V 0.15 M☉ 22.1 ly
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Red dwarfs news

Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b
icon15. 10. 2026
iconStars | Exoplanets | Red dwarfs | Super-Earths | Planetary atmospheres | TESS
Image: Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b
TOI-2257 b represents a unique case in planetary science due to its 35-day orbital period and high eccentricity, which describes how much an orbit deviates from a perfect circle. Located in a sparsely populated region of planetary parameter space, it sits at a critical threshold where the combined effects of stellar radiation and tidal forces - gravitational stresses caused by the host star - begin to lose their influence over the planet. Simulations show that the planet remains near this transi...
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Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class
icon6. 10. 2026
iconStars | Exoplanets | Red dwarfs | James Webb Space Telescope | Planetary atmospheres | Ocean plane
Image: Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class
Analysis of sub-Neptune planets around Red dwarf stars using JWST data reveals a new category of hybrid worlds. These planets have atmospheric compositions that do not align with traditional gas dwarf or water world definitions. Study highlights include TOI-776 c....
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Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere
icon3. 10. 2026
iconStars | Exoplanets | Red dwarfs | James Webb Space Telescope | Planetary atmosphere
Image: Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere
Analysis of four transit observations of TRAPPIST-1 c shows the planet is likely airless. By using a new method to account for stellar activity, researchers ruled out thick carbon dioxide and nitrogen atmospheres for this rocky exoplanet....
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study iconResearch in Red dwarfs

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Browse the latest scientific studies on stars and exoplanets in our galaxy. Stellar Catalog provides access to scientific data from astrophysics and stellar or planetary astronomy. It's a resource for anyone interested in the newest discoveries about what lies beyond our solar system.
Latest discoveries

 WISE 0855-0714
7.3 ly
 study icon Water Cloud and Chemical Modulations in the Coldest Brown Dwarf
17. 10. 2026

WASP 94
687 ly
 study icon A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum
16. 10. 2026

KELT-2
439 ly
 study icon Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity
15. 10. 2026

TOI-2257
189 ly
 study icon The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b
15. 10. 2026

KELT-18
1032 ly
 study icon High-resolution transmission spectroscopy of KELT-18b Metastable helium detection at 1083 nm
14. 10. 2026
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More research

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: Stars

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Stars
Stars are enormous spheres of hot gas that shine by generating energy through nuclear fusion in their cores. Most stars are made primarily of hydrogen and helium. In the center of a star, intense pressure and temperature cause hydrogen atoms to fuse into helium, releasing a tremendous amount of energy as light and heat.
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