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Etoile 41-60
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Nom de l étoile Mass Distance

Gliese 3618
LHS 288, Luyten 143-23, LTT 3946, RHG95 1673
 M5.5V 0.1 M☉ 15.8 ly

Gliese 1002
LHS 2, G 158-27, GCTP 9.01, Gaia DR2 2441630500517079808, GJ 1002, JP11 5942, 2MASS J00064325-0732147, NLTT 248, TIC 176287658, PM 00042-0747, UCAC4 413-000170, WISEA J000642.61-073237.0, Zkh 3
 M5.5 V C 0.11 M☉ 15.8 ly

Gliese 412
WX UMa, BD+44 2051, G 176-11, LTT 12976, LFT 757, LHS 38, LHS 39, NLTT 26245, FK5 4979, SAO 43609, HIP 54211, PLX 2582
 M2 V 0.48 M☉ 16 ly

Gliese 412 B
WX Ursae Majoris
 M6 V 0.1 M☉ 16 ly

AD Leonis
Gliese 388, BD+20 2465, G 54-23, LHS 5167, LTT 12761, NLTT 24015, SAO 81292, PLX 2420, TYC 1423-174-1
 dM3 0.4 M☉ 16.2 ly

Gliese 832
GJ 832, CD-49°13515, HD 204961, HIP 106440, LHS 3685, PLX 5190
 M1.5V 0.45 M☉ 16.2 ly

Gliese 1005
Luyten 722-22, HIC 1242, HIP 1242, G 158-50, G 266-76, LHS 1047, LP 764-87, LTT 114, GJ 1005, 2MASS J00152799-1608008
 M4V 0.18 M☉ 16.3 ly

Gliese 1005 B
 M7V 0.11 M☉ 16.3 ly

Gliese 682
CD-44 11909, GJ 682, LHS 451, LFT 1358, HIP 86214, HIC 86214, PLX 3992
 M3.5 0.2 M☉ 16.3 ly

40 Eridani C
DY Eri, BD-07°781 C, LHS 25, LTT 1909, omi02 Eri C
 M4.5 V 0.2 M☉ 16.4 ly

EV Lacertae
Gliese 873, GJ 873, BD+43 4305, LHS 3853, LTT 16695, HIP 112460, PLX 5520
 M3.5 0.35 M☉ 16.5 ly

EI Cancri B
LHS 2077, NLTT 20637
 M7 V 0.1 M☉ 16.6 ly

EI Cancri
EI Cnc, Gliese 1116, G 9-38, G 47-14, G 41-11, LP 426-40, LTT 12343
 M7 0.12 M☉ 16.8 ly

Gliese 3379
G 099-049, G 99-49, G 106-17, LTT 17897, NLTT 15908, PLX 1383.02, TYC 134-605-1, GJ 3379, WDS J06001+0242A, PLX 1383.02, 2MASS J06000351+0242236
 M3.5 V 0.23 M☉ 17 ly

Gliese 445
G 254-29, AC+79 3888, HIC 57544, HIP 57544, LFT 849, LHS 2459, LTT 13235, NLTT 28539, PLX 2722, GJ 445, глизе 445, JP11 5142, 2MASS J11474143+7841283, TIC 358615829, TYC 4553-192-1
 M4.0Ve C 0.2 M☉ 17.1 ly

2MASS J1540-5101
2MASS J154043.42-510135.7, WISEA J154045.67-510139.3, UCAC4 195-119117
 M6.5 V 0.09 M☉ 17.4 ly

Gliese 3323
LHS 1723, NLTT 14393, 2MASS J05015746-0656459, 1RXS J050157.6-065641, LP 656-38
 M4 Ve 0.16 M☉ 17.5 ly

Gliese 526
Lalande 25372, BD+15°2620, CD+15° 2620, HD 119850, HIP 67155, PLX 3135, SAO 100695, TYC 899-789-1, Wolf 498
 M1.5 V 0.28 M☉ 17.7 ly

Stein 2051
G 175-34, HIP 21088, WDS J04312+5858AB, Gliese 169.1, PLX 986.01, LHS 26, NLTT 13373, TYC 3744-412-1, 2MASS J04311147+585837, WISE J043113.20+585816.7
 M4 Ve 0.22 M☉ 18 ly

Gliese 251
LHS 1879, Ross 578, Wolf 294, HD 265866, HIP 33226, LHS 1879, LTT 11941, GJ 251
 M3 Ve 0.35 M☉ 18.2 ly
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Naines rouges nouvelles

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774
iconYesterday
iconÉtoiles | Exoplanètes | Naines rouges | TESS
Image: Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774
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
iconYesterday
iconÉtoiles | Exoplanètes | Naines rouge
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
iconÉtoiles | Exoplanètes | Naines rouges | Super-Terre | Atmosphères planétaires | 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 Naines rouges

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Parcourez les dernières études scientifiques sur les étoiles et les exoplanètes de notre galaxie. Découvrez les dernières recherches en astrophysique et en astronomie stellaire.
Les recherches en cours

 TIC 220432308
1129 ly
 +1 study icon Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields
yesterday

TOI 431
106 ly
 +4 study icon Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey
yesterday

L 115-21
41.9 ly
 study icon A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274)
yesterday

TOI-3686
841 ly
 study icon TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance
yesterday

HD 112485
5881 ly
 study icon Ensemble pulsational characteristics of eclipsing binaries containing β Cep stars observed by the TESS mission
19. 10. 2026
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Publications plus anciennes

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: Étoiles

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Étoiles
Les étoiles sont d’immenses sphères de gaz chaud qui brillent en produisant de l’énergie grâce à la fusion nucléaire dans leur noyau. La plupart des étoiles sont composées principalement d’hydrogène et d’hélium. Au centre d’une étoile, la pression et la température élevées provoquent la fusion des atomes d’hydrogène en hélium, libérant ainsi une énorme quantité d’énergie sous forme de lumière et de chaleur.
More about Étoiles tag icon
Random terms
Position de la étoileLuminositéTempérature des étoilesMasse stellaireTaille de l´étoileL´âge des étoiles

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