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Liste des Naines rouges

        
    
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Etoile 461-480
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Nom de l étoile Mass Distance

Ross 46
G 97-54, G 102-16, GJ 3356, Gliese 3356, LTT 11684, NLTT 15307, 2MASS J05345212+1352471, TIC 52373734, WISEA J053452.03+135242.6
M3V 0.33 M☉ 38.8 ly

UCAC4 203-192841
PM J22403-4931B
- 38.9 ly

G 109-55
GJ 268.3, Gliese 268.3, GJ 9227, Gliese 9227, HIC 35191, HIP 35191, 2MASS J07161977+2708331, NLTT 17613, TIC 155753765, TYC 1917-2452-1
M3V - 38.9 ly

UCAC4 203-192840
PM J22403-4931A
M5.5 - 38.9 ly

G 184-31
M4.5V - 38.9 ly

DS Leonis
DS Leo, Gliese 410, GJ 410, Gl 410, HD 95650, HIC 53985, HIP 53985, V* DS Leo
M1.0V 0.58 M☉ 38.9 ly

Gliese 180
LHS 1712, CSI-17-04516, HIC 22762, HIP 22762, LFT 377, L 736-30, LP 776-27, LPM 198, LTT 2116, 2MASS J04534995-1746235, NLTT 14144, PLX 1097, PLX 1097.00, TYC 5903-680-1, [RHG95] 838, GJ 180
M3 Vc 0.39 M☉ 39 ly

UCAC4 439-049099
PM J09218-0219
M2.5V - 39 ly

L 504-27
M4 - 39 ly

Gliese 96
G 173-53, BD+47 612, GJ 96, HIC 11048, HIP 11048, 2MASS J02221463+4752481, NLTT 7753, TIC 409527090, TYC 3298-1434-1, WISEA J022214.85+475248.5
M0V 0.57 M☉ 39 ly

BUG 5
BUG 5, ** BUG 5A, WDS J17074-0558A, 2MASS J17072343-0558249, DENIS J170723.4-055824, WDS J17074-0558AB, TIC 145473406
M9Ve - 39 ly

VV Lyncis B
- 39.1 ly

G 148-48
M5 - 39.1 ly

G 208-42
GJ 1243, Gliese 1243, HAT 155-01856, KIC 9726699, 2MASS J19510930+4628598, TIC 273589987, WISEA J195109.50+462903.0
M4.0V - 39.1 ly

G 148-47
LSPMJ1221+3038W, GIC 106A, LP 320-416, NLTT 30450, 2MASS J12212673+3038376, TIC 357187278, WISE J122126.56+303835.0
M4.5e - 39.1 ly

VV Lyncis C
Ross 989
M4.0V - 39.1 ly

VV Lyncis
V* VV Lyn, BD+36 1638A, G 111-12, G 87-44, G 90-8, GJ 277, Gliese 277, HIC 36626, HIP 36626, LTT 12034, NLTT 17999, 2MASS J07315773+3613102, TIC 16034014, TYC 2465-984-1, WDS J07319+3613A
M2.5V C - 39.1 ly

WT 2458
2MASS J09455843-3253299, TIC 11974826, WISEA J094558.17-325328.4
M4.5 - 39.2 ly

Ross 149
M4V - 39.2 ly

Wolf 654
LTT 15087, GJ 3992, Gliese 3992, HIC 84099, HIP 84099, 2MASS J17113472+3826341, TIC 85463294, TYC 3073-1045-1, Gaia DR2 1341113541156480768, NLTT 44340
M4V 0.36 M☉ 39.3 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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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.
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