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Catalogue étoile
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Liste des etoile

        Notre galaxie, la Voie lactée, abrite des milliards d'étoiles, des plus massives et brillantes aux plus faibles vestiges stellaires. Certaines étoiles sont isolées, tandis que beaucoup font partie de systèmes binaires ou multiples. Cette page présente une liste des étoiles les plus proches du Système solaire, permettant de cartographier notre voisinage stellaire et de comprendre la diversité des étoiles qui nous sont les plus proches.

La liste peut être filtrée par catégorie stellaire, ce qui vous permet d'explorer des types d'étoiles spécifiques comme les naines rouges, les étoiles semblables au Soleil, les naines blanches ou les naines brunes. Cette vue flexible facilite la comparaison de différentes populations stellaires et la concentration sur les objets d'intérêt. Bien que l'accent soit mis principalement sur les étoiles proches, le catalogue s'étend également au-delà de notre voisinage immédiat, offrant une perspective plus large sur les types d'étoiles au sein de notre galaxie.
    
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Etoile 501-520
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Nom de l étoile Mass Distance

L 762-51
LHS 2794, EPIC 212285603, GJ 3804, Gliese 3804, HIC 67164, HIP 67164, LFT 1035, L 762-51, LP 798-34, LTT 5346, 2MASS J13455074-1758047, NLTT 35132, TIC 286942673, TYC 6127-534-1
dM3.5 - 36.5 ly

L 136-37
LTT 2816, NLTT 17788, 2MASS J07205204-6210118, DENIS J072051.9-621011, TIC 349374765, WISEA J072051.59-621009.5
M3 - 36.6 ly

Gliese 173
GJ 173, BD-11 916, LP 715-52, GCRV 2717, HIC 21556, HIP 21556, LTT 2050, 2MASS J04374188-1102198, MCC 106, NLTT 13657, TIC 55997717, TYC 5324-581-1, WEB 4138
M1V 0.48 M☉ 36.6 ly

Ross 508
LHS 396, G 137-2, G 136-103, GJ 585, Gliese 585, JP11 5158, LFT 1203, LTT 14584, 2MASS J15235112+1727569, NLTT 40124, TIC 400019820, WISEA J152350.85+172744.4
M4.92 0.18 M☉ 36.6 ly

EGGR 248
GJ 1086, Gliese 1086, G 106-4, G 99-37, LTT 17876, NLTT 15714, 2MASS J05511947-0010213, SDSS J055119.47-001021.4, TIC 176670072, WD 0548-001
DQ8P - 36.6 ly

UCAC4 608-044702
2MASS J08401597+3127068, TIC 341526939, LSPM J0840+3127
M3.5Ve - 36.6 ly

HD 28343
GJ 169, Gliese 169, HIC 20917, HIP 20917, LTT 11433, NLTT 13343, 2MASS J04290013+2155214, TIC 17558287, TYC 1277-601-1, WISEA J042900.05+215523.6
M0.5V - 36.6 ly

2MASS J0700+3157
2MASSI J0700366+315726, TIC 165098841, WISEA J070036.77+315719.7, WDS J07006+3157AB
L3+L6.5 - 36.6 ly

11 Leonis Minoris
11 LMi, BD+36°1979, GJ 356, Gliese 356, HD 82885, HIC 47080, HIP 47080, HR 3815, SAO 61586, WDS 09357+3549, GC 13242, TIC 8915802, TYC 2500-1533-1, WISEA J093538.92+354834.4, LTT 12535, NLTT 22117, 2MASS J09353959+3548366
G8Va 0.96 M☉ 36.6 ly

2MASS J19251275+0700362
TIC 133125017, WISE J192512.78+070038.8
L7 - 36.6 ly

Arcturus
* alf Boo, Alpha Boötis, Alramech, Abramech, α Boötis, 16 Boötis, BD+19°2777, GJ 541, Gliese 541, HD 124897, HIC 69673, HIP 69673, HR 5340, SAO 100944, LHS 48, GCTP 3242.00
K1.5IIIFe-0.5 1.1 M☉ 36.7 ly

Gliese 3959
2E 3717, G 180-60, HAT 193-01110, NLTT 43010, 2MASS J16311879+4051516, SDSS J163118.77+405152.1, NN 3959, GJ 3959
M6 V 0 M☉ 36.7 ly

G 107-69
LHS 229, G 111-7, G 193-50, GJ 275.2 A, Gliese 275.2 A, 2MASS J07304280+4811599, NLTT 17949, TIC 328328639, WISEA J073042.55+481145.2
M4V - 36.8 ly

2MASS J16452211-1319516
TIC 203506666, WISEA J164521.83-132000.6
L1.5 - 36.8 ly

LP 625-34
GJ 3967, Gliese 3967, 2MASS J16400599+0042188, NLTT 43307, TIC 281935723,
M5V - 36.8 ly

HD 85512
CD−42°5678, Gaia DR2 5412947081287925504, GJ 370, Gliese 370, HIC 48331, HIP 48331, LHS 2201, 2MASS J09510700-4330097
K6Vk: 0.69 M☉ 36.8 ly

PM J17189-4131
DENIS J171854.5-413140, 2MASS J17185456-4131395, TIC 192642951, WISEA J171854.33-413149.6
M6 - 36.8 ly

G 3-14
LHS 1290, G 71-28, GJ 70, Gliese 70, HIC 8051, HIP 8051, LFT 1851, LTT 10604, NLTT 5733, 2MASS J01432015+0419172, TIC 369534824, TYC 32-1005-1, WISEA J014319.89+041910.0
M2V - 36.9 ly

LP 938-71
DENIS J010250.6-373744, LHS 132, 2MASS J01025100-3737438, NLTT 3459, TIC 180724005, WISEA J010252.38-373741.0
M8.0V - 36.9 ly

PM J19515-3510
NSN 488A, WDS J19516-3511A
M4 D - 37 ly
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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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Évolution stellaire

Stars are born and die in various ways depending on their mass, composition, and other factors. The most common life cycle for stars like our Sun involves several key stages.
Stellar evolution visualisation

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