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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 381-400
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Nom de l étoile Mass Distance

Gliese 3147
LP 245-10, GJ 3147, LHS 1378, NLTT 7516, TIC 63781635, 2MASS J02170993+3526330, WISEA J021710.48+352629.7
M7V C - 33.7 ly

ULAS J133553.45+113005.2
WISEP J133553.41+113004.7
T9 0.02 M☉ 33.7 ly

Pollux
β Geminorum, 78 Geminorum, BD+28°1463, GCTP 1826.00, Gliese 286, GJ 286, HD 62509, HIP 37826, HR 2990, LFT 548, LHS 1945, LTT 12065, SAO 79666, * bet Gem
K0IIIb 1.9 M☉ 33.8 ly

32 G. Eridani
LWR 4A, BD-13 544, Ci 20 190, 2E 674, GJ 117, Gliese 117, HIC 13402, HIP 13402, HR 857, JP11 713, LTT 1372, 2MASS J02523210-1246109, NLTT 9195, NSV 975, RBS 367, TD1 1733, TIC 30016911, TYC 5292-897-1, V* EP Eri, HD 17925
K1V 0.88 M☉ 33.8 ly

CFBDS J213926+022023
2MUCD 20912, WISEP J213927.09+022023.7, 2MASS J21392676+0220226, SIMP J01365662+0933473
T1.5 0.04 M☉ 33.8 ly

Gliese 1277
LHS 532, LTT 928-1, LFT 1750, L 167-14, NLTT 55304, 2MASS J22562466-6003490
M4.5 V 0 M☉ 33.9 ly

Gliese 649
LHS 3257, ASCC 694128, BD+25 3173, Ci 20 1014, GCRV 9782, G 169-38, G 170-6, GJ 649, Gliese 649, HIC 83043, HIP 83043, IRAS 16560+2549, LFT 1313, LTT 15016, 2MASS J16580884+2544392, MCC 785, NLTT 43922, Ross 860, TIC 236743275, TYC 2063-479-1, Zkh 239
M1V 0.51 M☉ 33.9 ly

LSPM J2044+1517
2MASS J20443743+1517352, TIC 341162242, WISEA J204437.70+151733.1
M8 - 33.9 ly

CPD-69 177
WD 0310-688
DA3.0 0.66 M☉ 33.9 ly

LP 848-50
2MASS J10424135-2416050, NLTT 25128, SIPS J1042-2416, TIC 188035578
- 33.9 ly

2MASS J1237+6526
SDSS J123738.88+652613.5, TIC 147681982, 2MASS 1237+6526, 2MASS J12373919+6526148
T6.5 0.04 M☉ 33.9 ly

WISE J154214.00+223005.2
WISEA J154214.00+223005.2, WISE J154214.00+223005.2, EQ J1542+2230
T9.5 - 34 ly

HD 122303
LHS 2842, BD-01 2892, DO 3431, G 64-35, GJ 536, Gliese 536, HIC 68469, HIP 68469, LFT 1061, L 979-36, LPM 504, LTT 5470, 2MASS J14010324-0239180, NLTT 35989, TIC 119147875, TYC 4978-501-1, WISEA J140102.63-023911.1
M0V 0.53 M☉ 34 ly

SCR J0533-4257
SYU 7, 2MASS J05332802-4257205, RAVE J053328.0-425721, RBS 661, 1RXS J053328.4-425713, TIC 302962949, WDS J05335-4257AB
M4.5 - 34 ly

2MASS J09083803+5032088
2MUCD 10802, SDSS J090837.91+503207.5, TIC 150171368, WISEA J090837.55+503203.3
L8 - 34 ly

LP 852-7
WD 1202-232, 2MASS J12052666-2333125, NLTT 29555, TIC 398243520
DA5.7 - 34 ly

Gliese 341
LHS 2128, CD-59 2351, HD 304636, HIC 45908, HIP 45908, LFT 643, L 140-9, LTT 3453, 2MASS J09213761-6016551, NLTT 21618, TOI 741
M1V 0.52 M☉ 34.1 ly

Gliese 3459
LP 783-1, LHS 1935, GJ 3459, HIC 37217, HIP 37217, LFT 540, L 672-9, LP 783-1, LTT 2906, NLTT 18223, 2MASS J07384089-2113276, TIC 415085843, TYC 5992-530-1
M3.0 - 34.1 ly

Gliese 653
HD 154363, GJ 653, LHS 431, LFT 1316, TIC 142456308, LDS 585, BD-04 4225, GC 23043, G 19-13, HIC 83591, HIP 83591, LTT 6822, 2MASS J17050345-0503584, MCC 787, TYC 5072-408-1, WISEA J170502.78-050410.9, Wolf 635
K4/5V - 34.1 ly

LP 169-22
LHS 2395, 2MASS J11193058+4641437, NLTT 26984, TIC 148673115, UCAC2 47535582, USNO-B1.0 1366-00221246
M5.5 - 34.1 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.
More about Étoiles tag icon

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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