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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 61-80
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Nom de l étoile Mass Distance

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

2MASS 0939-2448
2MASS J09393548−2448279, 2MASS J09393548-2448279
T8 0.03 M☉ 16.6 ly

70 Ophiuchi
Gliese 702, GJ 702, LHS 458, V2391 Ophiuchi, BD+02 3482, HD 165341, HIP 88601, HR 6752, PLX 4137, 70 Oph
K0-V 0.9 M☉ 16.7 ly

Altair
Alpha Aquilae, α Aquilae, Gliese 768, 53 Aquilae, 53 Aql, BD+08°4236, FK5 745, GCTP 4665.00, Gliese 768, HD 187642, HIP 97649, HR 7557, LFT 1499, LHS 3490, LTT 15795, NLTT 48314, SAO 125122, WDS 19508+0852A, alf Aql
A7 V 1.8 M☉ 16.7 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

WISE J1506+7027
WISEPC J150649.97+702736.0, 2MASS J15065257+7027247, WISE J150649.97+702736.1, TIC 232535619, EQ J1506+7027
T6 0.09 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

2MASS J08173001-6155158
DENIS J081730.0-615520, TIC 309290163, WISEA J081729.76-615503.8, Gaia DR2 5278042880077383040
T6 0.01 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

2MASS J0254+0223
2MASS J02540788+0223563, ULAS J025409.58+022358.7, WISEA J025409.55+022358.5, WISE J025409.51+022358.6, PSO J043.5+02
T8 0.06 M☉ 17.6 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

LP 816-60
LP 816-060, HIP 103039, NLTT 50038, TYC 6348-400-1, 2MASS J20523304-1658289
M3.5 V 0.19 M☉ 18.3 ly

2MASS J11145133-2618235
TIC 20489807, 2MASS J11145133-2618235, WISEA J111448.74-261827.9
T7.5 0.03 M☉ 18.4 ly

WISE 1741+2553
WISEPA J174124.26+255319.5, EQ J1741+2553, 2MASS J17412462+2553343, WISEP J174124.25+255319.5
T9 0 M☉ 18.5 ly

2MASS 1835+3259
2MASSI J1835379+325954, 2MASS 1835+32, 2MASS J18353790+3259545, 2MUCD 11792, [B2006] J183537.9+325955, LSPM J1835+3259, USNO-B1.0 1229-00376318, LSR J1835+3259
M8.5 0.07 M☉ 18.6 ly

Gliese 205
Wolf 1453, BD-03° 1123, GJ 205, HD 36395, HIP 25878, LHS 30, SAO 132211, W. B. V. 592, Weisse I, 5h 592, Strb. 1611, Cin. 705, Ci 20=334, G 99-15, LFT 416, LTT 2293, NLTT 15215 PLX 1255, TYC 4770-574-1, 2MASS J05312734-0340356
M1.5 V 0.56 M☉ 18.6 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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