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Liste des Sous-géantes

        
    
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Etoile 21-40
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Nom de l étoile Mass Distance

Delta Aquilae Aa
del Aql, Al Mizān I, δ Aql, 30 Aql, BD+02° 3879, FK5 730, Gliese 760, GJ 760, HD 182640, HIP 95501, HR 7377, SAO 124603, NLTT 47775
F1IV-V(n) 1.7 M☉ 50.6 ly

51 Pegasi
Helvetios, 51 Peg, Gliese 882, GJ 882, HR 8729, BD +19°5036, HD 217014, LTT 16750, NLTT 55385, GCTP 5568.00, SAO 90896, HIC 113357, HIP 113357, GC 32003, 2MASS J22572795+2046077, TIC 139298196, TYC 1717-2193-1, WDS J22575+2046A
G2IV B 1.1 M☉ 50.6 ly

Mu Arae
Cervantes, CD −51° 11094, FK5 662, GC 24024, Gliese 691, GJ 691, HD 160691, HIC 86796, HIP 86796, HR 6585, SAO 244981, LTT 7053, * mu. Ara, 2MASS J17440870-5150027, TIC 362661163, TYC 8355-436-1
G3IV-V C 1.1 M☉ 50.9 ly

Tau Boötis
τ Boo, 4 Boötis, NSV 6444, BD+18°2782, FK5 507, GC 18637, GJ 527, HD 120136, HIP 67275, HR 5185, SAO 100706, ADS 9025, CCDM 13473+1727, LTT 14021
F7IV-V 1.4 M☉ 50.9 ly

HD 158614
STF 2173, BD−00°3300, Gliese 678, GJ 678, HIP 85667, HR 6516, SAO 141702, WDS J17304-0104
G9-IV-VHdel1 0.96 M☉ 53.7 ly

HD 158614 B
G9IV-V 0.95 M☉ 53.7 ly

HD 200968
K1IV - 56.7 ly

Tau6 Eridani
τ6 Eri, 27 Eridani, CD−23°1565, FK5 140, GC 168827, HD 23754, HIP 17651, HR 1173, SAO 101600
F5IV-V 1.4 M☉ 58 ly

Delta Leonis
Zosma, Zozma, Zosca, Duhr, Zubra, δ Leo, 68 Leo, BD +21°2298, FK5 422, GC 15438, GCTP 2614.00, Gl 419, Gliese 419, HD 97603, HIP 54872, HR 4357, SAO 81727, del Leo
A5IV(n) 2.2 M☉ 58.4 ly

HP Boötis
HD 130948, GJ 564, BD+24° 2786, HD 130948, FK5 3172, HIP 72567, HR 5534, SAO 83553
F9IV-V 0.97 M☉ 59.4 ly

Psi Velorum
ψ Vel, CD−39°5580, GJ 351, Gliese 351, HD 82434, HIP 46651, HR 3786, SAO 221234, WDS J09307-4028AB
F0 IV 1.4 M☉ 59.7 ly

Psi Velorum B
F3 IV - 60.1 ly

Xi Geminorum
31 Geminorum, HR 2484, HD 48737, BD+13°1396, FK5 256, HIP 32362, SAO 96074, ksi Gem, ksi Geminorum, ξ Gem, Al Zirr, Alzirr,
F5IV-V 1.7 M☉ 60.2 ly

HD 78366
GJ 334.2, GJ 334.2, HR 3625, TIC 355127594, TYC 2495-846-1, HIP 44897
G0IV-V - 61.8 ly

110 Herculis
BD+20° 3926, FK5 703, Gliese 9635, GJ 9635, HD 173667, HIP 92043, HR 7061, SAO 86406, 110 Her
F5.5IV-V - 63.1 ly

Tau Cygni
τ Cygni, 65 Cygni, BD+37°4240, HD 202444, HIP 104887, HR 8130, SAO 71121, GC 29723, CCDM J21148+3803AB, GJ 822.1, Gliese 822.1
F2IV 1.7 M☉ 65.8 ly

HD 212330
CP-58 7954,SAO 247441,HR 8531
G2IV-V - 66.3 ly

V2213 Ophiuchi
V2213 Oph, HD 154417, Gliese 9583, GJ 9583, GJ 654.1, HIP 83601, HR 6349, 2MASS J17051682+0042090, TIC 297236135, TYC 398-1908-1, LSPM J1705+0042, LTT 15050
F8.5IV-V - 67.2 ly

V* TX Ps
GJ 871.1 B, Gliese 871.1 B, 2MASS J22450004-3315258, TIC 206605715
M5IVe - 68 ly

V* WW Ps
GJ 871.1 A, L 574-62, TIC 206605718, TYC 7501-987-1
M4IVe - 68.1 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.
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