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Liste des Des étoiles semblables au soleil

        
    
Plus à propos Étoiles de type solaire
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Etoile 141-160
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Nom de l étoile Mass Distance

HD 220182
GJ 9823, Gliese 9823, G 216-42, G 190-20, WISEA J232137.16+440554.8, 2MASS J23213644+4405520, HIP 115331
G9V - 69.9 ly

HD 199288
HIP 103458, GJ 9712, Gliese 9712, LHS 503
G2VFe-1.0 0.82 M☉ 70 ly

HD 68017
G3V 0.93 M☉ 70.4 ly

HD 144287
G8+V - 70.5 ly

HD 116956
G9V - 70.6 ly

HD 159062
G9V_Fe-0.8 0.76 M☉ 70.6 ly

HD 197214
G6V - 70.8 ly

HD 24409
GC 4713, GJ 3257, Gliese 3257, 2MASS J03561156+5938309, TYC 3729-1086-1, HIP 18413, LSPM J0356+5938
G3V - 70.9 ly

HD 59967
G3V - 70.9 ly

HD 210918
TYC 7999-1575-1, HIP 109821, HR 8477, Gliese 851.2, GJ 9774, Gliese 9774
G2V - 71 ly

HD 124292
G8/K0V - 71.1 ly

Pi1 Ursae Minoris B
BD+80°481, HD 139813, HIP 75829, SAO 2558
G9V 0.92 M☉ 71.1 ly

Pi1 Ursae Minoris
π1 UMi, ADS 9696, WDS J15292+8027, BD+80°480, HD 139777, HIP 75809, HR 5829, SAO 2556, * pi.01 UMi A
G1.5V(n) 1 M☉ 71.1 ly

HD 195987
G9V - 71.3 ly

HD 48189
G1/2V - 71.4 ly

HD 45184
LTT 2547, HD 45184, SAO 171711, UCAC3 123-24555, CD-28 2981, HIC 30503, SKY# 10971, uvby98 100045184, CPD-28 1279, HIP 30503, SPOCS 311, WISEA J062443.79-284649.6, DENIS J062443.8-284648, HR 2318, TD1 7076, YZ 118 2962, GC 8299, IRAS 06227-2845, TIC 49831913, Gaia DR1 2898239464575224320, GEN# +1.00045184, 2MASS J06244387-2846483, TYC 6518-2342-1, Gaia DR2 2898239468873596800, GJ 3394, Gliese 3394, NLTT 16502, UBV 6421, GSC 06518-02342, PPM 250356, UBV M 12080
G2Va 1 M☉ 71.4 ly

HD 71148
TYC 3415-2484-1, HIP 41484, HR 3309, BD+46 1398, Gliese 307.1
G1V - 71.6 ly

Gamma Antliae
CD–29° 8316, GJ 3597, Gliese 3597, HIC 50921, HIP 50921, PPM 257610, SAO 178771, HD 90156, LTT 3817, 2MASS J10235528-2938441, TIC 193032655, TYC 6631-431-1, WISEA J102355.24-293842.8
G5V C 0.99 M☉ 71.6 ly

HD 164922
BD +26°3151, Gliese 700.2, GJ 700.2, Gliese 9613, GJ 9613, LFT 1388, SAO 85678, HIC 88348, HIP 88348, 2MASS J18023085+2618471, LHS 3353, WISEA J180231.16+261840.6, TIC 159019691, TYC 2099-2717-1
G9V C 0.87 M☉ 71.7 ly

HD 4308
BD−27°223, GC 897, GJ 31.5, Gliese 31.5, GJ 9028, Gliese 9028, HD 4308, HIC 3497, HIP 3497, SAO 248244, PPM 352003, LFT 71, LHS 1139, LPM 40, LTT 416, TYC 8847-598-1, GCRV 50662, 2MASS J00443925-6538581, TIC 234501204, WISEA J004439.51-653905.9
G6VFe-0.9 C 0.95 M☉ 71.9 ly
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Étoiles de type solaire nouvelles

Thick-disk stars identified as hosts to ancient hot jupiter planets
icon16. 10. 2026
iconÉtoiles | Exoplanètes | Étoiles de type solaire | Jupiter chaud | Formation des planète
Image: Thick-disk stars identified as hosts to ancient hot jupiter planets
Large gas giant planets that orbit very close to their parent stars are known as hot Jupiters. By analyzing a sample of 268 stars, researchers have identified several hot Jupiters orbiting stars belonging to the high-alpha thick disk of our galaxy. The thick disk represents a component of the Milky Way containing older stars with specific chemical signatures, particularly higher amounts of alpha elements like magnesium, silicon, and calcium relative to iron. These systems are significantly older...
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Atmospheric differences between morning and evening sides of planet WASP-39 b revealed
icon12. 10. 2026
iconÉtoiles | Exoplanètes | Étoiles de type solaire | Jupiter chaud | Atmosphères planétaire
Image: Atmospheric differences between morning and evening sides of planet WASP-39 b revealed
Observations of the hot Jupiter WASP-39 b reveal significant differences between its morning and evening atmospheres. Climate models successfully match temperature patterns but still struggle to explain the observed asymmetry in carbon dioxide levels....
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Water vapor detected in the atmosphere of ultrahot Neptune LTT 9779 b
icon9. 10. 2026
iconÉtoiles | Exoplanètes | Étoiles de type solaire | Atmosphères planétaire
Image: Water vapor detected in the atmosphere of ultrahot Neptune LTT 9779 b
New observations of the ultrahot Neptune LTT 9779 b reveal the presence of water vapor on its dayside. The planet shows no signs of thermal inversion or significant atmospheric escape, supporting the theory that it is a tidally locked world....
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study iconResearch in Des étoiles semblables au soleil

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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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