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Liste des Des étoiles semblables au soleil

        
    
Plus à propos Étoiles de type solaire
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Etoile 361-380
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Nom de l étoile Mass Distance

HD 178076
29 Ari, BD+14°419, FK5 2176, GJ 3161, HD 15814, HIP 11843, HR 741, SAO 92998, WDS J02329+1502
G8V 1.1 M☉ 95.2 ly

HD 219077
CD−63°1596, HD 219077, HIC 114699, HIP 114699, HR 8829, LHS 3912, LFT 1769, LTT 9415, 2MASS J23140661-6242002, NLTT 56181, SAO 255435, TIC 394125166, TYC 9128-1083-1, WISEA J231407.33-624204.3
G8V+ C 1.1 M☉ 95.2 ly

HD 15096
G5 0.85 M☉ 95.4 ly

HD 208906
TYC 2215-517-1, USNO-A2 1125-18964513, HIP 108490
G0VmF2 - 95.4 ly

HD 58781
G5 - 95.5 ly

HD 3277
G8V - 95.5 ly

29 Arietis B
G5V 0.88 M☉ 95.5 ly

HD 70642
CD−39°4247, GJ 304, Gliese 304, HIC 40952, HIP 40952, SAO 199126, LTT 3116, GC 11411, 2MASS J08212815-3942199, TIC 183356952, TYC 7665-696-1, WISEA J082127.93-394217.3
G6VCN+0.5 C 1 M☉ 95.5 ly

HD 71974
G5V - 95.7 ly

HD 96937
Gliese 3644, GJ 3644, HD 96937, HIP 54541, TYC 262-70-1, 2MASS J11094022+0227223
G8V - 95.8 ly

HD 1273
G5VFe-1.2CH-0.9 - 95.9 ly

HD 19632
G5V - 96.1 ly

BD+32 4747
HD 224635
G1 - 96.1 ly

38 Geminorum B
G6V 0.89 M☉ 96.2 ly

BD+32 4747 B
HD 224636
G8 - 96.2 ly

HD 46090
G3/5V - 96.2 ly

HD 46375
BD+05°1295, HIC 31246, HIP 31246, SAO 114040, SLE 299A, CoRoT 1889, 2MASS J06331263+0527464, TIC 234928947, TYC 154-891-1, WDS J06332+0528A
G9V C 0.92 M☉ 96.3 ly

HD 22468 B
HD 22468, HD 22468
G5V 0.6 M☉ 96.3 ly

HD 33636
G0V_CH-0.3 - 96.5 ly

HD 35956
TYC 708-525-1, USNO-A2 0975-01637058, HIP 25662
G0V - 96.5 ly
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Étoiles de type solaire nouvelles

Granulation patterns in LTT 9779 and WASP 121 revealed by JWST
iconToday
iconÉtoiles | Exoplanètes | Étoiles de type solaire | Télescope spatial James Webb
Image: Granulation patterns in LTT 9779 and WASP 121 revealed by JWST
Stars are not perfectly static spheres of light. Their surfaces are covered in granulation, a boiling pattern caused by heat rising from deep within the star and cooling as it reaches the surface. These granules appear as bright, shifting cells that create constant, tiny flickers in a star's brightness. Understanding these rapid fluctuations is essential because they can mimic or mask the faint signals of orbiting planets. By analyzing high-precision data from the JWST, researchers measured t...
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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
New analysis of 268 stars identifies several hot Jupiters orbiting ancient stars in the Milky Way's thick disk. These systems, over 8 billion years old, show distinct differences in mass and orbital periods compared to younger thin-disk populations....
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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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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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