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Liste des Des étoiles semblables au soleil

        
    
Plus à propos Étoiles de type solaire
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Etoile 181-200
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Nom de l étoile Mass Distance

HD 101177
G0V - 76 ly

HD 168009
BD+45° 2684, Gliese 9622, GJ 9622, HIC 89474, HIP 89474, HR 6847, SAO 47343, 2MASS J18153245+4512333, GJ 708.4, Gliese 708.4, TIC 416117806, TYC 3525-186-1, WISEA J181532.37+451232.3
G1V 0.99 M☉ 76 ly

HD 127334
BD+32° 2482, HD 127304, HIP 70892, HR 5422, SAO 64178
G5VCH0.3 - 76.3 ly

HD 1461
32 G. Ceti[9], BD−08°38, Gliese 16.1, GJ 16.1, HD 1461, HIP 1499, HR 72, SAO 128690, PPM 182101, LTT 149, NLTT 950, GCRV 50265, 2MASS J00184182-0803105
G3VFe0.5 C 1.1 M☉ 76.3 ly

HD 212168
CPD-75 1748 A
G0V - 76.3 ly

Omega Sagittarii
Terebellum, ψ Sgr, 58 Sagittarii, CPD−26°6880, FK5 1629, GC 27583, HD 188376, HIP 98066, HR 7597, SAO 188722, PPM 270451, ome Sgr
G5IV 1.5 M☉ 76.3 ly

Epsilon Ceti B
1 M☉ 76.8 ly

HD 218868
G8V - 76.8 ly

HD 26491
G1V - 77 ly

Alpha Coronae Borealis B
G5V 0.92 M☉ 77.2 ly

KU Librae
KU Lib
G8Vk: - 77.4 ly

HD 12846
HIP 9829, TYC 1758-1907-1
G2V - 77.4 ly

Omega Draconis B
1.2 M☉ 77.5 ly

HD 202628
G1.5V 1.1 M☉ 77.6 ly

Mu2 Cancri
* mu.02 Cnc, μ Cnc, 10 Cancri, BD+22°1862, FK5 2630, HD 67228, HIP 39780, HR 3176, SAO 79959
G1IVb 1.2 M☉ 77.7 ly

HD 45270
TYC 8894-491-1, HIP 30314
G1V - 77.9 ly

HD 130042
TYC 9019-141-1, HIP 72493, USNO-A2 0225-20993146
- 78 ly

EZ Ceti
G3V - 78 ly

12 Persei B
1.2 M☉ 78 ly

HD 185414
G0 - 78.1 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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