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Estrellas similares al sol
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Lista de Estrellas similares al sol

        
    
Más sobre Estrellas de tipo solar
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Estrellas 261-280
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Nombre de la estrella Mass Distance

HD 96064
TYC 4924-1114-1, USNO-A2 0825-07378630, HIP 54155
G8V - 85.8 ly

HD 204521
BD+69°1169, GJ 4194, Gliese 4194, HIP 105766, SAO 10045, TYC 4465-1133-1
G0V Fe-0.8 1 M☉ 86 ly

HD 225261
G9V - 86 ly

V450 Andromedae
V* V450 And
G5V - 86.1 ly

HD 114260
G8V - 86.2 ly

V966 Cassiopeiae
V966 Cas
G5V - 86.2 ly

HD 3821
G1V - 86.3 ly

HD 117635
TYC 4966-99-1, USNO-A2 0825-08025798, HIP 65982
G8V - 86.4 ly

VW Cephei
VW Cep, LHS 3565, SAO 9828, LTT 16039, BD+75 752, GJ 9703, Gliese 9703, HD 197433, HIP 101750
G8V - 86.6 ly

HD 175726
G0V - 86.7 ly

HD 47127
LTT 11882, HIC 31660, HIP 31660, 2MASS J06373390+1210505, NLTT 16752, TIC 307943195, TYC 741-1283-1, WDS J06376+1211A, Gaia DR2 3352152743956693376
G5 E 1 M☉ 86.8 ly

HD 122676
Hip 68634, SAO 100829, BD+15 2658
G7V - 86.9 ly

HD 143291
G9V - 86.9 ly

Rho Indi
ρ Ind, CPD–70° 2971, FK5 865, HR 8701, HD 216437, HIC 113137, HIP 113137, SAO 258084, 2MASS J22543949-7004254, TIC 277774779, TYC 9340-1818-1
G1VFe+0.3 C 1.3 M☉ 87.1 ly

HD 32850
TYC 710-98-1, USNO-A2 0975-01349902, HIP 23786
G9V - 87.1 ly

LZ Ursae Majoris
V* LZ UMa
G5V - 87.2 ly

HD 18144
G8V - 87.4 ly

HD 108309
G2V - 87.6 ly

HD 161612
TYC 7385-524-1, USNO-A2 0525-29583965, HIP 87116
G8V - 87.7 ly

HD 48938
LTT 2639, HD 48938, PLX 1580, UBV 6713, CD -27 3248, HIC 32322, PPM 250932, UBV M 12414, CPD -27 1448, HIP 32322, SAO 172264, uvby98 100048938, GC 8831, HR 2493, YZ 117 3241, GCRV 57986, IRAS 06428-2717, SPOCS 321, 2MASS J06445195-2720302, SRS 7272, GJ 243, Gliese 243, NLTT 16949, TD1 8032
G0VFe-0.8CH-0.5 1.1 M☉ 87.7 ly
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Estrellas de tipo solar noticias

Granulation patterns in LTT 9779 and WASP 121 revealed by JWST
iconToday
iconEstrellas | Exoplanetas | Estrellas de tipo solar | Telescopio espacial 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
iconEstrellas | Exoplanetas | Estrellas de tipo solar | Júpiter caliente | Formación planetari
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
iconEstrellas | Exoplanetas | Estrellas de tipo solar | Júpiter caliente | Atmósferas planetari
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 Estrellas similares al sol

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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: Estrellas

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Estrellas
Las estrellas son enormes esferas de gas caliente que brillan al generar energía mediante fusión nuclear en sus núcleos. La mayoría de las estrellas están compuestas principalmente de hidrógeno y helio. En el centro de una estrella, la alta presión y temperatura hacen que los átomos de hidrógeno se fusionen en helio, liberando una enorme cantidad de energía en forma de luz y calor.
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