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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 161-180
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Nombre de la estrella Mass Distance

HD 26913
G8V - 72 ly

HD 97343
CD-25 8519, LTT 4131, HIP 54704
G8.5V - 72.1 ly

HD 98281
Gl 423.1, Gliese 423.1, HIP 55210, BD-4 3049
G8V - 72.2 ly

Mu2 Cygni
HD 206827, HR 8310, SAO 89939
G2V 0.99 M☉ 72.2 ly

HD 205536
G9V - 72.5 ly

HD 32778
G7VFe-1.4CH-1.2 - 72.8 ly

HD 145825
G3V 1 M☉ 72.9 ly

BD+01 2063
G5V - 73 ly

HD 14214
HIC 10723, NLTT 7585, TYC 38-1343-1, AG +01 242, HIP 10723, PLX 473, UBV M 8857, ASCC 1097722, HR 672, PMC 90-93 698, UBV 2359, BD +01 410, IRAS 02154+0131, PM 02154+0131, USNO -B1.0 0917-00023340, Ci 20 164, LFT 202, PPM 145462, uvby98 100014214, CSI +01 410 1, LHS 1382, SAO 110456, YZ 0 2751, FK5 1061, LSPM J0218+0145, SBC7 83, YZ 1 460, GC 2770, LTT 10783, SBC9 118, GCRV 1281, 2MASS J02180145+0145282, N30 470, TD1 1343
G1V 1.2 M☉ 73.1 ly

HD 4915
G5V - 73.1 ly

HD 88742
G0V - 73.2 ly

HD 59468
CD-51 2507, Gl 275, Gliese 275, HIP 36210
G6.5V - 73.3 ly

HD 210667
G9V - 73.3 ly

Sigma Coronae Borealis Ba
G1V 1.1 M☉ 73.9 ly

HD 97334
GJ 417, Gliese 417, BD+36◦2162
G0 V - 74 ly

HD 222143
BD+45 4288,SAO 53210,HD 222143,HR 8964
G2 - 74.4 ly

HD 75767
G1.5V - 74.9 ly

HD 149612
G5VFe-1.2CH-0.9 - 75.4 ly

HD 131923
G4V - 75.5 ly

HD 39855
** GAN 2A, ADS 4503 A, BD-19 1297, GSC 05939-02257, HIC 27922, HIP 27922, 2MASS J05543015-1942156, TIC 160301040, TYC 5939-2257-1, WDS J05545-1942A
G8VFe-0.7 C 0.87 M☉ 75.9 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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