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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 221-240
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Nombre de la estrella Mass Distance

HD 34721
HIP 24786, HR 1747, TYC 5906-910-1, USNO-A2 0675-01998636
G0V - 80.6 ly

HD 113283
TYC 9516-1604-1, HIP 64690
G5V - 80.6 ly

HD 12051
G9V - 80.6 ly

HD 1562
G1V - 80.7 ly

HD 105590
G4+K5 - 80.9 ly

HD 191499
G9V - 80.9 ly

HD 51419
TYC 1356-1547-1, USNO-A2 1050-04603306, HIP 33537
G5VFe-1 - 81 ly

HD 114853
G1.5V - 81.6 ly

HD 105631
G7V - 81.7 ly

HD 181655
G5V - 81.9 ly

HD 215500
TYC 4273-505-1, USNO-A2 1500-09278232, HIP 112245
G8V - 82 ly

HD 218687
TYC 1167-1661-1, USNO-A2 0975-21198176, HIP 114378
G0V - 82 ly

HD 115043
TYC 3846-925-1, USNO-A2 1425-07923010, HIC 64532, HIP 64532, BD+57 1425, GJ 503.2, GJ 9434, Gliese 9434, 2MASS J13133699+5642298, TIC 157272202, TYC 3846-925-1, Gaia DR2 1566224665609504128, Allady
G1Va - 82.1 ly

HD 223913
CD-66 2653
G0V - 82.4 ly

HD 3823
HR 176, HIP 3170, GJ 29, Gliese 29, SAO 232143, CD-60 118, LHS 1123
G0VFe-0.9CH-0.4 1 M☉ 82.4 ly

BD+49 2959
HD 179958, LHS 3441, GJ 9648 A, Gliese 9648 A, 2MASS J19120500+4951207, WISE J191204.80+495127.1
G2V - 82.4 ly

BD+49 2959 B
HD 179957, GJ 9648 B, Gliese 9648 B, 2MASS J19120467+4951141, WISE J191204.47+495120.4
G3V - 82.4 ly

78 Ursae Majoris B
TYC 3845-1189-2
G6V - 82.6 ly

HD 96700
CD−29° 8875, Gliese 9346, GJ 9346, Gliese 412.2, GJ 412.2, HD 96700, HIC 54400, HIP 54400, HR 4328, SAO 179558, LHS 2354, DENIS J110754.4-301028, GC 15311, LFT 763, LTT 4098, NLTT 26384, 2MASS J11075444-3010284, TIC 23270430, TYC 7201-619-1, WISEA J110754.00-301030.0
G1VFe-0.5 C 0.96 M☉ 82.8 ly

HD 76218
HIP 43852, 2MASS J08555568+3611464, TYC 2491-1201-1, TIC 188503588
G5V - 82.8 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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