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Étoiles massives de la séquence principale
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Lista de Étoiles massives de la séquence principale

        
    
Más sobre Estrellas masivas de la secuencia principal
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Estrellas 541-560
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Nombre de la estrella Mass Distance

HAT-P-57
2MASS 18185842+103
1.5 M☉ 950 ly

HD 99837
HIP 56025, TIC 452712793, 2MASS J11285863-2446009, WISE J112858.63-244601.0
A0V - 957 ly

TOI-2154
1.2 M☉ 967 ly

TOI 2529
TIC 269333648
1.1 M☉ 972 ly

TOI 4373
TIC 315350812
- 985 ly

TOI 2152
TIC 395393265, TYC 4498-01400-1, 2MASS J01452120+7747244
F4V 1.5 M☉ 988 ly

Kepler 100
KOI-41, 2MASS J19253263+4159249, KIC 6521045, WISE J192532.66+415924.6
1.1 M☉ 1001 ly

K2-237
2MASS J16550453-2842380, EPIC 229426032
F9V 1.2 M☉ 1002 ly

TOI 1181
TIC 229510866
F9IV 1.4 M☉ 1013 ly

HD 181793
Am 1.6 M☉ 1022 ly

TIC 245076932
TIC 245076932, TYC 8259-1806-1, 2MASS J13121527-5112519, Gaia DR3 6080787214190400384
1.1 M☉ 1026 ly

HD 99837 B
- 1028 ly

KELT-18
1.5 M☉ 1032 ly

HAT-P-70
TOI 624
1.9 M☉ 1038 ly

HAT-P-29
TOI-6028
F8V 1.2 M☉ 1040 ly

TOI 4791
TIC 100389539, 2MASS 07173322-1949443, TYC 5973-02018-1, WISE J071733.21-194944.2
1.2 M☉ 1051 ly

EPIC 249893012
1.1 M☉ 1054 ly

TOI 3837
TYC 1968-371-1, 2MASS J10103984+2416239, TIC 308073360
0.89 M☉ 1060 ly

TOI 4127
TIC 141488193, 2MASS J07013709+7224538
1.2 M☉ 1061 ly

Omicron Persei Ab
B2V 10 M☉ 1079 ly
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Estrellas masivas de la secuencia principal noticias

Lambda Bootis phenomenon identified in the massive early B-type star HD 37356
icon10. 8. 2026
iconEstrellas | Estrellas masivas de la secuencia princi
Image: Lambda Bootis phenomenon identified in the massive early B-type star HD 37356
The Lambda Bootis phenomenon is a unique chemical condition in stars where certain elements, known as refractory elements (materials that condense at high temperatures, such as iron), are significantly less abundant than expected, while volatile elements remain at normal levels. This feature has now been identified in the massive early B-type star HD 37356, marking the first time this characteristic has been observed in such a massive stellar object. Researchers analyzed high-quality spectra ...
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Circumstellar disks observed around five massive Herbig Be stars
icon24. 6. 2026
iconEstrellas | Estrellas masivas de la secuencia principal | Formación planetari
Image: Circumstellar disks observed around five massive Herbig Be stars
A survey of 24 massive Herbig Be stars identifies circumstellar disks around 5 of them. These disks contain enough material to potentially form giant planets, following scaling laws similar to those seen in lower-mass young stars....
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HD 48914 binary system characteristics measured via photometric and radial velocity data
icon20. 6. 2026
iconEstrellas | Estrellas masivas de la secuencia princi
Image: HD 48914 binary system characteristics measured via photometric and radial velocity data
HD 48914 is an eclipsing binary system where the Be-shell star spins at its physical limit of 467 km/s. New data from TESS reveals a large surrounding gas disk and confirms the companion star was previously stripped of its mass through intense stellar interaction....
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study iconResearch in Étoiles massives de la séquence principale

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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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