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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 401-420
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Nombre de la estrella Mass Distance

WASP 166
F9V 1.2 M☉ 373 ly

HD 169142
CD−29 14904, TYC 6856-876-1, GSC 06856-00876, 2MASS J18242978-2946492
A9III/IVe 1.7 M☉ 375 ly

WASP-33
HD 15082, TOI 1599
A5V 1.5 M☉ 378 ly

HD 14016
F8 - 382 ly

BD+79 230
TIC 289949453, BEBOP-3
1.1 M☉ 385 ly

HD 158485
A4V - 390 ly

HD 105186
GSC 00280-00346, TIC 376866659, YZ 0 3356, AG+00 1544, 2MASS J12064238+0016267, TOI-7475, Gaia DR3 3699014818172636288, AP J12064238+0016267, PPM 158518, TYC 280-346-1, Gaia DR2 3699014818172636288, BD+01 2652, SAO 119221
F3V 1.5 M☉ 390 ly

NGTS-34
TIC 147277741, NGTS-34
F8V 1.3 M☉ 392 ly

HIP 75056
HD 136164, 2MASS J15201339-3455316
A2V 1.7 M☉ 398 ly

TOI 622
TIC 83092282, 2MASS J08211322-4629031, Gaia DR3 5516690878153930240
F6V 1.3 M☉ 400 ly

WASP 18
HD 10069, HIP 7562, PPM 306061, SAO 215585, 2MASS J15595095-2803422, Gaia DR2 4955371367334610048, TOI 185
F6V 1.3 M☉ 400 ly

Alcyone B
24 Tauri
A0V - 403 ly

Alcyone C
- 403 ly

Alcyone D
F3V - 403 ly

TOI 422
- 405 ly

HD 31221
A2 1.4 M☉ 405 ly

TOI 2295
1.2 M☉ 410 ly

22 Scorpii
i Sco, 22 Sco, CD−24° 12695, HD 148605, HIC 80815, HIP 80815, HR 6141, SAO 184429
B3 V 6.1 M☉ 413 ly

KELT-7
1.5 M☉ 418 ly

HD 152384
A0V - 419 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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