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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 521-540
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Nombre de la estrella Mass Distance

WASP 121
TYC 7630-352-1, Gaia 5565050251402363648, 2MASS J07102406-3905506, 1SWASP J071024.05-390550.5, CD-38 3220, TIC 22529346, TOI-495, Gaia EDR3 5565050255701441664
F6V C 1.4 M☉ 858 ly

Rigel Ba
B9V 3.8 M☉ 860 ly

Rigel Bb
B9V 2.9 M☉ 860 ly

Rigel C
B9V 3.8 M☉ 860 ly

TOI 4406
2MASS J01121157-5655316, TYC 8477-00008-1
1.2 M☉ 861 ly

TOI 6019
TIC 125520907
1.1 M☉ 862 ly

NGTS-38
TYC 6536-3043-1, 2MASS J07145152-2925498, Gaia 5606317297918628992, TIC 65910228
1.5 M☉ 872 ly

HD 56414
TOI 1228, TIC 300038935, 2MASS J07112249−6850006, Gaia DR2 5268547016621360768
A 1.9 M☉ 873 ly

42 Orionis
c Orionis, BD-04°1185, CCDM J05354-0450AB, GC 6934, HIC 26237, HIP 26237, HR 1892, HD 37018, NSV 2318, SAO 132320, WDS J05354-0450AB
B1V 12 M☉ 884 ly

TOI 1251
1.1 M☉ 892 ly

TOI 3364
TIC 280655495, 2MASS 09380910-4920069, Tycho-2 8176-00923-1, WISE J093809.09-492006.7
1.2 M☉ 899 ly

Delta Cephei B
B7-8 0 M☉ 917 ly

Delta Cephei Cb
F0V 1.6 M☉ 917 ly

TOI 1107
TIC 394561119, 2MASS J10222579-8213080
1.4 M☉ 924 ly

WASP-186
1.2 M☉ 925 ly

TOI 2497
TIC 97568467, TYC 0725-01745-1, 2MASS J06001500+1153030
1.9 M☉ 930 ly

TOI 329
1.1 M☉ 932 ly

HAT-P-32
GSC 3281-00800, 2MASS J02041028+464116
1.2 M☉ 934 ly

WASP-15
F7 - 935 ly

TOI 2046
TIC 468574941
F8V 1.2 M☉ 940 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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