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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 481-500
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Nombre de la estrella Mass Distance

TOI 6038
TIC 194736418
1.3 M☉ 581 ly

K2-100
1.2 M☉ 596 ly

HD 201585
MASCARA-1, GC 29588, BD+10 4478, HIC 104513, HIP 104513, 2MASS J21101237+1044197, SAO 106887, TIC 354619337, TYC 1108-1313-1
A8 D 1.7 M☉ 598 ly

TOI 1143
1.5 M☉ 605 ly

HD 152564
TYC 9275-3003-1, HR 6276, HIP 83150
Ap/Bp - 625 ly

TOI-6564
TOI 6564, TIC 453668803
1.2 M☉ 631 ly

TOI 5786
2MASS J19331736+3042152
1.2 M☉ 632 ly

WASP-76
2MASS 01463185+0242019, BD+01 316, AG+02 184, SAO 110122, 1SWASP J014631.86+024202.0, TIC 293435336, TYC 32-111-1, YZ 2 503
F7 D 1.5 M☉ 637 ly

29 Persei
29 Per, BD+49°899, FK5 2188, GC 3934, HD 20365, HIC 15404, HIP 15404, HR 987, SAO 23944
B3V 6.8 M☉ 637 ly

TOI 1333
TOI-1333A
1.5 M☉ 639 ly

HD 2685
TOI-135, HIP 2268, TIC 150035071
F2V 1.4 M☉ 644 ly

WASP 101
F6 1.3 M☉ 651 ly

XO-3
TYC 3727-1064-1, GSC 03727-01064, 2MASS J04215269+5749018
F5V 1.2 M☉ 658 ly

TOI-6649
TIC 258940847, Gaia DR3 2806600569174401920
1.3 M☉ 659 ly

WASP-35
F9V 1.1 M☉ 660 ly

HD 73135
kA7 hF1 mF2 (Am) 1.8 M☉ 668 ly

KELT-9
HD 195689
A0 - 676 ly

HAT-P-30
WASP-51, GSC 0208-00722
1.2 M☉ 679 ly

WASP 94
WASP-94A, TOI-107, CD-34 14724, HJ 5234, TYC 7466-1400-1, WISE J205507.96-340808.3, 2MASS J20550794-3408079
F8 1.5 M☉ 687 ly

TOI 6651
TIC 174328045, TYC 2286-515-1, 2MASS J01030925+3523208
1.3 M☉ 690 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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