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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 581-600
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Nombre de la estrella Mass Distance

TOI-4079 B
1.1 M☉ 1186 ly

TOI 6016
TIC 327369524
1.3 M☉ 1186 ly

TOI 2533
TYC 2010-124-1, TIC 418012030, 2MASS J14103331+2625241
F8 1.1 M☉ 1205 ly

HD 34736
- 1215 ly

HD 34736 B
- 1215 ly

TOI 4776
TIC 196286578
- 1222 ly

WASP 193
1SWASPJ105723.88-295949.6, TIC 49043968, 2MASS ID 10572385-2959497
F9V 1 M☉ 1232 ly

TOI 2580
TYC 4076-01264-1
1.3 M☉ 1236 ly

WASP 120
F5 1.4 M☉ 1248 ly

TOI-7701
, Gaia DR3 5064022838647963008, TIC 122522333
- 1253 ly

TOI 5110
1.5 M☉ 1266 ly

WASP 31
1.2 M☉ 1266 ly

AE Aurigae
AE Aurigae, AG 34°542, BD 34°980, GC 6429, HD 34078, HIP 24575, HR 1712, SAO 57816, AE Aurigae, AG 34°542, BD 34°980, GC 6429, HD 34078, HIP 24575, HR 1712, SAO 57816
O9.5V 19.2 M☉ 1267 ly

TOI 5153
F8V 1.2 M☉ 1273 ly

TOI 3023
TIC 454248975, 2MASS 11011602-7221246, WISE J110115.86-722124.2, Gaia DR3 5227928170880093568, UCAC4 089-025477
- 1273 ly

TOI 2485
TIC 328934463, TYC 1998-674-1, 2MASS J13404904+2259024, TYC 1998-674-1
1.6 M☉ 1296 ly

TOI 6752
TIC 87422071, TYC 7912-829-1, 2MASS J18120831-4414359, Gaia DR3 6721152093391972480
1.2 M☉ 1302 ly

V1247 Orionis
- 1309 ly

WASP 17
F4 1.2 M☉ 1315 ly

TOI 375
TIC 280097543, 2MASS J03083602-7722598, TYC 9366-00188-1, WISE J030835.98-772259.8
1.4 M☉ 1316 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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