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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 561-580
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Nombre de la estrella Mass Distance

Omicron Persei B
- 1079 ly

TOI 2005
TIC 147660886, 2MASS J10560763-4322362, TYC 7736-00803-1
1.6 M☉ 1091 ly

TOI-791
TIC 306472057, 2MASS J07534434-6942063, APASS 33130674, Gaia DR2 5270467966514084224, TYC 9184-01675-1, UCAC4 102-020935, WISE J075344.34-694206.2
F7 1.3 M☉ 1097 ly

TIC 241249530
1.3 M☉ 1103 ly

TOI 640
1.5 M☉ 1106 ly

TOI 2641
TIC 162802770, 2MASS J11243133-4243555
F9V 1.2 M☉ 1131 ly

TOI 4562
TIC 349576261,
F7V 1.2 M☉ 1131 ly

TOI 159
TOI-159
F1V 1.7 M☉ 1137 ly

TOI 4386
TIC 350575997, HD 147541, 2MASS J16262913-6327282, TYC 9041-3481-1
A4/6IV/V E - 1138 ly

HAT-P-41
GSC 0488-02442, 2MASS 19491743+0440207
1.4 M☉ 1145 ly

TOI 2236
TIC 394722182, 2MASS 01203986-8658476, TYC 9498-00283-1, WISE J012039.88-865847.8
- 1150 ly

TOI 5422
TIC 80611440
1.1 M☉ 1153 ly

TOI-333
2MASS J23332579-4110174, TIC 224245334
F7V 1.2 M☉ 1155 ly

TOI 615
2MASS ID J08533810-4032376
F2V 1.4 M☉ 1155 ly

HD 200775
B3 10.7 M☉ 1158 ly

HD 200775 B
9.3 M☉ 1158 ly

HD 36030
TYC 105-1954-1, USNO-A2 0900-01680686
B9V - 1163 ly

NGTS-2
WASP-179, TYC 7282-1298-1
F5V 1.6 M☉ 1175 ly

TOI 2570
TIC 239816546, GAIA EDR3 3445148131761842944, 2MASS 05484513+3205028, WISE J054845.12+320502.6
- 1180 ly

TOI-4079
F8V - 1186 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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