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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 601-620
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Nombre de la estrella Mass Distance

TOI 1338
BEBOP-1, EBLM J0608-59
F9V 1.1 M☉ 1318 ly

TOI 558
- 1326 ly

WASP 167
KELT-13, TOI-748, TIC 104024556, 2MASS J13041053-3532582
F1V 1.5 M☉ 1346 ly

WASP 12
TYC 1891-1178-1, 2MASS J06303279+2940202, UCAC2 42216354
1.4 M☉ 1347 ly

HD 57372
B8p Si - 1352 ly

HD 37061 Aa
B1V 16.4 M☉ 1356 ly

HD 37061 Ab
4.4 M☉ 1356 ly

HD 37061 B
3.8 M☉ 1356 ly

HD 37061 C
8.1 M☉ 1356 ly

TOI 1406
1.2 M☉ 1381 ly

KELT-25
CD-24 5016, TIC 65412605, TYC 6528-1639-1, TOI 626
A 2.2 M☉ 1393 ly

HD 188101
B9 4.1 M☉ 1394 ly

TOI 3807
- 1402 ly

TOI 6442
2MASS J07112000-3551019, NGTS-33
A9V 1.6 M☉ 1442 ly

TOI 7041
TIC 201175570
1.1 M☉ 1443 ly

TOI 2420
TIC 268532343
- 1450 ly

KELT 16
TYC 2688-1839-1, 2MASS J20570443+3139397
F7V 1.2 M☉ 1451 ly

KIC 8462852
TYC 3162-665-1, Tabbys star, Boyajians Star, WISE J200615.45+442724.7, KIC 8462852, NSVS 5711291, Gaia DR2 2081900940499099136, 2MASS J20061546+4427248, UCAC4 673-083862
F3V 1.4 M☉ 1470 ly

TOI-7169
TIC 372048733
- 1478 ly

HD 87304
CD-33 6615 A
A8V kA2.5mA2.5 - 1480 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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