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Étoiles massives de la séquence principale
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Lista de Étoiles massives de la séquence principale

        
    
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Estrellas 441-460
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Nombre de la estrella Mass Distance

HD 23514
1.3 M☉ 456 ly

HD 28109
TIC 29781292, TOI-282, 2MASS J04205712-6806095, UCAC4 110-003794, WISE J042057.17-680609.5, Gaia DR2 4668163021600295552, HIP 20295, TYC 9154-01248-1
F8/G0V 1.3 M☉ 459 ly

TOI 677
1.2 M☉ 463 ly

Omega Fornacis
ω For, CD–28°819, HD 16046, HIC 11918, HIP 11918, HR 749, SAO 167882, CCDM J02338-2814AB, WDS J02338-2814
B9V 3.4 M☉ 466 ly

Omega Fornacis B
A3V 2.2 M☉ 466 ly

HR 5907
HD 142184
B2.5V 5.5 M☉ 467 ly

Omega1 Scorpii
Jabhat al Akrab, ω1 Sco, 9 Scorpii, BD−20°4405, HD 144470, HIP 78933, HR 5993, SAO 184123
B1V 11.4 M☉ 471 ly

HD 74438
Gaia EDR3 5318498001679049728
A5 1.7 M☉ 472 ly

HD 74438 B
A9 1.5 M☉ 472 ly

Tau Scorpii
Paikauhale, Alniyat, Al Niyat, τ Sco, 23 Sco, FK5 620, GC 22303, HD 149438, HIC 81266, HIP 81266, HR 6165, SAO 184481
B0.2 V 15 M☉ 474 ly

TOI 1153
1.6 M☉ 475 ly

HIP 81208
B9V 2.6 M☉ 477 ly

HD 142666
Gaia DR3 6243489715051060480, 2MASS J15564002-2201400, TIC 220764844, TYC 6199-618-1, V1026 Sco, WISEA J155640.01-220140.0, PDS 76
F0V_sh B 2 M☉ 477 ly

HD 69962
HIP 40860, TYC 1932-1517-1, TIC 302187609, 2MASS J08201753+2529483
F5 E - 481 ly

HD 36968
F2V - 485 ly

CQ Tauri
F2 1.5 M☉ 487 ly

WASP-74
- 488 ly

HD 201033
TOI-1431, TIC 375506058, TYC 3956-803-1, HIC 104051, HIP 104051, MASCARA-5, 2MASS J21044887+5535166, Renson 56060, SAO 33117, YZ 55 6891
Am C 1.9 M☉ 488 ly

HIP 33609
Gaia DR3 5557593814516968960, TOI-588, TIC 130415266, HD 52470, TYC 8122-01924-1, 2MASS J06585996-4701240
2.4 M☉ 495 ly

HD 131488
1.9 M☉ 497 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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