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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 661-680
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Nombre de la estrella Mass Distance

HD 135160 Ba
- 2676 ly

HD 135160 Bb
- 2676 ly

TOI 7081
TOI-7081
F8V 1.1 M☉ 2729 ly

HATS 26
2MASS 09394244-2835081, GSC 6614-01083, Gaia DR3 5656896924435896832
1.3 M☉ 2729 ly

TYC 150-392-1
kA3hF2mF3Eu C - 2756 ly

TIC 235934420
- 2769 ly

TIC 235934420 B
- 2769 ly

HATS-31
Gaia DR3 3498553232585634816
1.3 M☉ 2845 ly

Upsilon Orionis
υ Ori, 36 Orionis, HD 36512, HIC 25923, HIP 25923, HR 1855, SAO 132222, BD−07° 1106, Thabit, Tabit
O9.7 V 20 M☉ 2861 ly

UCAC4 558-030081
WISE J063103.27+213114.7, Gaia DR2 3376154975413069952, 2MASS J06310327+2131147, WISE J063103.27+213114.7
- 2872 ly

TIC 457579488
- 2901 ly

TOI 1480
1.4 M☉ 2925 ly

TYC 754-1161-1
2MASS J06431451+1123090, GSC 00754-01161
A2V D - 3069 ly

CoRoT-36
Gaia EDR3 4477340334766250496, 2MASS J18310024+0711001
F3 V 1.3 M☉ 3200 ly

HD 45166
B7 V 3.4 M☉ 3276 ly

NGTS 23
2MASS J04414374-4002404, TIC 77287067
F9V 1 M☉ 3433 ly

Kepler 1790
1.2 M☉ 3490 ly

HD 331986
- 3551 ly

TOI 5301
TIC 58825110
1.5 M☉ 3651 ly

HD 228777 Aa
CzeV4315, TIC 12248375
B9 - 3652 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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