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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 641-660
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Nombre de la estrella Mass Distance

TOI 2583
TIC 7548817, 2MASS 18090407+4520127, WISE J180904.08+452012.7
1.2 M☉ 1831 ly

UCAC2 45176266
- 1879 ly

2MASS J1252+2640
GPM 193.008944+26.673958, 2MASS J12520212+2640262, TIC 156514476
1.1 M☉ 1883 ly

NGTS-9
TOI-1935
F8V 1.3 M☉ 1963 ly

TOI-6443
TIC 125563127, TYC 6543-2384-1, 2MASS J07393705-2527556
F0V 1.7 M☉ 2052 ly

UCAC3 253-304972
Qatar-3
1.1 M☉ 2062 ly

Kepler-1768
2MASS J19594973+4446187, KIC 8651389, SPOCS 3833, Gaia DR3 2076155515517119744, KOI-1754, TIC 239236731, Gaia DR2 2076155515517119744
F7V 1.2 M☉ 2064 ly

CoRoT-11
2MASS 18424494+0556156, CoRoT 105833549, Gaia DR3 4285511294172309504
F6V 1.3 M☉ 2126 ly

Kepler 511
2MASS J18514696+4734295, KIC 10386922, KOI-289, WISE J185146.93+473429.7
1 M☉ 2134 ly

HATS-9
2MASS J19231442-2009587, EPIC 217671466, GSC 6305-02502, K2-142, WISE J192314.43-200958.9
1.1 M☉ 2196 ly

V356 Sagittarii
V356 Sgr, BD−20°5268, GC 25739, HD 173787, HIP 92235, SAO 187294, PPM 268914
B3V 11 M☉ 2206 ly

TYC 3801-1529-1
2.1 M☉ 2301 ly

HD 698
V742 Cas
7.5 M☉ 2309 ly

TOI-4034
TOI-4034, TIC 375654303
1.2 M☉ 2498 ly

TIC 400799224
Gaia EDR3 5238414793089292160, 2MASS 11095818-6645149, WISEA J110958.16-664514.8
1.8 M☉ 2566 ly

Z Canis Majoris
Z CMa, BD−11 1760, HD 53179, HIP 34042, PPM 218073, SAO 152302
Bpe 12 M☉ 2630 ly

Z Canis Majoris B
3 M☉ 2630 ly

HD 48914
V505 Mon
7.4 M☉ 2673 ly

HD 135160 Aa
- 2676 ly

HD 135160 Ab
- 2676 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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