Étoiles massives de la séquence principale

	Mass	Distance
10 Canum Venaticorum 10 CVn, BD+40°2570, GJ 484, HD 110897, HIP 62207, HR 4845, SAO 63177	F9V_Fe-0.3	0.87 M☉	57.3 ly
Gamma Coronae Australis γ CrA, CD−37° 13048, HIP 93825, SAO 210928, CCDM J19064-3704AB, HD 177474, HR 7226	F8V	1.2 M☉	57.8 ly
Gamma Coronae Australis B HD 177475, HR 7227	F8V	1.1 M☉	57.8 ly
Tau1 Hydrae τ1 Hya, 31 Hydrae, BD−02°2901, GJ 348, Gliese 348, HD 81997, HIP 46509, HR 3759, SAO 136895, WDS J09291-0246	F5V	1.2 M☉	57.9 ly
Rho Geminorum ρ Gem A, 62 Gem, BD+32° 1562, HD 58946, HIP 36366, Gliese 274A, GJ 274 A, HR 2852	F1V	1.4 M☉	58.1 ly
Alpha Comae Berenices TIC 138128530, 2MASS J13095936+1731456, GJ 501.0, Gliese 501.0, alf Com, HIP 64241, WISE J130958.97+173146.5, α Com, Alpha Com, 42 Comae Berenices, 42 Com, STF 1728, ADS 8804 , BD+18 2697, CCDM J13100+1732, GC 17833, Gliese 501, IDS 13051+1803 AB, LTT 13802, NLTT 33105, PPM 129630, SAO 100443, WDS 13100+1732	F5V	1.2 M☉	58.1 ly
Alpha Comae Berenices B HD 114379, HR 4969	F5V	1.1 M☉	58.1 ly
Iota Centauri ι Cen, CD−36°8497, FK5 496, GJ 508.1, Gliese 508.1, HD 115892, HIP 65109, HR 5028, SAO 204371	kA1.5hA3mA3Va	2.5 M☉	58.2 ly
Beta Arietis Sheratan, Sharatan, Al Sharatain, 6 Arietis, Gl 80, HR 553, BD +20°306, HD 11636, SAO 75012, FK5 66, HIP 8903, bet Ari	kA4hA5mA5Va	2.3 M☉	58.7 ly
HD 125276	F9VFe-1.5CH-0.7	-	58.7 ly
HD 46588 HR 2401, Gliese 240.1, GJ 240.1, 23 H. Camelopardalis, AG+79°200, BD+79°212, GC 8711, HD 46588, HIP 32439, SAO 5946, WDS J06462+7934A	F7V	1.1 M☉	59.4 ly
Chi Cancri χ Cnc, chi Cnc, 18 Cancri, BD+27°1589, FK5 1217, GJ 303, Gliese 303, HD 69897, HIP 40843, HR 3262, SAO 80104	F6V	1.1 M☉	59.4 ly
HD 114837	F6VFe-0.4	1.1 M☉	59.5 ly
Eta Corvi η Crv, Eta Corvi, Eta Crv, 8 Corvi, 8 Crv, BD−15°3489, GC 17087, GJ 471.2, GJ 9411, Gliese 9411, HD 109085, HIP 61174, HR 4775, LTT 4755, NLTT 31021, PPM 225971, SAO 157345	F2V	1.4 M☉	59.5 ly
212 G. Puppis 212 Pup, HIP 38423, GC 10651, CD-34 4036，SAO 198540，HD 64379，HR 3079, 2MASS J07521555-3442199, TIC 150796339, WISE J075215.48-344217.3	F5VFe-0.5	1.3 M☉	59.8 ly
Theta Cygni 13 Cyg, θ Cyg, BD+49 3062, GJ 765, Gliese 765, HD 185395, HR 7469, SAO 31815, HIP 96441	F3+V	-	60.1 ly
Tau Piscis Austrini τ PsA, 15 Piscis Austrini, CPD−33° 6227, HD 210302, HIP 109422, HR 8447, SAO 213602	F6V	1.3 M☉	60.2 ly
Delta Geminorum del gam, Wasat, 55 Geminorum, BD+22° 1645, FK5 279, Gliese 271, Gl 271, HD 56986, HIP 35550, HR 2777, SAO 79294	F2VkF0mF0	1.6 M☉	60.7 ly
HD 25457 BD-00 632，SAO 130893，HR 1249, TYC 4725-1276-1, USNO-A2 0825-00911530, HIP 18859	F7V	-	61 ly
6 Ceti 6 Cet, BD−16° 17, GJ 10, Gliese 10, HD 693, HIP 910, HR 33, SAO 147133	F8VFe-0.8CH-0.5	1.1 M☉	61.6 ly

Nombre de la estrella

Mass

Distance

10 Canum Venaticorum

10 CVn, BD+40°2570, GJ 484, HD 110897, HIP 62207, HR 4845, SAO 63177

F9V_Fe-0.3

0.87 M☉

57.3 ly

Gamma Coronae Australis

γ CrA, CD−37° 13048, HIP 93825, SAO 210928, CCDM J19064-3704AB, HD 177474, HR 7226

F8V

1.2 M☉

57.8 ly

Gamma Coronae Australis B

HD 177475, HR 7227

F8V

1.1 M☉

57.8 ly

Tau1 Hydrae

τ1 Hya, 31 Hydrae, BD−02°2901, GJ 348, Gliese 348, HD 81997, HIP 46509, HR 3759, SAO 136895, WDS J09291-0246

F5V

1.2 M☉

57.9 ly

Rho Geminorum

ρ Gem A, 62 Gem, BD+32° 1562, HD 58946, HIP 36366, Gliese 274A, GJ 274 A, HR 2852

F1V

1.4 M☉

58.1 ly

Alpha Comae Berenices

TIC 138128530, 2MASS J13095936+1731456, GJ 501.0, Gliese 501.0, alf Com, HIP 64241, WISE J130958.97+173146.5, α Com, Alpha Com, 42 Comae Berenices, 42 Com, STF 1728, ADS 8804 , BD+18 2697, CCDM J13100+1732, GC 17833, Gliese 501, IDS 13051+1803 AB, LTT 13802, NLTT 33105, PPM 129630, SAO 100443, WDS 13100+1732

F5V

1.2 M☉

58.1 ly

Alpha Comae Berenices B

HD 114379, HR 4969

F5V

1.1 M☉

58.1 ly

Iota Centauri

ι Cen, CD−36°8497, FK5 496, GJ 508.1, Gliese 508.1, HD 115892, HIP 65109, HR 5028, SAO 204371

kA1.5hA3mA3Va

2.5 M☉

58.2 ly

Beta Arietis

Sheratan, Sharatan, Al Sharatain, 6 Arietis, Gl 80, HR 553, BD +20°306, HD 11636, SAO 75012, FK5 66, HIP 8903, bet Ari

kA4hA5mA5Va

2.3 M☉

58.7 ly

HD 125276

F9VFe-1.5CH-0.7

58.7 ly

HD 46588

HR 2401, Gliese 240.1, GJ 240.1, 23 H. Camelopardalis, AG+79°200, BD+79°212, GC 8711, HD 46588, HIP 32439, SAO 5946, WDS J06462+7934A

F7V

1.1 M☉

59.4 ly

Chi Cancri

χ Cnc, chi Cnc, 18 Cancri, BD+27°1589, FK5 1217, GJ 303, Gliese 303, HD 69897, HIP 40843, HR 3262, SAO 80104

F6V

1.1 M☉

59.4 ly

HD 114837

F6VFe-0.4

1.1 M☉

59.5 ly

Eta Corvi

η Crv, Eta Corvi, Eta Crv, 8 Corvi, 8 Crv, BD−15°3489, GC 17087, GJ 471.2, GJ 9411, Gliese 9411, HD 109085, HIP 61174, HR 4775, LTT 4755, NLTT 31021, PPM 225971, SAO 157345

F2V

1.4 M☉

59.5 ly

212 G. Puppis

212 Pup, HIP 38423, GC 10651, CD-34 4036，SAO 198540，HD 64379，HR 3079, 2MASS J07521555-3442199, TIC 150796339, WISE J075215.48-344217.3

F5VFe-0.5

1.3 M☉

59.8 ly

Theta Cygni

13 Cyg, θ Cyg, BD+49 3062, GJ 765, Gliese 765, HD 185395, HR 7469, SAO 31815, HIP 96441

F3+V

60.1 ly

Tau Piscis Austrini

τ PsA, 15 Piscis Austrini, CPD−33° 6227, HD 210302, HIP 109422, HR 8447, SAO 213602

F6V

1.3 M☉

60.2 ly

Delta Geminorum

del gam, Wasat, 55 Geminorum, BD+22° 1645, FK5 279, Gliese 271, Gl 271, HD 56986, HIP 35550, HR 2777, SAO 79294

F2VkF0mF0

1.6 M☉

60.7 ly

HD 25457

BD-00 632，SAO 130893，HR 1249, TYC 4725-1276-1, USNO-A2 0825-00911530, HIP 18859

F7V

61 ly

6 Ceti

6 Cet, BD−16° 17, GJ 10, Gliese 10, HD 693, HIP 910, HR 33, SAO 147133

F8VFe-0.8CH-0.5

1.1 M☉

61.6 ly

Estrellas masivas de la secuencia principal noticias

Lambda Bootis phenomenon identified in the massive early B-type star HD 37356

10. 8. 2026

Estrellas | 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

24. 6. 2026

Estrellas | 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

20. 6. 2026

Estrellas | 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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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.

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.

More about Estrellas

Random terms

Posición de la estrella Luminosidad Temperatura de la estrella Masa estelar Tamaño de la estrella Edad de las estrellas

	HD 37356 1484 ly			Discovery of the λ Bootis phenomenon in an early B-type star 10. 8. 2026
	VOS 70 3810 ly			A λ=1.3 millimeter Survey for Disks around Herbig Be Stars 24. 6. 2026
	HD 48914 2673 ly			A Be-shell star rotating at the critical limit and a partially stripped companion in a post-mass-transfer solution for the eclipsing binary V505 Mon 20. 6. 2026
	HD 188101 1394 ly			HD 188101: A Spotted B Star with Abundance Anomalies 6. 3. 2026
	Beta Pictoris 64 ly			The multi-wavelength vertical structure of the archetypal β Pictoris debris disk 5. 3. 2026

Lista de Étoiles massives de la séquence principale

Estrellas masivas de la secuencia principal noticias

Research in Étoiles massives de la séquence principale

Frequently Asked Questions about nearby stars

What is the nearest star?

What are the nearest stars to Earth?

What is the solar neighborhood?

How do astronomers measure distances to stars?

Are there any exoplanets orbiting the nearest stars?

Why are the nearest stars important for astronomy and physics?

StellarGuide: Estrellas