Étoiles massives de la séquence principale

	Mass	Distance
19 Draconis BD+65° 1157, Gliese 648, GJ 648, HD 153597, HIP 82860, HR 6315, SAO 17281, h Draconis	F8V	1 M☉	50 ly
WG 21	DA6.6	-	50.2 ly
Castor Aa Alpha Geminorum, α Gem, 66 Geminorum, FK5 287, GJ 278, Gliese 278, HIP 36850, SAO 60198, BD+32°1581A, PLX 1785.00, HR 2891, HD 60179	A1V	2.8 M☉	50.9 ly
Castor Ba BD+32°1581B, HR 2890, HD 60178	A2Vm	3 M☉	50.9 ly
Sigma Boötis * sig Boo, σ Boo, 28 Boötis, BD+30°2536, GC 19659, Gliese 557, GJ 557, HD 128167, HIP 71284, HR 5447, SAO 83416, CCDM 14347+2945	F4VkF2mF1	1.2 M☉	51.4 ly
99 Herculis b Her, 99 Her, BD+30°3128, GJ 704, HD 165908, HIP 88745, HR 6775, SAO 66648	F7VgF7mF5	0.94 M☉	51.4 ly
Chi Herculis chi Her, χ Her, 1 Her, BD+42° 2648, FK5 1166, Gliese 602, GJ 602, HD 142373, HIP 77760, HR 5914, SAO 45772, WDS J16254+1402AB	F8VFe-2Hdel-1	1.1 M☉	51.9 ly
Phi2 Ceti phi02 Cet, φ2 Cet, 19 Cet, NSV 316, BD−11° 153, GJ 37, Gliese 37, HD 4813, HIP 3909, HR 235, SAO 147470	F7V	1.2 M☉	51.9 ly
10 Ursae Majoris 10 UMa, 10 UMa, BD+42° 1956, FK5 339, Gliese 332, GJ 332, HD 76943, HIP 44248, HR 3579, SAO 42642	F3V	1.4 M☉	52.4 ly
HD 65907 LHS 1959, GCRV 5309, IDS 07559-6002 A, PPM 356380, CCDM J07578-6018A, LFT 560, SAO 250035, CD -59 1773, GJ 294 A, Gliese 294, LPM 276, Ci 20 453, HD 65907A, LTT 3020, SPOCS 359, 2MASS J07574692-6018111, TD1 11543, CPC 20.1 2000, HIC 38908, NLTT 18763, TYC 8911-793-1, CPD -59 944, HIP 38908, PLX 1902, UBV 7701, GC 10804, HR 3138, PM 07569-6010, uvby98 225160124	F9.5V	0.91 M☉	52.7 ly
I Carinae I Car, CD−73° 576, GJ 391, Gliese 391, HD 90589, HIC 50954, HIP 50954, HR 4102, SAO 256710	F3V	1.4 M☉	53.1 ly
Alpha Circini 17. G Circini, CD−64° 86, HD 128898, HIP 71908, HR 5463, SAO 252853, alf Cir	A7VpSrCrEu	1.6 M☉	53.5 ly
Ksi Pegasi ksi Peg, LHS 3851, GJ 872, Gliese 872	F6V	1.2 M☉	53.5 ly
Psi5 Aurigae psi05 Aur, 56 Aurigae, ADS 5425, BD+43°1595, FK5 255, GJ 245, Gliese 245, HD 48682, HIP 32480, HR 2483, SAO 41330	F9V	1.1 M☉	54.2 ly
HD 55575 HR 2721, HIP 35136, GJ 1095, Gliese 1095, SAO 41644, BD+47 1419, TYC 3396-2196-1	F9V	0.91 M☉	55 ly
58 Ophiuchi 58 Oph, BD−21°4712, FK5 1463, GC 24030, Gliese 692, GJ 692, HD 160915, HIP 86736, HR 6595, SAO 185660, Gaia EDR3 4117290138348536064	F5V	1.3 M☉	56 ly
HD 10647 q01 Eri, q1 Eridani, 5 G. Eridani, Gliese 3109, GJ 3109, HR 506, HIC 7978, HIP 7978, SAO 232501, CPD−54° 365, WISE J014229.49-534428.1, TIC 229137615, TYC 8475-527-1, 2MASS J01422932-5344271	F9V	1.1 M☉	56.6 ly
Iota Horologii ι Hor, GJ 108, Gliese 108, HD 17051, HIC 12653, HIP 12653, HR 810, 2MASS J02423346-5048008, LTT 1322, NLTT 8800, TIC 166853853, TYC 8056-1164-1, WISEA J024233.84-504758.7	F8V C	1.3 M☉	56.6 ly
g Lupi CD−44° 10310, CPD−44° 7529, GC 21070, GJ 594, Gliese 594, HD 139664, HIP 76829, HR 5825, SAO 226064, PPM 320883, LTT 6256, NLTT 40843	F3/5V	1.4 M☉	56.7 ly
Xi Ophiuchi ksi Oph, ξ Oph, 40 Ophiuchi, BD−20°4731, FK5 917, GC 23423, HD 156897, HIP 84893, HR 6445, SAO 185296, CCDM J17210-2107AB, WDS J17210-2107AB, LTT 6908	F2V	1.3 M☉	57.1 ly

Nombre de la estrella

Mass

Distance

19 Draconis

BD+65° 1157, Gliese 648, GJ 648, HD 153597, HIP 82860, HR 6315, SAO 17281, h Draconis

F8V

1 M☉

50 ly

WG 21

DA6.6

50.2 ly

Castor Aa

Alpha Geminorum, α Gem, 66 Geminorum, FK5 287, GJ 278, Gliese 278, HIP 36850, SAO 60198, BD+32°1581A, PLX 1785.00, HR 2891, HD 60179

A1V

2.8 M☉

50.9 ly

Castor Ba

BD+32°1581B, HR 2890, HD 60178

A2Vm

3 M☉

50.9 ly

Sigma Boötis

* sig Boo, σ Boo, 28 Boötis, BD+30°2536, GC 19659, Gliese 557, GJ 557, HD 128167, HIP 71284, HR 5447, SAO 83416, CCDM 14347+2945

F4VkF2mF1

1.2 M☉

51.4 ly

99 Herculis

b Her, 99 Her, BD+30°3128, GJ 704, HD 165908, HIP 88745, HR 6775, SAO 66648

F7VgF7mF5

0.94 M☉

51.4 ly

Chi Herculis

chi Her, χ Her, 1 Her, BD+42° 2648, FK5 1166, Gliese 602, GJ 602, HD 142373, HIP 77760, HR 5914, SAO 45772, WDS J16254+1402AB

F8VFe-2Hdel-1

1.1 M☉

51.9 ly

Phi2 Ceti

phi02 Cet, φ2 Cet, 19 Cet, NSV 316, BD−11° 153, GJ 37, Gliese 37, HD 4813, HIP 3909, HR 235, SAO 147470

F7V

1.2 M☉

51.9 ly

10 Ursae Majoris

10 UMa, 10 UMa, BD+42° 1956, FK5 339, Gliese 332, GJ 332, HD 76943, HIP 44248, HR 3579, SAO 42642

F3V

1.4 M☉

52.4 ly

HD 65907

LHS 1959, GCRV 5309, IDS 07559-6002 A, PPM 356380, CCDM J07578-6018A, LFT 560, SAO 250035, CD -59 1773, GJ 294 A, Gliese 294, LPM 276, Ci 20 453, HD 65907A, LTT 3020, SPOCS 359, 2MASS J07574692-6018111, TD1 11543, CPC 20.1 2000, HIC 38908, NLTT 18763, TYC 8911-793-1, CPD -59 944, HIP 38908, PLX 1902, UBV 7701, GC 10804, HR 3138, PM 07569-6010, uvby98 225160124

F9.5V

0.91 M☉

52.7 ly

I Carinae

I Car, CD−73° 576, GJ 391, Gliese 391, HD 90589, HIC 50954, HIP 50954, HR 4102, SAO 256710

F3V

1.4 M☉

53.1 ly

Alpha Circini

17. G Circini, CD−64° 86, HD 128898, HIP 71908, HR 5463, SAO 252853, alf Cir

A7VpSrCrEu

1.6 M☉

53.5 ly

Ksi Pegasi

ksi Peg, LHS 3851, GJ 872, Gliese 872

F6V

1.2 M☉

53.5 ly

Psi5 Aurigae

psi05 Aur, 56 Aurigae, ADS 5425, BD+43°1595, FK5 255, GJ 245, Gliese 245, HD 48682, HIP 32480, HR 2483, SAO 41330

F9V

1.1 M☉

54.2 ly

HD 55575

HR 2721, HIP 35136, GJ 1095, Gliese 1095, SAO 41644, BD+47 1419, TYC 3396-2196-1

F9V

0.91 M☉

55 ly

58 Ophiuchi

58 Oph, BD−21°4712, FK5 1463, GC 24030, Gliese 692, GJ 692, HD 160915, HIP 86736, HR 6595, SAO 185660, Gaia EDR3 4117290138348536064

F5V

1.3 M☉

56 ly

HD 10647

q01 Eri, q1 Eridani, 5 G. Eridani, Gliese 3109, GJ 3109, HR 506, HIC 7978, HIP 7978, SAO 232501, CPD−54° 365, WISE J014229.49-534428.1, TIC 229137615, TYC 8475-527-1, 2MASS J01422932-5344271

F9V

1.1 M☉

56.6 ly

Iota Horologii

ι Hor, GJ 108, Gliese 108, HD 17051, HIC 12653, HIP 12653, HR 810, 2MASS J02423346-5048008, LTT 1322, NLTT 8800, TIC 166853853, TYC 8056-1164-1, WISEA J024233.84-504758.7

F8V C

1.3 M☉

56.6 ly

g Lupi

CD−44° 10310, CPD−44° 7529, GC 21070, GJ 594, Gliese 594, HD 139664, HIP 76829, HR 5825, SAO 226064, PPM 320883, LTT 6256, NLTT 40843

F3/5V

1.4 M☉

56.7 ly

Xi Ophiuchi

ksi Oph, ξ Oph, 40 Ophiuchi, BD−20°4731, FK5 917, GC 23423, HD 156897, HIP 84893, HR 6445, SAO 185296, CCDM J17210-2107AB, WDS J17210-2107AB, LTT 6908

F2V

1.3 M☉

57.1 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