Étoiles massives de la séquence principale

	Mass	Distance
Psi1 Draconis B BD+72° 805, HD 162004, HIC 86620, HIP 86620, HR 6637, SAO 8891	F8V	1.2 M☉	74 ly
Psi1 Draconis 31 Draconis, 31 Dra, ADS 10759 AB, Gliese 694.1, GJ 694.1, ψ¹ Dra A: BD+72° 804, HD 162003, HIC 86614, HIP 86614, HR 6636, SAO 8890	F5IV-V C	1.4 M☉	74.2 ly
Zeta Virginis Heze, 79 Virginis, BD+00°3076, FK5 501, GJ 3792, Gliese 3792, HD 118098, HIP 66249, HR 5107, SAO 139420, WDS J13347-0036, NT3, NGCA-V98	A2Van	2 M☉	74.6 ly
94 Ceti BD-01° 457, FK5 116, GJ 128, Gliese 128, HD 19994, HIP 14954, HR 962, LTT 1515, SAO 130355	F8.5V C	1.3 M☉	74.6 ly
Gamma Ceti Kaffaljidhma, γ Cet, 86 Ceti, BD+02 422, HD 16970, HIP 12706, HR 804, SAO 110707, WDS 02433+0314	A2Vn	1.9 M☉	74.8 ly
Gamma Ceti B	F3V	1.2 M☉	74.8 ly
HD 90508	F9-V	-	75 ly
Zeta Serpentis ζ Ser, 57 Serpentis, BD−03° 4217, GC 24503, HD 164259, HIP 88175, HR 6710, SAO 142025	F2V	1.4 M☉	75 ly
Upsilon Aquarii υ Aqr, 59 Aquarii, BD−21 6251, FK5 849, HD 213845, HIP 111449, HR 8592, SAO 191235	F7V	1.4 M☉	75.1 ly
HD 90089 BD+83°297, FK5 911, GJ 392.1, HD 90089, HIP 51502, HR 4084, SAO 1714, WDS J10311+8234A	F4VkF2mF2	1.3 M☉	75.1 ly
Sigma Ceti σ Cet, 76 Cet, BD−15° 449, FK5 1071, HD 15798, HIP 11783, HR 740, SAO 148445, * sig Cet	F5V / F4IV	1.2 M☉	75.2 ly
HD 91949	F0	-	75.4 ly
36 Draconis 36 Dra, BD+64° 1252, FK5 685, GJ 9619, Gliese 9619, HD 168151, HIP 89348, HR 6850, SAO 17828	F5V	1.2 M☉	75.5 ly
Alpha2 Librae B		1.8 M☉	75.8 ly
64 Piscium B 64 Piscium Ab	F8V	1.2 M☉	76.3 ly
64 Piscium 64 Psc, BD+16° 76, FK5 1020, GJ 9031, HD 4676, HIP 3810, HR 225, SAO 92099, WDS J00490+1656A, 64 Piscium Aa	F8V	1.2 M☉	76.3 ly
88 Leonis STF 1547 AB, 88 Leonis, BD+15°2345, HD 100180, HIP 56242, HR 4437, WDS J11317+1422, Wolf 401, 88 Leo A, AG+14°1209, GJ 3669, Gliese 3669, SAO 99648, LTT 13145, 88 Leo B, AG+14°1208, GJ 3670, SAO 99647, LTT 13146	F9.5V	1.1 M☉	76.5 ly
HD 167425	F9.5V	-	76.6 ly
Epsilon Ceti * eps Cet, ε Cet, 83 Cet, BD−12° 501, HD 16620, HIP 12390, HR 781, SAO 148528	F5V	1.4 M☉	76.8 ly
Delta Herculis Aa Sarin, δ Her, 65 Her, BD 25° 3221, CCDM J17151+2451A, FK5 641, GC 23294, HD 156164, HIP 84379, HR 6410, SAO 84951	A1IVn	2.4 M☉	76.8 ly

Nombre de la estrella

Mass

Distance

Psi1 Draconis B

BD+72° 805, HD 162004, HIC 86620, HIP 86620, HR 6637, SAO 8891

F8V

1.2 M☉

74 ly

Psi1 Draconis

31 Draconis, 31 Dra, ADS 10759 AB, Gliese 694.1, GJ 694.1, ψ¹ Dra A: BD+72° 804, HD 162003, HIC 86614, HIP 86614, HR 6636, SAO 8890

F5IV-V C

1.4 M☉

74.2 ly

Zeta Virginis

Heze, 79 Virginis, BD+00°3076, FK5 501, GJ 3792, Gliese 3792, HD 118098, HIP 66249, HR 5107, SAO 139420, WDS J13347-0036, NT3, NGCA-V98

A2Van

2 M☉

74.6 ly

94 Ceti

BD-01° 457, FK5 116, GJ 128, Gliese 128, HD 19994, HIP 14954, HR 962, LTT 1515, SAO 130355

F8.5V C

1.3 M☉

74.6 ly

Gamma Ceti

Kaffaljidhma, γ Cet, 86 Ceti, BD+02 422, HD 16970, HIP 12706, HR 804, SAO 110707, WDS 02433+0314

A2Vn

1.9 M☉

74.8 ly

Gamma Ceti B

F3V

1.2 M☉

74.8 ly

HD 90508

F9-V

75 ly

Zeta Serpentis

ζ Ser, 57 Serpentis, BD−03° 4217, GC 24503, HD 164259, HIP 88175, HR 6710, SAO 142025

F2V

1.4 M☉

75 ly

Upsilon Aquarii

υ Aqr, 59 Aquarii, BD−21 6251, FK5 849, HD 213845, HIP 111449, HR 8592, SAO 191235

F7V

1.4 M☉

75.1 ly

HD 90089

BD+83°297, FK5 911, GJ 392.1, HD 90089, HIP 51502, HR 4084, SAO 1714, WDS J10311+8234A

F4VkF2mF2

1.3 M☉

75.1 ly

Sigma Ceti

σ Cet, 76 Cet, BD−15° 449, FK5 1071, HD 15798, HIP 11783, HR 740, SAO 148445, * sig Cet

F5V / F4IV

1.2 M☉

75.2 ly

HD 91949

75.4 ly

36 Draconis

36 Dra, BD+64° 1252, FK5 685, GJ 9619, Gliese 9619, HD 168151, HIP 89348, HR 6850, SAO 17828

F5V

1.2 M☉

75.5 ly

Alpha2 Librae B

1.8 M☉

75.8 ly

64 Piscium B

64 Piscium Ab

F8V

1.2 M☉

76.3 ly

64 Piscium

64 Psc, BD+16° 76, FK5 1020, GJ 9031, HD 4676, HIP 3810, HR 225, SAO 92099, WDS J00490+1656A, 64 Piscium Aa

F8V

1.2 M☉

76.3 ly

88 Leonis

STF 1547 AB, 88 Leonis, BD+15°2345, HD 100180, HIP 56242, HR 4437, WDS J11317+1422, Wolf 401, 88 Leo A, AG+14°1209, GJ 3669, Gliese 3669, SAO 99648, LTT 13145, 88 Leo B, AG+14°1208, GJ 3670, SAO 99647, LTT 13146

F9.5V

1.1 M☉

76.5 ly

HD 167425

F9.5V

76.6 ly

Epsilon Ceti

* eps Cet, ε Cet, 83 Cet, BD−12° 501, HD 16620, HIP 12390, HR 781, SAO 148528

F5V

1.4 M☉

76.8 ly

Delta Herculis Aa

Sarin, δ Her, 65 Her, BD 25° 3221, CCDM J17151+2451A, FK5 641, GC 23294, HD 156164, HIP 84379, HR 6410, SAO 84951

A1IVn

2.4 M☉

76.8 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