Étoiles massives de la séquence principale

	Mass	Distance
V658 Carinae HD 92406, V658 Car, HD 92406, Hen 3-462, THA 35-III-25, uvby98 100092406, ALS 1712, LLNS 2157, TIC 458267524, V* V658 Car, CD-58 3440, LS 1712, TYC 8613-763-1, WEB 9498, CEL 3612, 2MASS J10384726-5843323, UBV M 16421, [JE82] 517, CPD-58 2461, NSV 18470, UCAC2 6053104, Gaia DR2 5350666550826252032, GEN# 1.00092406, RAVE J103847.3-584332, UCAC4 157-049429, Gaia DR3 5350666550826252032, GSC 08613-00763, SBC9 628, USNO-B1.0 0312-00178638	Bp_sh D	4.5 M☉	329 ly
HD 166191 HIC 89046, HIP 89046, 2MASS J18103033-2334003, TIC 114619435, TYC 6843-1557-1, WISE J181030.32-233400.6, 2XMM J181030.3-233400	F3/5V D	-	330 ly
HD 163296 BD-21 4779, HH 409, HIC 87819, HIP 87819, JP11 2900, 2MASS J17562128-2157218, PDS 473, TIC 105083750, TYC 6262-2131-1, SAO 185966, 2XMM J175621.3-215722	A1Vep C	2.3 M☉	331 ly
HD 106906 2MASS J12175319-5558319, HIP 59960, TYC 8637-2434-1, TIC 390472975, WISE J121753.15-555831.9, BYV 1A	F5V	1.5 M☉	334 ly
HD 106906 B		-	334 ly
HD 131399 CD−33°10153, HD 131399, HIP 72940, SAO 206071	A1V	2 M☉	335 ly
HD 100453 HD 100453A, CD-53 4102, GSC 08617-01438, HIP 56354, 2MASS J11330559-5419285, TYC 8617-1438-1, Gaia DR3 5345011040956367104	A9Ve	1.6 M☉	338 ly
HIP 41378 K2-93, EPIC 211311380, BD+10 1799, 2MASS J08262784+1004493, TIC 366443426, TYC 800-1325-1	F8 D	1.2 M☉	346 ly
HD 109832	A9V	1.8 M☉	350 ly
HIP 65426 HD 116434, 2MASS J13243609-5130159, GC 18126, TIC 438702139, TYC 8260-1526-1, Gaia DR3 6070080754075553792	A2V C	2 M☉	351 ly
HD 111520		-	352 ly
HD 156623 TYC 8341-414-1, HIP 84881, USNO-A2 0375-31087304, GC 23402, 2MASS J17205061-4525149, TIC 217302172	A0V C	1.9 M☉	353 ly
TOI 2010 TIC 26547036	F0	1.1 M☉	354 ly
HD 100546 KR Mus, HIC 56379, HIP 56379, SAO 251457, CD−69° 893, GC 15855, 2MASS J11332542-7011412, PDS 340, TIC 280773136, TYC 9229-2446-1, WISEA J113325.38-701141.0, IRAS 11312-6955	A0VaekB8_lB B	2.2 M☉	359 ly
HIP 73990 HD 133803	A9V	1.7 M☉	359 ly
TOI 2458 HD 34562, TIC 449197831, TYC 0100-00856-1, 2MASS J05182917+0115139	F9V	1.1 M☉	363 ly
TOI 201 TOI-201		1.3 M☉	366 ly
HD 120326	F0	-	369 ly
TOI 1751 HD 146757, TYC 4192-02025-1, TIC 287080092		-	370 ly
TOI 1744 TOI-1744 A, BD 60 1982, TOI-1744 A, BD 60 1982	F8V	1.2 M☉	372 ly

Nombre de la estrella

Mass

Distance

HD 92406, V658 Car, HD 92406, Hen 3-462, THA 35-III-25, uvby98 100092406, ALS 1712, LLNS 2157, TIC 458267524, V* V658 Car, CD-58 3440, LS 1712, TYC 8613-763-1, WEB 9498, CEL 3612, 2MASS J10384726-5843323, UBV M 16421, [JE82] 517, CPD-58 2461, NSV 18470, UCAC2 6053104, Gaia DR2 5350666550826252032, GEN# 1.00092406, RAVE J103847.3-584332, UCAC4 157-049429, Gaia DR3 5350666550826252032, GSC 08613-00763, SBC9 628, USNO-B1.0 0312-00178638

Bp_sh D

4.5 M☉

329 ly

HD 166191

HIC 89046, HIP 89046, 2MASS J18103033-2334003, TIC 114619435, TYC 6843-1557-1, WISE J181030.32-233400.6, 2XMM J181030.3-233400

F3/5V D

330 ly

HD 163296

BD-21 4779, HH 409, HIC 87819, HIP 87819, JP11 2900, 2MASS J17562128-2157218, PDS 473, TIC 105083750, TYC 6262-2131-1, SAO 185966, 2XMM J175621.3-215722

A1Vep C

2.3 M☉

331 ly

HD 106906

2MASS J12175319-5558319, HIP 59960, TYC 8637-2434-1, TIC 390472975, WISE J121753.15-555831.9, BYV 1A

F5V

1.5 M☉

334 ly

HD 106906 B

334 ly

HD 131399

CD−33°10153, HD 131399, HIP 72940, SAO 206071

A1V

2 M☉

335 ly

HD 100453

HD 100453A, CD-53 4102, GSC 08617-01438, HIP 56354, 2MASS J11330559-5419285, TYC 8617-1438-1, Gaia DR3 5345011040956367104

A9Ve

1.6 M☉

338 ly

HIP 41378

K2-93, EPIC 211311380, BD+10 1799, 2MASS J08262784+1004493, TIC 366443426, TYC 800-1325-1

F8 D

1.2 M☉

346 ly

HD 109832

A9V

1.8 M☉

350 ly

HIP 65426

HD 116434, 2MASS J13243609-5130159, GC 18126, TIC 438702139, TYC 8260-1526-1, Gaia DR3 6070080754075553792

A2V C

2 M☉

351 ly

HD 111520

352 ly

HD 156623

TYC 8341-414-1, HIP 84881, USNO-A2 0375-31087304, GC 23402, 2MASS J17205061-4525149, TIC 217302172

A0V C

1.9 M☉

353 ly

TOI 2010

TIC 26547036

1.1 M☉

354 ly

HD 100546

KR Mus, HIC 56379, HIP 56379, SAO 251457, CD−69° 893, GC 15855, 2MASS J11332542-7011412, PDS 340, TIC 280773136, TYC 9229-2446-1, WISEA J113325.38-701141.0, IRAS 11312-6955

A0VaekB8_lB B

2.2 M☉

359 ly

HIP 73990

HD 133803

A9V

1.7 M☉

359 ly

TOI 2458

HD 34562, TIC 449197831, TYC 0100-00856-1, 2MASS J05182917+0115139

F9V

1.1 M☉

363 ly

TOI 201

TOI-201

1.3 M☉

366 ly

HD 120326

369 ly

TOI 1751

HD 146757, TYC 4192-02025-1, TIC 287080092

370 ly

TOI 1744

TOI-1744 A, BD 60 1982, TOI-1744 A, BD 60 1982

F8V

1.2 M☉

372 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