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Массивные звезды главной последовательности
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Звезды 1-20
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Имя звезды Mass Distance

Sirius
Dog Star, Aschere, Canicula, Al Shira, Sothis, Alhabor, Mrgavyadha, Lubdhaka, Tenrōsei, α Canis Majoris (α CMa), 9 Canis Majoris (9 CMa), HD 48915, HR 2491, BD−16°1591, GJ 244, LHS 219, ADS 5423, LTT 2638, HIP 32349, alf CMa
A0mA1 Va 2.1 M☉ 8.7 ly

Altair
Alpha Aquilae, α Aquilae, Gliese 768, 53 Aquilae, 53 Aql, BD+08°4236, FK5 745, GCTP 4665.00, Gliese 768, HD 187642, HIP 97649, HR 7557, LFT 1499, LHS 3490, LTT 15795, NLTT 48314, SAO 125122, WDS 19508+0852A, alf Aql
A7 V 1.8 M☉ 16.7 ly

Eta Cassiopeiae
Achird, Gliese 34, Wolf 24, Achird, η Cas 24 Cassiopeiae, ADS 671, BD+57°150, GCTP 155, HD 4614, HIP 3821, HR 219, LHS 123/122, LFT 74, LTT 10287, SAO 21732, Struve 60, GC 962
F9V 0.97 M☉ 19.3 ly

Vega
Alpha Lyrae, Lucida Lyrae, Gliese 721, GJ 721, Wega, α Lyrae, 3 Lyrae, BD+38°3238, GCTP 4293.00, HD 172167, HIC 91262, HIP 91262, HR 7001, LTT 15486, SAO 67174
A0Va 2.1 M☉ 25 ly

Fomalhaut
α Piscis Austrini, α PsA, Alpha PsA, 24 Piscis Austrini, CPD −30° 6685, FK5 867, Gl 881, HD 216956, HIP 113368, HR 8728, SAO 191524, alf PsA
A3V C 1.9 M☉ 25.1 ly

Pi3 Orionis
Tabit, π³ Ori, 1 Ori, Pi3 Orionis, BD+06°762, FK5 1134, GCTP 1077.00, Gliese 178, HD 30652, HIP 22449, HR 1543, LTT 11517, SAO 112106
F6 V 1.2 M☉ 26.2 ly

Chi Draconis
Gliese 713, χ Dra, 44 Dra, BD+72° 839, FK5 695, Gliese 713, HD 170153, HIP 89937, HR 6927, LHS 3379, LTT 15438, SAO 9087
F7 V 1 M☉ 26.3 ly

Zeta Tucanae
FK5 10, GCTP 54, Gliese 17, GJ 17, HD 1581, HIP 1599, HR 77, LHS 5, LTT 167, SAO 248163, GC 401
F9.5V 0.99 M☉ 28.1 ly

Xi Ursae Majoris Aa
Alula Australis, ξ Ursae Majoris, ξ UMa, Xi UMa, 53 Ursae Majoris, BD+32°2132, CCDM J11182+3132, GC 15537, HIP 55203, IDS 11128+3206, SAO 62484, WDS J11182+3132
F8.5 V 0.97 M☉ 28.8 ly

Gamma Leporis
13 Leporis, BD−22° 1211, CD−22° 2438, FK5 217, Gliese 216 A, HD 38393, HIP 27072, HR 1983, SAO 170759, BD−22 1210, Gliese 216 B, HD 38392, HR 1982, LTT 2363, SAO 170757
F6 V 0.82 M☉ 29 ly

Gamma Pavonis
γ Pav, CD−65° 2751, FK5 805, Gliese 827, HD 203608, HIP 105858, HR 8181, LHS 3674, LTT 8510, SAO 254999, gam Pav
F9 V 1.2 M☉ 30.2 ly

Beta Leonis
Denebola, * bet Leo, Deneb Aleet, β Leonis, 94 Leo, BD+15°2383, FK5 444, GCTP 2738.00, GJ 448, Gliese 448, HD 102647, HIC 57632, HIP 57632, HR 4534, LFT 853, LHS 2462, LTT 13249, SAO 99809, 2MASS J11490366+1434197, TIC 14725877, TYC 870-988-1, USNO-B1.0 1045-00205720
A3Va 1.8 M☉ 35.9 ly

Beta Virginis
Zavijava, Zavijah, Alaraph, Minelauva, β Vir, 5 Virginis, BD+02°2489, FK5 445, HD 102870, HIC 57757, HIP 57757, HR 4540, SAO 119076, LHS 2465, bet Vir, GJ 449, Gliese 449, LFT 854, LTT 13264, 2MASS J11504173+0145528, NLTT 28736, SAO 119076, SDSS J115041.71+014552.7, TIC 366661076, TYC 273-924-1, WISEA J115042.25+014550.1
F9V 1.4 M☉ 35.9 ly

Theta Persei
* tet Per, θ Per, BD+48°746, GJ 107, Gliese 107, CCDM J02441+4913, IDS 02374+4848, WDS J02442+4914, 13 Persei, HR 799, HD 16895, HIP 12777, FK5 93, GC 3277, PPM 45428, SAO 38288
F8V 1.1 M☉ 36.4 ly

Gamma Serpentis
LHS 408, 41 Ser, * gam Ser, Ainalhai, 41 Serpentis, BD+16° 2849, FK5 591, GCTP 3604.00, HD 142860, HIP 78072, HR 5933, LHS 408, SAO 101826, TIC 377415363, TYC 1496-2119-1, WISEA J155627.41+153928.7, NLTT 41572, N30 3579, GJ 603, Gliese 603
F6V 1.3 M☉ 36.4 ly

Zeta Doradus
GJ 189, Gliese 189, * zet Dor, CPD−57° 735, FK5 189, HD 33262, HIP 23693, HIC 23693, HR 1674, SAO 233822, GC 6258, 2MASS J05053067-5728217, TIC 381949122, TYC 8514-2291-1, WDS J05055-5728A
F9VFe-0.5 1.1 M☉ 38.1 ly

Iota Pegasi
ι Peg, 24 Pegasi, BD+24°4533, FK5 831, HD 210027, HIC 109176, HIP 109176, HR 8430, SAO 90238, WDS J22070+2521A
F5V 1.3 M☉ 38.8 ly

Gamma Virginis
Porrima, Antevorta, Arich, 29 Virginis, BD-00°2601, GCTP 2924.00, Gl 482 AB, Gliese 482, HIP 61941, HIC 61941, LHS 2604, SAO 138917, WDS 12417-0127, * gam Vir A
F1-F2V 1.6 M☉ 39.2 ly

Gamma Virginis B
F0mF2V 1.5 M☉ 39.2 ly

Zeta Trianguli Australis
* zet TrA, CD -69°2558, FK5 610, GCTP 3719.00, Gliese 624, Gl 624, HD 147584, HIC 80686, HIP 80686, HR 6098, LTT 6558, SAO 253554, GC 22089, 2MASS J16282814-7005037, WISEA J162828.62-700502.6, TIC 362747897, TYC 9278-2951-1
F9V 1.1 M☉ 39.4 ly
Звезды 1-20
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study iconResearch in Массивные звезды главной последовательности

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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: Звезды

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Звезды
Звёзды — это огромные шары раскалённого газа, которые светятся благодаря выработке энергии в процессе ядерного синтеза в их ядрах. Большинство звёзд состоит в основном из водорода и гелия. В центре звезды из-за высокого давления и температуры атомы водорода сливаются в гелий, высвобождая огромное количество энергии в виде света и тепла.
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