Солнцеподобные звезды

	Mass	Distance
Sol Sol, Helios, Slunce, Sun, Sonne, солнце, Soleil	G2V	1 M☉	0 ly
Alpha Centauri Gliese 559, FK5 538, CD−60°5483, CCDM J14396-6050, GC 19728, α Cen A, Rigil Kentaurus, Rigil Kent, α1 Centauri, HR 5459, HD 128620, GCTP 3309.00, LHS 50, SAO 252838, HIP 71683, alf Cen A	G2V	1.1 M☉	4.4 ly
Tau Ceti Gliese 71, GJ 71, 52 Cet, BD−16° 295, FK5 59, HD 10700, HIP 8102, HIC 8102, HR 509, SAO 147986, LFT 159, LHS 146, LTT 935, * tau Cet, τ Ceti	G8 V	0.69 M☉	11.9 ly
82 G. Eridani e Eri, e Eridani, 82 Eridani, Gliese 139, GJ 139, HD 20794, LHS 19, LTT 1583, HR 1008, SAO 216263, FK5 119, HIP 15510, HIC 15510	G6 V	0.7 M☉	19.7 ly
Xi Bootis Gliese 566, GJ 556, Ksi Bootis, ξ Boo, ξ Boötis, 37 Boötis, HD 131156, HIP 72659, HR 5544, SAO 101250	G8Ve	0.88 M☉	22 ly
Mu Cassiopeiae 30 Cassiopeiae, Gliese 53, HR 321, BD+54°223, HD 6582, LHS 8, LTT 10460, GCTP 219.00, SAO 22024, FK5 1030, LFT 107, HIP 5336, GC 1360, CCDM J01080+5455, MU Cas, V* MU Cas	G5Vb	0.74 M☉	25 ly
Beta Canum Venaticorum Asterion, Chara, Beta CVn, 8 CVn, BD +42 2321, FK5 470, HD 109358, HIP 61317, HR 4785, SAO 44230, Gliese 475, * bet CVn, Gaia DR2 1534011998570864256	G0 V	1 M☉	27.6 ly
61 Virginis 61 Vir, Gliese 506, BD-17°3813, FK5 1345, GCTP 3039.00, HD 115617, HIP 64924, HR 5019, LHS 349, LTT 5111, SAO 157844	G7 V	0.93 M☉	27.8 ly
Chi1 Orionis 54 Ori, Gliese 222, GJ 222, HR 2047, BD+20° 1162, HD 39587, LTT 11743, GCTP 1354.00, SAO 77705, HIC 27913, HIP 27913	G0 V	1 M☉	28.4 ly
Xi Ursae Majoris Ba ksi UMa B	G2 V	0.86 M☉	28.5 ly
41 G. Arae 41 Arae, CD-46° 11370, Gliese 666, GJ 666, HD 156274, HIP 84720, HR 6416, LHS 444, LTT 6886, SAO 227816, LPM 636, LFT 1334, * 41 Ara	G8V	0.81 M☉	28.7 ly
Beta Comae Berenices 43 Com, β Com, BD+28° 2193, FK5 492, Gl 502, GJ 502, Gliese 502, HD 114710, HIP 64394, HR 4983, LHS 348, LTT 13815, SAO 82706, * bet Com	G0 V	1.2 M☉	30 ly
Kappa 1 Ceti 96 Ceti, BD+02°518, FK5 1095, GCTP 691.00, Gliese 137, HD 20630, HIP 15457, HR 996, LTT 11094, SAO 111120, kap01 Cet, Kappa1 Ceti	G5V	1 M☉	30.3 ly
66 G. Centauri Gliese 442, HD 102365, HR 4523, 66 G. Centauri, CD -39°7301, LHS 311, LTT 4373, GCTP 2725.00, SAO 223020, HIP 57443	G6V	0.89 M☉	30.4 ly
61 Ursae Majoris 61 UMa, BD+35° 2270, FK5 1300, GCTP 2699.00, GJ 434, Gliese 434, HD 101501, HIC 56997, HIP 56997, HR 4496, LTT 13200, SAO 62655, NSV 5291, * 61 UMa	G8 V	0.85 M☉	31.2 ly
Alpha Mensae Alf Men, Alp Men, CD−74° 294, FK5 239, GJ 231, Gliese 231, HD 43834, HIP 29271, HR 2261, SAO 256274, LTT 2490	G7 V	1.1 M☉	33.3 ly
Iota Persei ι Per, 24 Pegasi, BD+49°857, FK5 112, GC 3740, HD 19373, HIC 14632, HIP 14632, HR 937, SAO 38597, PPM 45875, CCDM J03091+4936A, WDS J03091+4937A, LHS 166, * iot Per, GC 3740, GJ 124, Gliese 124, Koenig 3, LFT 256, LTT 11020, NLTT 9973, 2MASS J03090387+4936479, N30 638, TIC 116988032, TYC 3318-1840-1, WISEA J030905.34+493646.9	G0V	1.4 M☉	34.5 ly
Zeta Herculis B	G7 V	0.98 M☉	35 ly
Delta Trianguli δ Trianguli, δ Tri, Delta Tri, 8 Trianguli, BD+33° 395, Gliese 92, HD 13974, HIP 10644, HR 660, LHS 154, LTT 10770, SAO 55420, * del Tri	G0.5V	1 M☉	35.6 ly
11 Leonis Minoris 11 LMi, BD+36°1979, GJ 356, Gliese 356, HD 82885, HIC 47080, HIP 47080, HR 3815, SAO 61586, WDS 09357+3549, GC 13242, TIC 8915802, TYC 2500-1533-1, WISEA J093538.92+354834.4, LTT 12535, NLTT 22117, 2MASS J09353959+3548366	G8Va	0.96 M☉	36.6 ly

Имя звезды

Mass

Distance

Sol

Sol, Helios, Slunce, Sun, Sonne, солнце, Soleil

G2V

1 M☉

0 ly

Alpha Centauri

Gliese 559, FK5 538, CD−60°5483, CCDM J14396-6050, GC 19728, α Cen A, Rigil Kentaurus, Rigil Kent, α1 Centauri, HR 5459, HD 128620, GCTP 3309.00, LHS 50, SAO 252838, HIP 71683, alf Cen A

G2V

1.1 M☉

4.4 ly

Tau Ceti

Gliese 71, GJ 71, 52 Cet, BD−16° 295, FK5 59, HD 10700, HIP 8102, HIC 8102, HR 509, SAO 147986, LFT 159, LHS 146, LTT 935, * tau Cet, τ Ceti

G8 V

0.69 M☉

11.9 ly

82 G. Eridani

e Eri, e Eridani, 82 Eridani, Gliese 139, GJ 139, HD 20794, LHS 19, LTT 1583, HR 1008, SAO 216263, FK5 119, HIP 15510, HIC 15510

G6 V

0.7 M☉

19.7 ly

Xi Bootis

Gliese 566, GJ 556, Ksi Bootis, ξ Boo, ξ Boötis, 37 Boötis, HD 131156, HIP 72659, HR 5544, SAO 101250

G8Ve

0.88 M☉

22 ly

Mu Cassiopeiae

30 Cassiopeiae, Gliese 53, HR 321, BD+54°223, HD 6582, LHS 8, LTT 10460, GCTP 219.00, SAO 22024, FK5 1030, LFT 107, HIP 5336, GC 1360, CCDM J01080+5455, MU Cas, V* MU Cas

G5Vb

0.74 M☉

25 ly

Beta Canum Venaticorum

Asterion, Chara, Beta CVn, 8 CVn, BD +42 2321, FK5 470, HD 109358, HIP 61317, HR 4785, SAO 44230, Gliese 475, * bet CVn, Gaia DR2 1534011998570864256

G0 V

1 M☉

27.6 ly

61 Virginis

61 Vir, Gliese 506, BD-17°3813, FK5 1345, GCTP 3039.00, HD 115617, HIP 64924, HR 5019, LHS 349, LTT 5111, SAO 157844

G7 V

0.93 M☉

27.8 ly

Chi1 Orionis

54 Ori, Gliese 222, GJ 222, HR 2047, BD+20° 1162, HD 39587, LTT 11743, GCTP 1354.00, SAO 77705, HIC 27913, HIP 27913

G0 V

1 M☉

28.4 ly

Xi Ursae Majoris Ba

ksi UMa B

G2 V

0.86 M☉

28.5 ly

41 G. Arae

41 Arae, CD-46° 11370, Gliese 666, GJ 666, HD 156274, HIP 84720, HR 6416, LHS 444, LTT 6886, SAO 227816, LPM 636, LFT 1334, * 41 Ara

G8V

0.81 M☉

28.7 ly

Beta Comae Berenices

43 Com, β Com, BD+28° 2193, FK5 492, Gl 502, GJ 502, Gliese 502, HD 114710, HIP 64394, HR 4983, LHS 348, LTT 13815, SAO 82706, * bet Com

G0 V

1.2 M☉

30 ly

Kappa 1 Ceti

96 Ceti, BD+02°518, FK5 1095, GCTP 691.00, Gliese 137, HD 20630, HIP 15457, HR 996, LTT 11094, SAO 111120, kap01 Cet, Kappa1 Ceti

G5V

1 M☉

30.3 ly

66 G. Centauri

Gliese 442, HD 102365, HR 4523, 66 G. Centauri, CD -39°7301, LHS 311, LTT 4373, GCTP 2725.00, SAO 223020, HIP 57443

G6V

0.89 M☉

30.4 ly

61 Ursae Majoris

61 UMa, BD+35° 2270, FK5 1300, GCTP 2699.00, GJ 434, Gliese 434, HD 101501, HIC 56997, HIP 56997, HR 4496, LTT 13200, SAO 62655, NSV 5291, * 61 UMa

G8 V

0.85 M☉

31.2 ly

Alpha Mensae

Alf Men, Alp Men, CD−74° 294, FK5 239, GJ 231, Gliese 231, HD 43834, HIP 29271, HR 2261, SAO 256274, LTT 2490

G7 V

1.1 M☉

33.3 ly

Iota Persei

ι Per, 24 Pegasi, BD+49°857, FK5 112, GC 3740, HD 19373, HIC 14632, HIP 14632, HR 937, SAO 38597, PPM 45875, CCDM J03091+4936A, WDS J03091+4937A, LHS 166, * iot Per, GC 3740, GJ 124, Gliese 124, Koenig 3, LFT 256, LTT 11020, NLTT 9973, 2MASS J03090387+4936479, N30 638, TIC 116988032, TYC 3318-1840-1, WISEA J030905.34+493646.9

G0V

1.4 M☉

34.5 ly

Zeta Herculis B

G7 V

0.98 M☉

35 ly

Delta Trianguli

δ Trianguli, δ Tri, Delta Tri, 8 Trianguli, BD+33° 395, Gliese 92, HD 13974, HIP 10644, HR 660, LHS 154, LTT 10770, SAO 55420, * del Tri

G0.5V

1 M☉

35.6 ly

11 Leonis Minoris

11 LMi, BD+36°1979, GJ 356, Gliese 356, HD 82885, HIC 47080, HIP 47080, HR 3815, SAO 61586, WDS 09357+3549, GC 13242, TIC 8915802, TYC 2500-1533-1, WISEA J093538.92+354834.4, LTT 12535, NLTT 22117, 2MASS J09353959+3548366

G8Va

0.96 M☉

36.6 ly

Солнцеподобные звёзды Новости

Thick-disk stars identified as hosts to ancient hot jupiter planets

Yesterday

Звезды | Экзопланеты | Солнцеподобные звёзды | Горячий юпитер | Формирование планет

Image: Thick-disk stars identified as hosts to ancient hot jupiter planets

Large gas giant planets that orbit very close to their parent stars are known as hot Jupiters. By analyzing a sample of 268 stars, researchers have identified several hot Jupiters orbiting stars belonging to the high-alpha thick disk of our galaxy. The thick disk represents a component of the Milky Way containing older stars with specific chemical signatures, particularly higher amounts of alpha elements like magnesium, silicon, and calcium relative to iron. These systems are significantly older...

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Atmospheric differences between morning and evening sides of planet WASP-39 b revealed

12. 10. 2026

Звезды | Экзопланеты | Солнцеподобные звёзды | Горячий юпитер | Атмосферы планет

Image: Atmospheric differences between morning and evening sides of planet WASP-39 b revealed

Observations of the hot Jupiter WASP-39 b reveal significant differences between its morning and evening atmospheres. Climate models successfully match temperature patterns but still struggle to explain the observed asymmetry in carbon dioxide levels....

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Water vapor detected in the atmosphere of ultrahot Neptune LTT 9779 b

9. 10. 2026

Звезды | Экзопланеты | Солнцеподобные звёзды | Атмосферы планет

Image: Water vapor detected in the atmosphere of ultrahot Neptune LTT 9779 b

New observations of the ultrahot Neptune LTT 9779 b reveal the presence of water vapor on its dayside. The planet shows no signs of thermal inversion or significant atmospheric escape, supporting the theory that it is a tidally locked world....

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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.

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.

More about Звезды

Random terms

Позиция звезды Светимость Температура звезд Масса звезды Размер звезды Звездный возраст

	WASP 94 687 ly			A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum yesterday
	KELT-2 439 ly			Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity 15. 10. 2026
	TOI-2257 189 ly			The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b 15. 10. 2026
	KELT-18 1032 ly			High-resolution transmission spectroscopy of KELT-18b Metastable helium detection at 1083 nm 14. 10. 2026
	WASP 17 1315 ly			A Spatial Map of the Atmospheric Limb of a Hot Jupiter 14. 10. 2026

Список Солнцеподобные звезды

Солнцеподобные звёзды Новости

Research in Солнцеподобные звезды

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: Звезды