Des étoiles semblables au soleil

	Mass	Distance
Iota Pegasi B	G8V	0.82 M☉	38.8 ly
Lambda Serpentis * lam Ser, 27 Serpentis, BD +7°3023, HD 141004, HIP 77257, HIC 77257, HR 5868, SAO 121186, LTT 14677, GJ 598, Gliese 598, JP11 2646, 2MASS J15462661+0721109, N30 3543, NLTT 41151, SAO 121186, TIC 296740796, TYC 364-1224-1, WEB 13090	G0-V	1.1 M☉	38.9 ly
Zeta Reticuli B ζ2 Ret, Zeta2 Ret, CPD−62°265, Gliese 138, GJ 138, HD 20807, HIC 15371, HIP 15371, HR 1010, SAO 248774, LFT 276, LHS 172, LTT 1576	G1V	0.99 M☉	39.3 ly
Zeta Reticuli ζ1 Ret, Zeta1 Ret, CPD−63°217, Gliese 136, GJ 136, HD 20766, HIP 15330, HR 1006, SAO 248770, LFT 275, LHS 171, LTT 1573	G2.5VHdel1	0.96 M☉	39.3 ly
85 Pegasi * 85 Peg, BDS 12701, HR 9088, HD 224930, LFT 1848, LHS 101, LTT 17088, SAO 91669, HIP 171, HIC 171, ADS 17175 A, GJ 914 A, BD +26°4734 A, BU 733 A, Gliese 914, GJ 914	G5VbFe-2	0.88 M☉	40.2 ly
HD 69830 285 G. Puppis, BD−12°2449, Gliese 302, GJ 302, HIP 40693, HR 3259, LHS 245, SAO 154093, 2MASS J08182389-1237541, Gaia DR2 5726982995343100928	G8V	0.86 M☉	41 ly
55 Cancri Copernicus, LHS 2062, LDS 6219A, GJ 324 A, Gliese 324, HD 75732, Rho1 Cancri, 55 Cnc, BD+28°1660, HIC 43587, HIP 43587, HR 3522, SAO 80585, rho01 Cnc, LFT 609, LTT 12310, NLTT 20414, TIC 332064670, TOI-1773, TYC 1949-2012-1, WISEA J085235.41+281948.5	G8V	1 M☉	41.1 ly
44 Boötis B	G9V	-	41.6 ly
HD 14412 22 G. Fornacis, CD−26°828, Gliese 95, GJ 95, HD 14412, HIC 10798, HIP 10798, HR 683, SAO 167697, LHS 1387, LTT 1178	G8V	0.82 M☉	41.9 ly
HD 147513 62 G. Sco, CD−38° 10983, CPD−38° 6407, FK5 3295, GC 22030, Gl 620.1, HIC 80337, HIP 80337, HR 6094, SAO 207622, Wo 9559, 62 G. Scorpii, RAG 8A, GJ 9559, Gliese 9559, GJ 620.1 A, Gliese 620.1 A, 2MASS J16240128-3911346, TIC 350673608, TYC 7853-621-1	G5V C	-	42 ly
HD 172051 86 G. Sagittarii, BD−21° 5081, Gliese 722, GJ 722, HD 172051, HIC 91438, HIP 91438, HR 6998, SAO 187086, WDS J18389-2103AB	G6V	0.87 M☉	42.5 ly
47 Ursae Majoris Chalawan, BD+41°2147, BD+41 2147, FK5 1282, GC 15087, GCTP 2556.00, Gliese 407, GJ 407, HD 95128, HIC 53721, HIP 53721, HR 4277, LTT 12934, SAO 43557, * 47 UMa, IRAS 10566+4041, 2MASS J10592802+4025485, NLTT 25907, TIC 21535479, TYC 3009-2703-1, WISEA J105927.66+402549.4	G1-VFe-0.5 B	1.1 M☉	45.3 ly
HD 211415 CD -54°9222, GCTP 5395.00, Gliese 853, GJ 853 A, HD 211415, HIC 110109, HIP 110109, HR 8501, LHS 3790, LFT 1702, LTT 8943, SAO 247400	G0V	0.94 M☉	45.9 ly
Alpha Fornacis B	G7V	-	45.9 ly
18 Scorpii BD−07°4242, GC 21864, Gliese 616, GJ 616, HD 146233, HIP 79672, HR 6060, SAO 141066, CCDM 16156-0822	G2Va	1 M☉	46.1 ly
Gliese 611 HIP 78775, GL 611, GJ 611, TYC-3061-1027-1, BD+39 2947, LHS 3152, CD +39 2947, SAO 65065, HD 144579	G8V	-	46.8 ly
Pi1 Ursae Majoris Pi1 UMa, π¹ Ursae Majoris, π¹ UMa, 3 Ursae Majoris, BD +65°643, GC 11817, HD 72905, HIP 42438, HIC 42438, HR 3391, PPM 16705, SAO 14609, * pi.01 UMa	G0.5V	0.9 M☉	47.1 ly
72 Herculis w Her, 72 Her, NSV 8553, BD+32°2896, FK5 1456, Gliese 672, GJ 672, HD 157214, HIP 84862, HR 6458, SAO 65963, LHS 441, LTT 15148, W Herculis	G0V	1.2 M☉	47.6 ly
HD 196761 CD−24° 16193, GJ 796, HD 196761, HIP 101997, HR 7898, LTT 8172, SAO 189549	G7.5IV-V	0.81 M☉	47.9 ly
HD 10307 BD+41°328, GJ 67, Gliese 67, HD 10307, HIC 7918, HIP 7918, HR 483, SAO 37434, LHS 1284, YPC 350	G1V	1 M☉	47.9 ly

Nom de l étoile

Mass

Distance

G8V

0.82 M☉

38.8 ly

* lam Ser, 27 Serpentis, BD +7°3023, HD 141004, HIP 77257, HIC 77257, HR 5868, SAO 121186, LTT 14677, GJ 598, Gliese 598, JP11 2646, 2MASS J15462661+0721109, N30 3543, NLTT 41151, SAO 121186, TIC 296740796, TYC 364-1224-1, WEB 13090

G0-V

1.1 M☉

38.9 ly

Zeta Reticuli B

ζ2 Ret, Zeta2 Ret, CPD−62°265, Gliese 138, GJ 138, HD 20807, HIC 15371, HIP 15371, HR 1010, SAO 248774, LFT 276, LHS 172, LTT 1576

G1V

0.99 M☉

39.3 ly

Zeta Reticuli

ζ1 Ret, Zeta1 Ret, CPD−63°217, Gliese 136, GJ 136, HD 20766, HIP 15330, HR 1006, SAO 248770, LFT 275, LHS 171, LTT 1573

G2.5VHdel1

0.96 M☉

39.3 ly

85 Pegasi

* 85 Peg, BDS 12701, HR 9088, HD 224930, LFT 1848, LHS 101, LTT 17088, SAO 91669, HIP 171, HIC 171, ADS 17175 A, GJ 914 A, BD +26°4734 A, BU 733 A, Gliese 914, GJ 914

G5VbFe-2

0.88 M☉

40.2 ly

HD 69830

285 G. Puppis, BD−12°2449, Gliese 302, GJ 302, HIP 40693, HR 3259, LHS 245, SAO 154093, 2MASS J08182389-1237541, Gaia DR2 5726982995343100928

G8V

0.86 M☉

41 ly

55 Cancri

Copernicus, LHS 2062, LDS 6219A, GJ 324 A, Gliese 324, HD 75732, Rho1 Cancri, 55 Cnc, BD+28°1660, HIC 43587, HIP 43587, HR 3522, SAO 80585, rho01 Cnc, LFT 609, LTT 12310, NLTT 20414, TIC 332064670, TOI-1773, TYC 1949-2012-1, WISEA J085235.41+281948.5

G8V

1 M☉

41.1 ly

44 Boötis B

G9V

41.6 ly

HD 14412

22 G. Fornacis, CD−26°828, Gliese 95, GJ 95, HD 14412, HIC 10798, HIP 10798, HR 683, SAO 167697, LHS 1387, LTT 1178

G8V

0.82 M☉

41.9 ly

HD 147513

62 G. Sco, CD−38° 10983, CPD−38° 6407, FK5 3295, GC 22030, Gl 620.1, HIC 80337, HIP 80337, HR 6094, SAO 207622, Wo 9559, 62 G. Scorpii, RAG 8A, GJ 9559, Gliese 9559, GJ 620.1 A, Gliese 620.1 A, 2MASS J16240128-3911346, TIC 350673608, TYC 7853-621-1

G5V C

42 ly

HD 172051

86 G. Sagittarii, BD−21° 5081, Gliese 722, GJ 722, HD 172051, HIC 91438, HIP 91438, HR 6998, SAO 187086, WDS J18389-2103AB

G6V

0.87 M☉

42.5 ly

47 Ursae Majoris

Chalawan, BD+41°2147, BD+41 2147, FK5 1282, GC 15087, GCTP 2556.00, Gliese 407, GJ 407, HD 95128, HIC 53721, HIP 53721, HR 4277, LTT 12934, SAO 43557, * 47 UMa, IRAS 10566+4041, 2MASS J10592802+4025485, NLTT 25907, TIC 21535479, TYC 3009-2703-1, WISEA J105927.66+402549.4

G1-VFe-0.5 B

1.1 M☉

45.3 ly

HD 211415

CD -54°9222, GCTP 5395.00, Gliese 853, GJ 853 A, HD 211415, HIC 110109, HIP 110109, HR 8501, LHS 3790, LFT 1702, LTT 8943, SAO 247400

G0V

0.94 M☉

45.9 ly

Alpha Fornacis B

G7V

45.9 ly

18 Scorpii

BD−07°4242, GC 21864, Gliese 616, GJ 616, HD 146233, HIP 79672, HR 6060, SAO 141066, CCDM 16156-0822

G2Va

1 M☉

46.1 ly

Gliese 611

HIP 78775, GL 611, GJ 611, TYC-3061-1027-1, BD+39 2947, LHS 3152, CD +39 2947, SAO 65065, HD 144579

G8V

46.8 ly

Pi1 Ursae Majoris

Pi1 UMa, π¹ Ursae Majoris, π¹ UMa, 3 Ursae Majoris, BD +65°643, GC 11817, HD 72905, HIP 42438, HIC 42438, HR 3391, PPM 16705, SAO 14609, * pi.01 UMa

G0.5V

0.9 M☉

47.1 ly

72 Herculis

w Her, 72 Her, NSV 8553, BD+32°2896, FK5 1456, Gliese 672, GJ 672, HD 157214, HIP 84862, HR 6458, SAO 65963, LHS 441, LTT 15148, W Herculis

G0V

1.2 M☉

47.6 ly

HD 196761

CD−24° 16193, GJ 796, HD 196761, HIP 101997, HR 7898, LTT 8172, SAO 189549

G7.5IV-V

0.81 M☉

47.9 ly

HD 10307

BD+41°328, GJ 67, Gliese 67, HD 10307, HIC 7918, HIP 7918, HR 483, SAO 37434, LHS 1284, YPC 350

G1V

1 M☉

47.9 ly

Étoiles de type solaire nouvelles

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

Yesterday

Étoiles | Exoplanètes | Étoiles de type solaire | Jupiter chaud | Formation des planète

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

Étoiles | Exoplanètes | Étoiles de type solaire | Jupiter chaud | Atmosphères planétaire

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

Étoiles | Exoplanètes | Étoiles de type solaire | Atmosphères planétaire

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.

Étoiles

Les étoiles sont d’immenses sphères de gaz chaud qui brillent en produisant de l’énergie grâce à la fusion nucléaire dans leur noyau. La plupart des étoiles sont composées principalement d’hydrogène et d’hélium. Au centre d’une étoile, la pression et la température élevées provoquent la fusion des atomes d’hydrogène en hélium, libérant ainsi une énorme quantité d’énergie sous forme de lumière et de chaleur.

More about Étoiles

Random terms

Position de la étoile Luminosité Température des étoiles Masse stellaire Taille de l´étoile L´âge des étoiles

	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

Liste des Des étoiles semblables au soleil

Étoiles de type solaire nouvelles

Research in Des étoiles semblables au soleil

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: Étoiles