Sous-géantes | Stellar Catalog

	Mass	Distance
40 Leonis 40 Leo, BD+20° 2466, HD 89449, HIP 50564, HR 4054, SAO 99065	F6IV-V	1.4 M☉	69.2 ly
Theta Draconis θ Dra, 13 Her, BD+58°1608, FK5 598, HD 144284, HIP 78527, HR 5986, SAO 29765	F8IV-V	1.2 M☉	70.2 ly
71 Orionis HD 43042, HR 2220, 71 Ori, 2MASS J06145088+1909229, GJ 3390, Gliese 3390	F5.5IV-V	-	71 ly
HD 26923	G0IV	-	72 ly
HD 63433 BD+27 1490, GSC 01933-00747, HIC 38228, HIP 38228, 2MASS J07495506+2721473, SAO 79729, TIC 130181866, TYC 1933-747-1, TOI-1726, V* V377 Gem	G5IV E	0.99 M☉	73 ly
Eta Scorpii η Sco, eta Sco, CD−43 11485, FK5 638, GJ 657, Gliese 657, HD 155203, HIP 84143, HR 6380, SAO 227707	F5IV	1.8 M☉	73.2 ly
Alpha2 Librae α2 Lib, 9 Librae, BD−15 3966, FK5 548, HD 130841, HIP 72622, HR 5531, SAO 158840	kA2hA5mA4IV-V	1.4 M☉	75.8 ly
Kappa Tucanae κ Tuc, HD 7788, HIP 5896, HR 377, SAO 248346	F6IV	1.4 M☉	75.9 ly
Kappa Fornacis CD−24° 1038, GJ 97, Gliese 97, HD 14802, HIP 11072, HR 695, SAO 167736	G1IV	1.2 M☉	76 ly
HD 62644 LHS 1939, LPM 270, SAO 218923, CD -44 3675, GJ 284, LTT 2929, Ci 20 436, HD 62644, 2MASS J07425710-4510227, TD1 10901, CPC 0 4777, HIC 37606, NLTT 18354, TYC 8134-800-1, CPD -44 1829, HIP 37606, PLX 1831, UBV 7432, GC 10402, HR 2998, PM 07414-4503, UBV M 13584, GCRV 5148, LFT 545, PPM 312086, uvby98 100062644	G8IV-V	1.3 M☉	76.2 ly
Iota Leonis Aa ι Leo, 78 Leonis, Gliese 426.1, BD+11°2348, HD 99028, HIP 55642, HR 4399, SAO 99587	F1IV	1.7 M☉	77 ly
23 Ursae Majoris h UMa, 23 UMa, BD+63°845, FK5 355, GJ 3534, HD 81937, HIP 46733, HR 3757, SAO 14908, CCDM J09315+6303A/B	F0IV	1.9 M☉	77.5 ly
Eta Indi η Ind, CPD−52° 11752, FK5 776, HD 197157, HIP 102333, HR 7920, SAO 246709	A9IV	1.6 M☉	78.9 ly
Alpha Leonis Regulus, α Leonis, 32 Leonis, GJ 9316, HR 3982, ADS 7654, WDS J10084+1158, α Leo A, BD+12°2149, FK5 380, HD 87901, HIP 49669, SAO 98967, LTT 12716	B8IVn	3.8 M☉	79.3 ly
V401 Hydra V* V401 Hya, HD 73350, HIP 42333, 2MASS J08375030-0648248, WISEA J083750.08-064824.2, GJ 9273, Gliese 9273, TIC 51443167	G8/K0(IV)	-	79.4 ly
HD 166435	G1IV	-	79.6 ly
Delta Velorum Aa Alsephina, CD−54°1788, GCTP 2098.00, HD 74956, HIP 42913, HR 3485, SAO 236232, WDS 08447-5443	A2IV	2.4 M☉	80.6 ly
HD 195564 BD−10° 5423, FK5 1536, GJ 792.1, HD 195564, HIP 101345, HR 7845, SAO 163665	G2.5IV	1.1 M☉	80.7 ly
5 Serpentis 5 Ser, MQ Ser, BD+02° 2944, HD 136202, HIP 74975, HR 5694, SAO 120946, WDS J15193+0146A	F8IV	1.2 M☉	82 ly
HD 204079	K2IV-V	-	82.1 ly

Nom de l étoile

Mass

Distance

40 Leonis

40 Leo, BD+20° 2466, HD 89449, HIP 50564, HR 4054, SAO 99065

F6IV-V

1.4 M☉

69.2 ly

Theta Draconis

θ Dra, 13 Her, BD+58°1608, FK5 598, HD 144284, HIP 78527, HR 5986, SAO 29765

F8IV-V

1.2 M☉

70.2 ly

71 Orionis

HD 43042, HR 2220, 71 Ori, 2MASS J06145088+1909229, GJ 3390, Gliese 3390

F5.5IV-V

71 ly

HD 26923

G0IV

72 ly

HD 63433

BD+27 1490, GSC 01933-00747, HIC 38228, HIP 38228, 2MASS J07495506+2721473, SAO 79729, TIC 130181866, TYC 1933-747-1, TOI-1726, V* V377 Gem

G5IV E

0.99 M☉

73 ly

Eta Scorpii

η Sco, eta Sco, CD−43 11485, FK5 638, GJ 657, Gliese 657, HD 155203, HIP 84143, HR 6380, SAO 227707

F5IV

1.8 M☉

73.2 ly

Alpha2 Librae

α2 Lib, 9 Librae, BD−15 3966, FK5 548, HD 130841, HIP 72622, HR 5531, SAO 158840

kA2hA5mA4IV-V

1.4 M☉

75.8 ly

Kappa Tucanae

κ Tuc, HD 7788, HIP 5896, HR 377, SAO 248346

F6IV

1.4 M☉

75.9 ly

Kappa Fornacis

CD−24° 1038, GJ 97, Gliese 97, HD 14802, HIP 11072, HR 695, SAO 167736

G1IV

1.2 M☉

76 ly

HD 62644

LHS 1939, LPM 270, SAO 218923, CD -44 3675, GJ 284, LTT 2929, Ci 20 436, HD 62644, 2MASS J07425710-4510227, TD1 10901, CPC 0 4777, HIC 37606, NLTT 18354, TYC 8134-800-1, CPD -44 1829, HIP 37606, PLX 1831, UBV 7432, GC 10402, HR 2998, PM 07414-4503, UBV M 13584, GCRV 5148, LFT 545, PPM 312086, uvby98 100062644

G8IV-V

1.3 M☉

76.2 ly

Iota Leonis Aa

ι Leo, 78 Leonis, Gliese 426.1, BD+11°2348, HD 99028, HIP 55642, HR 4399, SAO 99587

F1IV

1.7 M☉

77 ly

23 Ursae Majoris

h UMa, 23 UMa, BD+63°845, FK5 355, GJ 3534, HD 81937, HIP 46733, HR 3757, SAO 14908, CCDM J09315+6303A/B

F0IV

1.9 M☉

77.5 ly

Eta Indi

η Ind, CPD−52° 11752, FK5 776, HD 197157, HIP 102333, HR 7920, SAO 246709

A9IV

1.6 M☉

78.9 ly

Alpha Leonis

Regulus, α Leonis, 32 Leonis, GJ 9316, HR 3982, ADS 7654, WDS J10084+1158, α Leo A, BD+12°2149, FK5 380, HD 87901, HIP 49669, SAO 98967, LTT 12716

B8IVn

3.8 M☉

79.3 ly

V401 Hydra

V* V401 Hya, HD 73350, HIP 42333, 2MASS J08375030-0648248, WISEA J083750.08-064824.2, GJ 9273, Gliese 9273, TIC 51443167

G8/K0(IV)

79.4 ly

HD 166435

G1IV

79.6 ly

Delta Velorum Aa

Alsephina, CD−54°1788, GCTP 2098.00, HD 74956, HIP 42913, HR 3485, SAO 236232, WDS 08447-5443

A2IV

2.4 M☉

80.6 ly

HD 195564

BD−10° 5423, FK5 1536, GJ 792.1, HD 195564, HIP 101345, HR 7845, SAO 163665

G2.5IV

1.1 M☉

80.7 ly

5 Serpentis

5 Ser, MQ Ser, BD+02° 2944, HD 136202, HIP 74975, HR 5694, SAO 120946, WDS J15193+0146A

F8IV

1.2 M☉

82 ly

HD 204079

K2IV-V

82.1 ly

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

Liste des Sous-géantes

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