Красные карлики

	Mass	Distance
Gliese 1093 Luyten 399-68, LHS 223, G 109-35, PLX 1635.01, NLTT 17247, 2MASS J06592868+1920577	M5 V	0.21 M☉	25.3 ly
LP 71-82 G 227-22, LSPM J1802+6415, NLTT 45873, 2MASS J18021660+6415445, 2E 4002, RX J1802.2+6415, TIC 233068870, WISEA J180216.92+641540.2	M5 V	-	25.4 ly
Gliese 623 HEN 1, LHS 417, G 202-45, HIC 80346, HIP 80346, LFT 1273, LHS 417, L 1707-1, LTT 14885, NLTT 42730, 2MASS J16240913+4821112	M3 V	0.51 M☉	25.6 ly
Gliese 623 B	M D	0.06 M☉	25.6 ly
Gliese 1224 LHS 3359, L 920-26, G 154-44, G 155-1	M4Ve	0.14 M☉	26 ly
SCR J0740-4257 UCAC4 236-016971, 2MASS J07401183-4257406, PM J07401-4257, TIC 123480394	M4.5	-	26 ly
Gliese 831 B	M4.5 V	0.12 M☉	26.1 ly
Gliese 257 CD-44 3045, HIC 33499, HIP 33499, LHS 222, LFT 502, LTT 2699, NLTT 17239, LPM 248, Ci 20 407, GJ 257, Gaia DR2 5559035514779133056	M3.5 V	0.25 M☉	26.2 ly
Gliese 257 B CD-44 3045B, GJ 257 B, CSI-44 3045 23, LPM 248B	M3 D	0.24 M☉	26.2 ly
Gliese 1151 G 122-49, LHS 316, PLX 2739.0, NLTT 28752, Zkh 171, GJ 1151, 2MASS J11505787+4822395, TIC 11893637, WISEA J115056.09+482228.4	M4.5Ve C	0.15 M☉	26.2 ly
Gliese 480.1 LP 399-68, LHS 340, GJ 9415, LFT 935, HIC 61874, HIP 61874, LTT 4836, NLTT 31495, 2MASS J12404633-4333595, TYC 7783-576-1, L 399-68	M3 V	0 M☉	26.3 ly
Gliese 486 GJ 486, Gl 486, Wolf 437, LHS 341, HIC 62452, HIP 62452, LFT 947, LTT 13654, G 60-32, Ci 20 737, TYC 882-1111-1, NLTT 31933, WISEA J124755.90+094500.2, LSPM J1247+0945, 2MASS J12475664+0945050, PLX 2943	M3.5Ve C	0.32 M☉	26.4 ly
Gliese 793 HIP 101180, LHS 3558, LTT 15991, G 262-15, LFT 1552, LTT 15991, NLTT 49417, MCC 820	M3 V	0.39 M☉	26.4 ly
Gliese 1154 LTT 13408, G 13-22, LHS 2531, NLTT 30062, PLX 2817.01, LSPM J1214+0037, 2MASS J12141654+0037263	M4.5 V	0 M☉	26.4 ly
Gliese 300 L 674-15, LHS 1989, LFT 571, LP 843-1, LTT 3080, NLTT 19136, 2MASS J08124088-2133056, JP11 5131, GJ 300	M3.5 V	0.17 M☉	26.5 ly
Gliese 686 BD+18 3421, LHS 452, G 170-55, HIC 86287, HIP 86287, L 1278-24, LFT 1363, LTT 15228, NLTT 45173, GJ 686	M1.5 Ve	0.42 M☉	26.6 ly
L 173-19 NLTT 6772, 2MASS J02003830-5558047, GSC 08485-00936, TIC 231055581	M V	0 M☉	26.8 ly
Gliese 48 HIP 4856, LHS 131, Ross 318, BD+70 68b, LFT 93, LTT 10362, NLTT 3359, MCC 364, 2MASS J01023213+7140475, Ross 318	M3.5V	0.34 M☉	26.9 ly
Gliese 54 GKI 3, CD-68 47, CPD-68 41, GALEX 6384743253449642140, LFT 117, LTT 660, LPM 62, LHS 1208, HIC 5496, HIP 5496, 2MASS J01102281-6726425, Gaia DR2 4704272495284592512, NLTT 3945, TIC 52121469, TYC 8855-238-1, NSV 427	M2.5V	0.43 M☉	26.9 ly
Gliese 54 B		0.3 M☉	26.9 ly

Имя звезды

Mass

Distance

Gliese 1093

Luyten 399-68, LHS 223, G 109-35, PLX 1635.01, NLTT 17247, 2MASS J06592868+1920577

M5 V

0.21 M☉

25.3 ly

LP 71-82

G 227-22, LSPM J1802+6415, NLTT 45873, 2MASS J18021660+6415445, 2E 4002, RX J1802.2+6415, TIC 233068870, WISEA J180216.92+641540.2

M5 V

25.4 ly

Gliese 623

HEN 1, LHS 417, G 202-45, HIC 80346, HIP 80346, LFT 1273, LHS 417, L 1707-1, LTT 14885, NLTT 42730, 2MASS J16240913+4821112

M3 V

0.51 M☉

25.6 ly

Gliese 623 B

M D

0.06 M☉

25.6 ly

Gliese 1224

LHS 3359, L 920-26, G 154-44, G 155-1

M4Ve

0.14 M☉

26 ly

SCR J0740-4257

UCAC4 236-016971, 2MASS J07401183-4257406, PM J07401-4257, TIC 123480394

M4.5

26 ly

Gliese 831 B

M4.5 V

0.12 M☉

26.1 ly

Gliese 257

CD-44 3045, HIC 33499, HIP 33499, LHS 222, LFT 502, LTT 2699, NLTT 17239, LPM 248, Ci 20 407, GJ 257, Gaia DR2 5559035514779133056

M3.5 V

0.25 M☉

26.2 ly

Gliese 257 B

CD-44 3045B, GJ 257 B, CSI-44 3045 23, LPM 248B

M3 D

0.24 M☉

26.2 ly

Gliese 1151

G 122-49, LHS 316, PLX 2739.0, NLTT 28752, Zkh 171, GJ 1151, 2MASS J11505787+4822395, TIC 11893637, WISEA J115056.09+482228.4

M4.5Ve C

0.15 M☉

26.2 ly

Gliese 480.1

LP 399-68, LHS 340, GJ 9415, LFT 935, HIC 61874, HIP 61874, LTT 4836, NLTT 31495, 2MASS J12404633-4333595, TYC 7783-576-1, L 399-68

M3 V

0 M☉

26.3 ly

Gliese 486

GJ 486, Gl 486, Wolf 437, LHS 341, HIC 62452, HIP 62452, LFT 947, LTT 13654, G 60-32, Ci 20 737, TYC 882-1111-1, NLTT 31933, WISEA J124755.90+094500.2, LSPM J1247+0945, 2MASS J12475664+0945050, PLX 2943

M3.5Ve C

0.32 M☉

26.4 ly

Gliese 793

HIP 101180, LHS 3558, LTT 15991, G 262-15, LFT 1552, LTT 15991, NLTT 49417, MCC 820

M3 V

0.39 M☉

26.4 ly

Gliese 1154

LTT 13408, G 13-22, LHS 2531, NLTT 30062, PLX 2817.01, LSPM J1214+0037, 2MASS J12141654+0037263

M4.5 V

0 M☉

26.4 ly

Gliese 300

L 674-15, LHS 1989, LFT 571, LP 843-1, LTT 3080, NLTT 19136, 2MASS J08124088-2133056, JP11 5131, GJ 300

M3.5 V

0.17 M☉

26.5 ly

Gliese 686

BD+18 3421, LHS 452, G 170-55, HIC 86287, HIP 86287, L 1278-24, LFT 1363, LTT 15228, NLTT 45173, GJ 686

M1.5 Ve

0.42 M☉

26.6 ly

L 173-19

NLTT 6772, 2MASS J02003830-5558047, GSC 08485-00936, TIC 231055581

M V

0 M☉

26.8 ly

Gliese 48

HIP 4856, LHS 131, Ross 318, BD+70 68b, LFT 93, LTT 10362, NLTT 3359, MCC 364, 2MASS J01023213+7140475, Ross 318

M3.5V

0.34 M☉

26.9 ly

Gliese 54

GKI 3, CD-68 47, CPD-68 41, GALEX 6384743253449642140, LFT 117, LTT 660, LPM 62, LHS 1208, HIC 5496, HIP 5496, 2MASS J01102281-6726425, Gaia DR2 4704272495284592512, NLTT 3945, TIC 52121469, TYC 8855-238-1, NSV 427

M2.5V

0.43 M☉

26.9 ly

Gliese 54 B

0.3 M☉

26.9 ly

Красные карлики Новости

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A

Today

Звезды | Экзопланеты | Красные карлики | TESS

Image: Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A

A small planet candidate has been identified in the binary star system known as Gliese 774. The object, which is smaller than the Earth, orbits its host star approximately every 4.2 days. Observations from the Transiting Exoplanet Survey Satellite (TESS) captured the planet as it passed in front of its star, briefly blocking a tiny fraction of the starlight. This periodic dimming event allowed for the identification of the candidate despite the complex environment of a binary system, where two s...

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Ammonia and hydrogen may separate inside Uranus and Neptune

Today

Звезды | Экзопланеты | Красные карлики

Image: Ammonia and hydrogen may separate inside Uranus and Neptune

Uranus and Neptune may be experiencing ammonia rain: simulations show their expected temperature profiles cross the boundary where ammonia and hydrogen separate. In warmer sub-Neptune TOI-270 d, the two are likely to mix in all proportions....

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Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

15. 10. 2026

Image: Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

The exoplanet TOI-2257 b orbits its star once every 35 days with a high eccentricity. New models suggest its atmospheric and orbital fate depends on whether it is a gas-rich mini-Neptune or a rocky super-Earth. Higher eccentricity would confirm a gaseous nature....

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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

TOI 431 106 ly		Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey today
L 115-21 41.9 ly		A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274) today
TOI-3686 841 ly		TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance today
HD 112485 5881 ly		Ensemble pulsational characteristics of eclipsing binaries containing β Cep stars observed by the TESS mission 19. 10. 2026
TOI-5322 1560 ly	+1	A Sample of Thick-Disk Stars Hosting Hot Jupiters 17. 10. 2026

Список Красные карлики