Красные карлики

	Mass	Distance
Proxima Centauri Alpha Centauri C, CCDM J14396-6050C, GCTP 3278.00, Gliese 551, HIP 70890, LFT 1110, LHS 49, LPM 526, LTT 5721, NLTT 37460, V645 Centauri	M5.5 Ve	0.12 M☉	4.2 ly
Barnard star GCTP 4098.00, Gl 140-024, Gliese 699, GJ 699, HIC 87937, HIP 87937, LFT 1385, LHS 57, LTT 15309, Munich 15040, Proxima Ophiuchi, V2500 Ophiuchi, Velox Barnardi, Vyssotsky 799	M4 V	0.14 M☉	6 ly
Wolf 359 CN Leonis, Gliese 406, GJ 406, G 045-020, LTT 12923, LFT 750, LHS 36, GCTP 2553	M6.5 Ve	0.11 M☉	7.9 ly
Lalande 21185 BD+36 2147, G 119-052, Gliese 411, GJ 411, HD 95735, HIP 54035, LFT 756, LHS 37, LTT 12960, MCC 594, PLX 2576, SAO 62377, NLTT 26105, NSV 18593	M2+V	0.46 M☉	8.3 ly
Luyten 726-8 B LHS 10, G 272-61B	M6 V	0.12 M☉	8.7 ly
Luyten 726-8 Gliese 65, GJ 65, BL Ceti, UV Ceti, LHS 9, LHS 10, G 272-61, LUY 726, IDS 01340-1828, L 726-8, 2MASS J01390120-1757026, WISE J013903.93-175655.7	M5.5 V	0.12 M☉	8.9 ly
Ross 154 Gliese 729, GJ 729, V1216 Sgr, CD−23° 14742, GCTP 4338, HIP 92403, LHS 3414, V1216 Sagittarii, Ross 154	M3.5 V	0.17 M☉	9.7 ly
Ross 248 Gliese 905, GJ 905, HH Andromedae, HH And, 2MASS J23415498+4410407, G 171-010, GCTP 5736.00, LHS 549	M5.0V	0.14 M☉	10.3 ly
Lacaille 9352 Gliese 887, GJ 887, HD 217987, CD -36°15693, GCTP 5584, LHS 70, SAO 214301, LTT 9348, LFT 1758, Cordoba 31353, NSV 14420, HIP 114046, UGPMF 591, CPC 18 11792, Ci 20 1400, HIC 114046	M1V	0.5 M☉	10.7 ly
Ross 128 FI Virginis, FI Vir, G 010-050, GCTP 2730, GJ 447, Gliese 447, HIC 57548, HIP 57548, LHS 315, Vyssotsky 286, LTT 13240, LFT 852, LSPM PM I11477+0048, 2MASS J11474440+0048164	M3V	0.17 M☉	11 ly
EZ Aquarii Luyten 789-6, Gliese 866, GJ 866, GCTP 5475.00, LHS 68, G 156-031, EZ Aqr, V* EZ Aqr	M5 V	0.11 M☉	11.1 ly
EZ Aquarii B	M5 V	0.11 M☉	11.1 ly
EZ Aquarii C	M5 V	0.1 M☉	11.1 ly
Struve 2398 Gliese 725, G 227-046, HD 173739, HIP 91768, LHS 58, Vyssotsky 184, ADS 11632, BD +59°1915, GCTP 4330.00 A/B	M3 V	0.33 M☉	11.5 ly
Struve 2398 B G 227-047, HD 173740, HIP 91772, LHS 91772.	M3.5 V	0.25 M☉	11.5 ly
Groombridge 34 GX Andromedae, V* GX And, BD+43° 44, GCTP 49, Gliese 15 A, GJ 15 A, Gl 15 A, G 171-047, HD 1326, HIP 1475, LHS 3, LTT 10108, SAO 36248	M2V	0.4 M☉	11.6 ly
Groombridge 34 B GQ Andromedae, Gliese 15 B, G 171-048, LHS 4, LTT 10109	M4.1 V	0.16 M☉	11.6 ly
DX Cancri Gliese 1111, GJ 1111, G 051-015, GCTP 2016.01, LHS 248, G 51-15, DX Cnc	M6.5 V	0.09 M☉	11.7 ly
Gliese 1061 LHS 1565, LFT 295, LTT 1702, LP 995-46, L 372-58, GJ 1061	M5.5 V	0.11 M☉	12 ly
YZ Ceti GCTP 248.01, Gliese 54.1, GJ 54.1, G 268-135, LHS 138, LTT 670, L 725-32, HIP 5643, YZ Cet	M4 Ve	0.13 M☉	12.1 ly

Имя звезды

Mass

Distance

Alpha Centauri C, CCDM J14396-6050C, GCTP 3278.00, Gliese 551, HIP 70890, LFT 1110, LHS 49, LPM 526, LTT 5721, NLTT 37460, V645 Centauri

M5.5 Ve

0.12 M☉

4.2 ly

Barnard star

GCTP 4098.00, Gl 140-024, Gliese 699, GJ 699, HIC 87937, HIP 87937, LFT 1385, LHS 57, LTT 15309, Munich 15040, Proxima Ophiuchi, V2500 Ophiuchi, Velox Barnardi, Vyssotsky 799

M4 V

0.14 M☉

6 ly

Wolf 359

CN Leonis, Gliese 406, GJ 406, G 045-020, LTT 12923, LFT 750, LHS 36, GCTP 2553

M6.5 Ve

0.11 M☉

7.9 ly

Lalande 21185

BD+36 2147, G 119-052, Gliese 411, GJ 411, HD 95735, HIP 54035, LFT 756, LHS 37, LTT 12960, MCC 594, PLX 2576, SAO 62377, NLTT 26105, NSV 18593

M2+V

0.46 M☉

8.3 ly

Luyten 726-8 B

LHS 10, G 272-61B

M6 V

0.12 M☉

8.7 ly

Luyten 726-8

Gliese 65, GJ 65, BL Ceti, UV Ceti, LHS 9, LHS 10, G 272-61, LUY 726, IDS 01340-1828, L 726-8, 2MASS J01390120-1757026, WISE J013903.93-175655.7

M5.5 V

0.12 M☉

8.9 ly

Ross 154

Gliese 729, GJ 729, V1216 Sgr, CD−23° 14742, GCTP 4338, HIP 92403, LHS 3414, V1216 Sagittarii, Ross 154

M3.5 V

0.17 M☉

9.7 ly

Ross 248

Gliese 905, GJ 905, HH Andromedae, HH And, 2MASS J23415498+4410407, G 171-010, GCTP 5736.00, LHS 549

M5.0V

0.14 M☉

10.3 ly

Lacaille 9352

Gliese 887, GJ 887, HD 217987, CD -36°15693, GCTP 5584, LHS 70, SAO 214301, LTT 9348, LFT 1758, Cordoba 31353, NSV 14420, HIP 114046, UGPMF 591, CPC 18 11792, Ci 20 1400, HIC 114046

M1V

0.5 M☉

10.7 ly

Ross 128

FI Virginis, FI Vir, G 010-050, GCTP 2730, GJ 447, Gliese 447, HIC 57548, HIP 57548, LHS 315, Vyssotsky 286, LTT 13240, LFT 852, LSPM PM I11477+0048, 2MASS J11474440+0048164

M3V

0.17 M☉

11 ly

EZ Aquarii

Luyten 789-6, Gliese 866, GJ 866, GCTP 5475.00, LHS 68, G 156-031, EZ Aqr, V* EZ Aqr

M5 V

0.11 M☉

11.1 ly

EZ Aquarii B

M5 V

0.11 M☉

11.1 ly

EZ Aquarii C

M5 V

0.1 M☉

11.1 ly

Struve 2398

Gliese 725, G 227-046, HD 173739, HIP 91768, LHS 58, Vyssotsky 184, ADS 11632, BD +59°1915, GCTP 4330.00 A/B

M3 V

0.33 M☉

11.5 ly

Struve 2398 B

G 227-047, HD 173740, HIP 91772, LHS 91772.

M3.5 V

0.25 M☉

11.5 ly

Groombridge 34

GX Andromedae, V* GX And, BD+43° 44, GCTP 49, Gliese 15 A, GJ 15 A, Gl 15 A, G 171-047, HD 1326, HIP 1475, LHS 3, LTT 10108, SAO 36248

M2V

0.4 M☉

11.6 ly

Groombridge 34 B

GQ Andromedae, Gliese 15 B, G 171-048, LHS 4, LTT 10109

M4.1 V

0.16 M☉

11.6 ly

DX Cancri

Gliese 1111, GJ 1111, G 051-015, GCTP 2016.01, LHS 248, G 51-15, DX Cnc

M6.5 V

0.09 M☉

11.7 ly

Gliese 1061

LHS 1565, LFT 295, LTT 1702, LP 995-46, L 372-58, GJ 1061

M5.5 V

0.11 M☉

12 ly

YZ Ceti

GCTP 248.01, Gliese 54.1, GJ 54.1, G 268-135, LHS 138, LTT 670, L 725-32, HIP 5643, YZ Cet

M4 Ve

0.13 M☉

12.1 ly

Красные карлики Новости

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

TOI-2257 b represents a unique case in planetary science due to its 35-day orbital period and high eccentricity, which describes how much an orbit deviates from a perfect circle. Located in a sparsely populated region of planetary parameter space, it sits at a critical threshold where the combined effects of stellar radiation and tidal forces - gravitational stresses caused by the host star - begin to lose their influence over the planet. Simulations show that the planet remains near this transi...

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Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class

6. 10. 2026

Image: Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class

Analysis of sub-Neptune planets around Red dwarf stars using JWST data reveals a new category of hybrid worlds. These planets have atmospheric compositions that do not align with traditional gas dwarf or water world definitions. Study highlights include TOI-776 c....

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Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere

3. 10. 2026

Звезды | Экзопланеты | Красные карлики | Космический телескоп имени Джеймса Уэбба | Атмосферы планет

Image: Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere

Analysis of four transit observations of TRAPPIST-1 c shows the planet is likely airless. By using a new method to account for stellar activity, researchers ruled out thick carbon dioxide and nitrogen atmospheres for this rocky exoplanet....

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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

	WISE 0855-0714 7.3 ly			Water Cloud and Chemical Modulations in the Coldest Brown Dwarf 17. 10. 2026
	WASP 94 687 ly			A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum 16. 10. 2026
	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

Список Красные карлики