Оранжевые карлики

	Mass	Distance
Delta Capricorni B	K/G	0.73 M☉	38 ly
HD 99279 B GJ 428 B, Gliese 428 B, TYC 8959-1969-1, TIC 315311765, 2MASS J11243947-6138542	K7	0.62 M☉	38.1 ly
Zeta Doradus B GJ 1075, Gliese 1075, HIC 23708, HIP 23708		0.53 M☉	38.1 ly
Gliese 572 B BD+45 2247B	K7V	-	38.2 ly
Gliese 414 HD 97101, GJ 414 A, LHS 2367, DO 14370, G 119-60, G 120-23, G 147-28, HIC 54646, HIP 54646, LFT 767, LTT 13009, NLTT 26534, 2MASS J11110509+3026459, TIC 9001920, TYC 2520-2524-1, WDS J11111+3027A, WISEA J111105.67+302643.6	K7V	0.65 M☉	38.7 ly
HD 99279 DENIS J112440.3-613851, GJ 428, Gliese 428, 2MASS J11244030-6138512, TIC 315311759, TYC 8959-1969-2, WISEA J112439.38-613851.3	K5-V	0.79 M☉	39.5 ly
HD 72673 11 G. Pyxidis, CD−31° 6229, GJ 309, Gliese 309, HD 72673, HIP 41926, HIC 41926, HR 3384, SAO 199352, LHS 249, LTT 3168	K1V	0.75 M☉	39.7 ly
V538 Aurigae V538 Aur, NSV 16618, BD+53° 934, GJ 211, Gliese 211, HD 37394, HIC 26779, HIP 26779, HR 1925, WDS J05413+5329A	K1	0.87 M☉	40 ly
85 Pegasi B ADS 17175 B, GJ 914 B, BD +26°4734 B, BU 733 B		0.55 M☉	40.2 ly
HD 196877	K7V	-	40.3 ly
HD 175224 B	K7Ve	-	40.3 ly
HD 175224 HIC 93069, HIP 93069, IRAS 18532-5603, TIC 379470817, WDS J18575-5600AB, WISEA J185730.57-555934.2	K5Ve	-	40.3 ly
HD 21531	K5V	-	40.7 ly
HD 190007 V1654 Aql, V1654 Aquilae, BD+02° 4076, GJ 775, Gliese 775, HD 190007, HIC 98698, HIP 98698, SAO 125379, GC 27782, 2MASS J20024703+0319344, SAO 125379, TIC 345217789, TYC 498-2720-1, USNO-B1.0 0933-00588224, WISE J200246.98+031935.5	K5V B	0.68 M☉	41.5 ly
HD 101581 LHS 2441, CD-43 7228, GJ 435, Gliese 435, HIC 56998, HIP 56998, LFT 835, LTT 4333, 2MASS J11410247-4424184, NLTT 28235, TIC 397362481, TYC 7753-1657-1, WISEA J114101.82-442416.0	K4.5Vk:	0.74 M☉	41.7 ly
HD 82106 TYC 234-468-1, HIC 46580, HIP 46580, Gliese 349, GJ 349	K3V	0.79 M☉	41.7 ly
HD 158633 BD+67°1014, Gliese 675, GJ 675, HD 158633, HIC 85235, HIP 85235, HR 6518, SAO 17474, LHS 287, LTT 15185	K0V	0.73 M☉	41.7 ly
36 Ursae Majoris B * 36 UMb	K7Ve	-	42.1 ly
Gliese 204 GJ 204, HD 36003, BD-03 1110, 2MASS J0528-0329, 2MASS J05282613-0329576, SAO 132145, HIC 25623, HIP 25623, TYC 4757-1577-1, GC 6757, LFT 412, LHS 1763	K5V	0.75 M☉	42.2 ly
HD 40307 CD−60 1303, CPD−60 508, GC 7474, Gliese 2046, GJ 2046, HIC 27887, HIP 27887, PPM 355061, SAO 249388, 2MASS J05540421-6001245, TIC 374859347, TYC 8892-1247-1	K2.5V C	0.75 M☉	42.2 ly

Имя звезды

Mass

Distance

Delta Capricorni B

K/G

0.73 M☉

38 ly

HD 99279 B

GJ 428 B, Gliese 428 B, TYC 8959-1969-1, TIC 315311765, 2MASS J11243947-6138542

0.62 M☉

38.1 ly

Zeta Doradus B

GJ 1075, Gliese 1075, HIC 23708, HIP 23708

0.53 M☉

38.1 ly

Gliese 572 B

BD+45 2247B

K7V

38.2 ly

Gliese 414

HD 97101, GJ 414 A, LHS 2367, DO 14370, G 119-60, G 120-23, G 147-28, HIC 54646, HIP 54646, LFT 767, LTT 13009, NLTT 26534, 2MASS J11110509+3026459, TIC 9001920, TYC 2520-2524-1, WDS J11111+3027A, WISEA J111105.67+302643.6

K7V

0.65 M☉

38.7 ly

HD 99279

DENIS J112440.3-613851, GJ 428, Gliese 428, 2MASS J11244030-6138512, TIC 315311759, TYC 8959-1969-2, WISEA J112439.38-613851.3

K5-V

0.79 M☉

39.5 ly

HD 72673

11 G. Pyxidis, CD−31° 6229, GJ 309, Gliese 309, HD 72673, HIP 41926, HIC 41926, HR 3384, SAO 199352, LHS 249, LTT 3168

K1V

0.75 M☉

39.7 ly

V538 Aurigae

V538 Aur, NSV 16618, BD+53° 934, GJ 211, Gliese 211, HD 37394, HIC 26779, HIP 26779, HR 1925, WDS J05413+5329A

0.87 M☉

40 ly

85 Pegasi B

ADS 17175 B, GJ 914 B, BD +26°4734 B, BU 733 B

0.55 M☉

40.2 ly

HD 196877

K7V

40.3 ly

HD 175224 B

K7Ve

40.3 ly

HD 175224

HIC 93069, HIP 93069, IRAS 18532-5603, TIC 379470817, WDS J18575-5600AB, WISEA J185730.57-555934.2

K5Ve

40.3 ly

HD 21531

K5V

40.7 ly

HD 190007

V1654 Aql, V1654 Aquilae, BD+02° 4076, GJ 775, Gliese 775, HD 190007, HIC 98698, HIP 98698, SAO 125379, GC 27782, 2MASS J20024703+0319344, SAO 125379, TIC 345217789, TYC 498-2720-1, USNO-B1.0 0933-00588224, WISE J200246.98+031935.5

K5V B

0.68 M☉

41.5 ly

HD 101581

LHS 2441, CD-43 7228, GJ 435, Gliese 435, HIC 56998, HIP 56998, LFT 835, LTT 4333, 2MASS J11410247-4424184, NLTT 28235, TIC 397362481, TYC 7753-1657-1, WISEA J114101.82-442416.0

K4.5Vk:

0.74 M☉

41.7 ly

HD 82106

TYC 234-468-1, HIC 46580, HIP 46580, Gliese 349, GJ 349

K3V

0.79 M☉

41.7 ly

HD 158633

BD+67°1014, Gliese 675, GJ 675, HD 158633, HIC 85235, HIP 85235, HR 6518, SAO 17474, LHS 287, LTT 15185

K0V

0.73 M☉

41.7 ly

36 Ursae Majoris B

* 36 UMb

K7Ve

42.1 ly

Gliese 204

GJ 204, HD 36003, BD-03 1110, 2MASS J0528-0329, 2MASS J05282613-0329576, SAO 132145, HIC 25623, HIP 25623, TYC 4757-1577-1, GC 6757, LFT 412, LHS 1763

K5V

0.75 M☉

42.2 ly

HD 40307

CD−60 1303, CPD−60 508, GC 7474, Gliese 2046, GJ 2046, HIC 27887, HIP 27887, PPM 355061, SAO 249388, 2MASS J05540421-6001245, TIC 374859347, TYC 8892-1247-1

K2.5V C

0.75 M☉

42.2 ly

Оранжевый карлик Новости

Sub-Neptune planet candidate observed orbiting the orange dwarf star TIC 402710280

Today

Звезды | Экзопланеты | Оранжевый карлик

Image: Sub-Neptune planet candidate observed orbiting the orange dwarf star TIC 402710280

A potential sub-Neptune planet candidate has been identified orbiting the orange dwarf star TIC 402710280. This star, located about 218 light-years away, was monitored using the Transiting Exoplanet Survey Satellite. A sub-Neptune is a type of planet that is larger than Earth but smaller than Neptune, representing one of the most common types of worlds found in our galaxy. This specific candidate completes a full trip around its host star in approximately 36.34 days. The planet was identified...

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Oscillation patterns in Gliese 570 A and Gliese 783 A reveal new stellar physics

18. 10. 2026

Звезды | Оранжевый карлик

Image: Oscillation patterns in Gliese 570 A and Gliese 783 A reveal new stellar physics

New measurements of orange dwarfs Gliese 570 A and Gliese 783 A reveal stellar oscillation patterns that challenge current convection models. The observed vibration strengths are steeper than theory predicts, pointing to gaps in our understanding of stellar physics....

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Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf

14. 10. 2026

Звезды | Экзопланеты | Оранжевый карлик | Коричневые карлики

Image: Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf

Massive brown dwarf HD 203771 b confirmed in an eccentric orbit around an orange dwarf star. New mass measurements place the companion at approximately 70 times the mass of Jupiter, revealing insights into how brown dwarfs migrate inward over time....

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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
HD 203771 184 ly		An Intermediate-orbit Brown Dwarf Confirmed with Astrometry+Radial Velocity Joint Analysis, and the Eccentricity Distribution of Brown Dwarfs Across Different Locations 14. 10. 2026
HD 89744 126 ly	+2	Gaseous SiO and Silicate Clouds in Three Benchmark Early-L Dwarfs 9. 10. 2026
DENIS J1253-5709 54.4 ly		Astrometric planet search around southern ultracool dwarfs: V. Discovery of the exoplanet candidate PALTA-1 b 9. 10. 2026
2MASS 0036+1821 28.5 ly		A Jupiter-like radio aurora in the L3.5 dwarf LSPM J0036+1821 9. 10. 2026

Список Оранжевые карлики

Оранжевый карлик Новости

Research in Оранжевые карлики

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