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Оранжевые карлики
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Звезды 121-140
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Имя звезды Mass Distance

BD+40 45
 K7 - 47.9 ly

HD 142709
LTT 6359, GJ 604, Gliese 604, HIC 78170, HIP 78170, 2MASS J15574075-4237271, NLTT 41579, TIC 255263370, TYC 7846-245-1, WISEA J155740.51-423729.2
 K4V - 48.1 ly

Gliese 259
GJ 259, HD 52698
 K1V - 48.1 ly

HD 176051 B
 K1V 0.71 M☉ 48.1 ly

BD+33 529
 K4 - 48.2 ly

Gliese 833
HD 205390, HIP 106696, SAO 247109, GJ 833
 K1V 0.77 M☉ 48.3 ly

HD 144628
GJ 613.0, Gliese 613.0, LTT 6436, LF 15 -56 39, HIC 79190, HIP 79190, 2MASS J16094280-5626430, NLTT 42064, TIC 206828302, TYC 8718-1921-1, WISEA J160942.57-562639.5
K2V - 48.4 ly

HD 218511
HIP 114361, Gliese 1279, GJ 1279, TYC-9338-287-1
 K6V - 48.4 ly

AB Doradus
AB Dor, CD−65° 332, HD 36705, HIC 25647, HIP 25647
 K0V 0.86 M☉ 48.4 ly

Gaia EDR3 5970971561918864768
 - 48.5 ly

Alpha Ophiuchi B
 K5-7V 0.85 M☉ 48.6 ly

CD-49 2340
 K8Vk: - 49.1 ly

HD 200779
HIP104092, Gliese 818, GL 818, TYC-538-1647-1, BD+06 4741
 K6V - 49.1 ly

BD+63 137
GJ 52, Gliese 52, LHS 136, G 244-13, G 243-60, HIP 5247, LFT 104, LSPM J0107+6356, LTT 10390, 2MASS J01070794+6356284, TIC 52626846, TYC 4025-626-1, Wolf 54, WISEA J010710.56+635632.0
 K7V C - 49.1 ly

HD 118926
 K5V - 49.3 ly

HD 238090
G 197-49, BD+55 1519, Gliese 458 A, GJ 458 A, HIC 59514, HIP 59514, LSPM J1212+5429S, LTT 13395, NLTT 29950, 2MASS J12122084+5429086, MCC 137, TIC 224289449, TYC 3834-814-1, WDS J12123+5429A, WEB 10581
 K5V C 0.58 M☉ 49.7 ly

HD 24916
NS 0357-0109 A, Gliese 157, GJ 157 A, HIP 18512, BD-01 565, LTT 1830
 K4V - 49.9 ly

HD 21197
LHS 1546, Gliese 141, GJ 141, HIP 15919, 2MASS J03245975-0521489, TIC 279182339, TYC 4715-1106-1, WISEA J032459.59-052157.2, NLTT 10867, LFT 282
K4V - 50 ly

HD 4967
2MASS J00513400-2254361, G 268-60, GJ 40, Gliese 40, HIP 4022, L 652-35, LFT 81, LHS 1159, LTT 490, TYC 6422-1073-1, WISEA J005134.49-225439.1, Gaia DR2 2349206308999273984
 K5V - 50.1 ly

HD 3443 B
TYC 6421-1924-2
 K0.5V 0.86 M☉ 50.2 ly
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Оранжевый карлик Новости

Sub-Neptune planet candidate observed orbiting the orange dwarf star TIC 402710280
iconToday
iconЗвезды | 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
icon18. 10. 2026
iconЗвезды | 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
icon14. 10. 2026
iconЗвезды | 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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study iconResearch in Оранжевые карлики

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Просмотрите последние научные исследования звезд и экзопланет в нашей галактике. Откройте для себя новейшие исследования в области астрофизики и звездной астрономии.
Текущее исследование

 WISE 0855-0714
7.3 ly
 study icon Water Cloud and Chemical Modulations in the Coldest Brown Dwarf
17. 10. 2026

HD 203771
184 ly
 study icon 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 study icon Gaseous SiO and Silicate Clouds in Three Benchmark Early-L Dwarfs
9. 10. 2026

DENIS J1253-5709
54.4 ly
 study icon 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
 study icon A Jupiter-like radio aurora in the L3.5 dwarf LSPM J0036+1821
9. 10. 2026
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Старые публикации

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.
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exoplanet iconStellarGuide: Звезды

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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.
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