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Звезды 81-100
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Имя звезды Mass Distance

44 Boötis C
 K4V - 42.2 ly

HD 27274
CD−53° 889, GJ 167, Gliese 167, HIC 19884, HIP 19884, SAO 233456
 K4.5Vk: 0.74 M☉ 42.5 ly

HD 211970
LTT 8985, CD-55 9073, Gliese 1267, GJ 1267, HIC 110443, HIP 110443, 2MASS J22221621-5433383, NLTT 53616, TIC 231704229, TYC 8822-210-1, WISEA J222215.97-543335.6
 K7Vk: C 0.61 M☉ 42.8 ly

HD 170657
NSV 10944, Gliese 716, GJ 716, HD 170657, HIC 90790, HIP 90790, SAO 161557, WDS J18313-1855A, LTT 7358
 K2V 0.79 M☉ 43 ly

HD 29697
V834 Tau, V834 Tauri, BD+20° 802, GJ 174, Gliese 174, HD 29697, HIC 21818, HIP 21818, SAO 76708
 K4V 0.75 M☉ 43.1 ly

HD 128165
HIC 71181, HIP 71181, SAO 29196, Gliese 556, GJ 556, GL 556, TYC-3860-1045-1, BD+53 1719
 K3V 0.78 M☉ 43.2 ly

HD 214749
LTT 9143, GJ 868.0, Gliese 868.0, PLX 5486, UBV 19400, CD-30 19255, HD 214749, PLX 5486.00, UBV M 26543, CPC 17 12286, HIC 111960, PPM 274115, UGP 576, CPD-30 6663, HIP 111960, SAO 191319, WISEA J224043.67-294028.1, GCRV 73405, IRAS 22379-2955, SKY# 43116, Gaia DR1 6608490497012980224, GEN# +1.00214749, 2MASS J22404335-2940278, TIC 47295522, Gaia DR2 6608490501308343168, GJ 868, Gliese 868, NLTT 54520, TYC 6969-1175-1
 K4.5Vk - 43.3 ly

HD 120476 B
 K6V - 44 ly

BD+62 780
 K7V - 44 ly

HD 120476
Gl 528, Gliese 528, HIC 67422, HIP 67422, LHS 6259, LTT 14035, NLTT 35353, BD+27 2296,
K4V - 44 ly

HD 10436
BD+63° 229, Gliese 69, GJ 69, HD 10436, HIP 8070, SAO 11943, LHS 1291
 K5Vbe 0.62 M☉ 44.1 ly

HD 145417
GJ 615, Gliese 615, LHS 413, HIC 79537, HIP 79537, LFT 1255, LTT 6464, NLTT 42227, 2MASS J16134869-5734118, TIC 207556694, TYC 8719-359-1, WISEA J161347.46-573428.1
 K3VFe-1.7 - 44.3 ly

HD 22496
CD−48° 1011, GJ 146, Gliese 146, HIC 16711, HIP 16711, LTT 1698, SAO 85397, 2MASS J03350093-4825089
 K5/M0V 0.68 M☉ 44.4 ly

HD 98712
BD-19 3242, HIC 55454, HIP 55454, PM J11214-2027, TYC 6090-1868-1, WISE J112126.79-202714.3, SZ Crateris, SZ Crt, GJ 425, GJ 425A, Gliese 425, SAO 179801
 K7V - 44.8 ly

HD 154577
CD-60 6576, GCTP, Gliese 656, GJ 656, HD 154577, HIC 83990, HIP 83990, LHS 3268, LTT 6833, SAO 253819
 K2.5Vk: 0.68 M☉ 44.8 ly

V439 Andromedae
BD+28°4704, GC 95, GSC 01735-02532, GSC 01735-00927, GJ 5, Gliese 5, HD 166, HIP 544, HR 8, SAO 73743, NSV 33
 K0Ve 0.89 M☉ 44.9 ly

BD+39 2376
NS 1045+3830, Gliese 400, GJ 400, HIP 52600, BD+39 2376, CCDM J10454+3831AB
 K7/M0V - 45.2 ly

HD 281621
LHS 1634, HIC 19337, HIP 19337, GL 162, Gliese 162, TYC-2362-37-1
 K7V - 45.4 ly

HD 23356
HIP 17420, BD -19 733, N1 354, LTT1759, NS 0343-1906
 K2V - 45.5 ly

HD 5133
BD−31° 325, Gaia DR2 5031808453624044800, Gliese 42, GJ 42, HD 5133, HIC 4148, HIP 4148, SAO 192793, LTT 498, 2MASS J00530108-3021249
 K2.5Vk: - 45.5 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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