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Seznam nejbližších Červení trpaslíci

        
    
Více o Červení trpaslíci
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Hvězdy 161-180
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Název hvězdy Mass Distance

Mu Herculis C
M3.5 V 0.39 M☉ 27.1 ly

Gliese 747 B
M3 V - 27.1 ly

Gliese 747
G 207-16, KUI 90, LFT 1451, LHS 471, L 1499-28, LP 336-6, LTT 15603, NLTT 47437
M3 V - 27.1 ly

Mu Herculis Ab
M4 V 0.32 M☉ 27.2 ly

Mu Herculis B
mu.02 Her
M3.5 V 0.44 M☉ 27.2 ly

Gliese 1227
LHS 465, G 227-29, LP 103-305, NLTT 46427, 2MASS J18222719+6203025
M4 V - 27.2 ly

Gliese 1289
G 130-4, LHS 4003, 2MASS J23430628+3632132, NLTT 57748, G 190-43, GJ 1289, TIC 352593978, WISEA J234307.14+363211.5
M4.5 V 0.21 M☉ 27.3 ly

2MASS J18352–3123
2MASS J18352154–3123385, 1RXS J183520.9−312327
M6.5V 0 M☉ 27.3 ly

2MASS J18352–3123 B
2MASS J18352205−3123421
M8 V - 27.3 ly

SCR 1138-7721
2MASS J11381671-7721484, WISEA J113810.11-772142.2, SCR J1138-7721
M5 V 0.18 M☉ 27.3 ly

2MASS J1546-5534
2MASS J15464185-5534468, DENIS J154641.8-553446, SCR J1546-5534, WISEA J154640.78-553446.0
M7.5 0.2 M☉ 27.4 ly

Gliese 185 B
0.37 M☉ 27.4 ly

TYC 3980-1081-1
IRAS 21500+5903, 2MASS J21513828+5917383
M3.9 0.2 M☉ 27.6 ly

Gliese 232
Ross 64, JP11 5117, LHS 1846, LFT 467, G 104-37, LTT 11838, Ci 20 385
M4 V 0 M☉ 27.7 ly

Gliese 618 B
LHS 416, LFT 1267, L 482-31, LTT 6509
M5 0 M☉ 27.7 ly

Gliese 618
CD-37 10765, LHS 415, LDS 6312, L 482-30, LFT 1266, LTT 6508, NLTT 42493, 2MASS J16200353-3731449, TYC 7853-670-1
M3 V - 27.8 ly

Gliese 493.1
Wolf 461, V* FN Vir, G 60-55, G 62-5, LFT 962, LHS 2664, LTT 13750, NLTT 32583, 2MASS J13003350+0541081
M4.5 Ve 0 M☉ 27.9 ly

Gliese 3454
LTT 17993, G 89-32, Nl 654, HEN 3, 2MASS J07362513+0704431, NLTT 18152
M4.5 V 0.15 M☉ 28 ly

Gliese 3454 B
M4 V 0.13 M☉ 28 ly

Gliese 877
HIP 113229, LHS 531, L 49-19, Ci 20 1389, GJ 877, HIC 113229, LFT 1747, 2MASS J22554532-7527320, NLTT 55234, Gaia DR2 6378584028690858496
M3 V 0 M☉ 28 ly
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Červení trpaslíci zprávy

Ammonia and hydrogen may separate inside Uranus and Neptune
iconToday
iconHvězdy | Exoplanety | Červení trpaslíci
Image: Ammonia and hydrogen may separate inside Uranus and Neptune
Ammonia and hydrogen can separate into distinct, hydrogen-rich and ammonia-rich phases under conditions expected inside some planets. Simulations indicate that the boundary between mixing and separation crosses published temperature profiles for Uranus and Neptune. This suggests ammonia may be raining out inside both planets today, moving from their hydrogen-rich envelopes into ammonia-rich regions. The simulations covered temperatures from 500 to 4,000 kelvins and pressures from 0.1 to 100 g...
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Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b
icon15. 10. 2026
iconHvězdy | Exoplanety | Červení trpaslíci | Superzemě | Atmosféry planet | TESS
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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Atmospheric composition of sub-Neptune planets around Red dwarf stars reveals new hybrid class
icon6. 10. 2026
iconHvězdy | Exoplanety | Červení trpaslíci | Vesmírný dalekohled Jamese Webba | Atmosféry planet | Oceánské planety
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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study iconResearch in Červení trpaslíci

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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.
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exoplanet iconStellarGuide: Hvězdy

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Hvězdy
Hvězdy jsou obrovské koule horkého plynu, které září díky energii vznikající jadernou fúzí v jejich jádru. Většina hvězd se skládá převážně z vodíku a helia. V centru hvězdy dochází díky vysokému tlaku a teplotě k přeměně vodíku na helium, přičemž se uvolňuje obrovské množství energie ve formě světla a tepla.
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