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Seznam nejbližších Červení trpaslíci

        
    
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Hvězdy 201-220
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Název hvězdy Mass Distance

FK Aquarii B
FL Aqr, V* FL Aqr
M3.5V C 0.42 M☉ 28.9 ly

Gliese 465
LHS 45, Ross 695, HIP 60559
dM2.0 0.23 M☉ 28.9 ly

SCR J0630-7643
SIPS J0630-7643, 2MASS J06304661-7643094
M6 Ve - 29 ly

SCR J0630-7643 B
** HEN 4B, WDS J06308-7643B, Gaia DR2 5260451999698559872, SCR J0630-7643B
- 29 ly

Gaia DR2 2090670890062670080
M8 - 29 ly

Xi Ursae Majoris Ab
M V 0.38 M☉ 29 ly

Xi Ursae Majoris Bb
M V 0.14 M☉ 29 ly

FK Aquarii
FK Aqr, Gliese 867, HD 214479, HIP 111802, BD-21 6267, FL Aquarii
M1 Ve 0.42 M☉ 29 ly

Gliese 2066
HIP 40501, HIC 40501 G 113-20, NLTT 19217
M2 V 0.46 M☉ 29.2 ly

Gliese 3421
G 193-27, LHS 224, LP 122-59, LTT 11965, LFT 506, L 1750-5
M5 V 0 M☉ 29.4 ly

LP 388-55
M7.5+L0 - 29.5 ly

SZ Ursae Majoris
V* SZ UMa, Gliese 424, GJ 424, HIC 55360, HIP 55360, LFT 795, LHS 41, LTT 13056, BD+66 717, NLTT 27039, MCC 38, G 236-65, 2MASS J11200526+6550470
M2 V - 29.6 ly

Gliese 433
HIP 56528, CD-31 9113, LHS 2429, LTT 4290, NLTT 27914, SAO 202602, Ci 20 649, L 907-1, PM J11354-3232, UGP 270, CPC 17 5737, GJ 433
M1.5 V 0.48 M☉ 29.6 ly

HD 115953
HU 644A, CHR 193, ADS 8862 A, BD+48 2108A, GJ 508 A, TYC 3460-2162-1, Gliese 508 A
M2V - 29.7 ly

HD 115953 B
BD+48 2108B, HU 644B, ADS 8862 B, GJ 508 B, TYC 3460-2162-2
- 29.7 ly

Gliese 3146
LP 469-206, LHS 1375, NLTT 7501, 2MASS J02162977+1335136, NN 3146
M5 Ve 0.05 M☉ 29.7 ly

V374 Pegasi
V* V374 Peg, G 188-38, Gliese 4247, HIP 108706, HIC 108706, 2MASS J22011310+2818248, NLTT 52699
M3.5 V 0 M☉ 29.7 ly

WT 460
2MASS J14115998-4132211, DENIS J141159.9-413221, TIC 179615113, WDS J14120-4132AB, WISEA J141159.27-413222.5
M5.5e - 29.7 ly

Gliese 283 B
LHS 234, LUY 5693B, CCDM J07402-1725B, GJ 283 B, LFT 544, L 745-46 B, LP 783-2, LTT 2916, 2MASS J07401922-1724449, NLTT 18270, TIC 289113766
M6.5 V 0.2 M☉ 29.9 ly

Gliese 3801
Ross 1015, LHS 2784, LTT 13999, StKM 2-972, G 165-25, HIC 66906, HIP 66906
M3.5 V 0 M☉ 30 ly
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Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A
iconToday
iconHvězdy | Exoplanety | Červení trpaslíci | TESS
Image: Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774 A
A small planet candidate has been identified in the binary star system known as Gliese 774. The object, which is smaller than the Earth, orbits its host star approximately every 4.2 days. Observations from the Transiting Exoplanet Survey Satellite (TESS) captured the planet as it passed in front of its star, briefly blocking a tiny fraction of the starlight. This periodic dimming event allowed for the identification of the candidate despite the complex environment of a binary system, where two s...
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Ammonia and hydrogen may separate inside Uranus and Neptune
iconToday
iconHvězdy | Exoplanety | Červení trpaslíci
Image: Ammonia and hydrogen may separate inside Uranus and Neptune
Uranus and Neptune may be experiencing ammonia rain: simulations show their expected temperature profiles cross the boundary where ammonia and hydrogen separate. In warmer sub-Neptune TOI-270 d, the two are likely to mix in all proportions....
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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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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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