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Seznam nejbližších Červení trpaslíci

        
    
Více o Červení trpaslíci
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Hvězdy 141-160
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Název hvězdy Mass Distance

Gliese 1093
Luyten 399-68, LHS 223, G 109-35, PLX 1635.01, NLTT 17247, 2MASS J06592868+1920577
M5 V 0.21 M☉ 25.3 ly

LP 71-82
G 227-22, LSPM J1802+6415, NLTT 45873, 2MASS J18021660+6415445, 2E 4002, RX J1802.2+6415, TIC 233068870, WISEA J180216.92+641540.2
M5 V - 25.4 ly

Gliese 623
HEN 1, LHS 417, G 202-45, HIC 80346, HIP 80346, LFT 1273, LHS 417, L 1707-1, LTT 14885, NLTT 42730, 2MASS J16240913+4821112
M3 V 0.51 M☉ 25.6 ly

Gliese 623 B
M D 0.06 M☉ 25.6 ly

Gliese 1224
LHS 3359, L 920-26, G 154-44, G 155-1
M4Ve 0.14 M☉ 26 ly

SCR J0740-4257
UCAC4 236-016971, 2MASS J07401183-4257406, PM J07401-4257, TIC 123480394
M4.5 - 26 ly

Gliese 831 B
M4.5 V 0.12 M☉ 26.1 ly

Gliese 257
CD-44 3045, HIC 33499, HIP 33499, LHS 222, LFT 502, LTT 2699, NLTT 17239, LPM 248, Ci 20 407, GJ 257, Gaia DR2 5559035514779133056
M3.5 V 0.25 M☉ 26.2 ly

Gliese 257 B
CD-44 3045B, GJ 257 B, CSI-44 3045 23, LPM 248B
M3 D 0.24 M☉ 26.2 ly

Gliese 1151
G 122-49, LHS 316, PLX 2739.0, NLTT 28752, Zkh 171, GJ 1151, 2MASS J11505787+4822395, TIC 11893637, WISEA J115056.09+482228.4
M4.5Ve C 0.15 M☉ 26.2 ly

Gliese 480.1
LP 399-68, LHS 340, GJ 9415, LFT 935, HIC 61874, HIP 61874, LTT 4836, NLTT 31495, 2MASS J12404633-4333595, TYC 7783-576-1, L 399-68
M3 V 0 M☉ 26.3 ly

Gliese 486
GJ 486, Gl 486, Wolf 437, LHS 341, HIC 62452, HIP 62452, LFT 947, LTT 13654, G 60-32, Ci 20 737, TYC 882-1111-1, NLTT 31933, WISEA J124755.90+094500.2, LSPM J1247+0945, 2MASS J12475664+0945050, PLX 2943
M3.5Ve C 0.32 M☉ 26.4 ly

Gliese 793
HIP 101180, LHS 3558, LTT 15991, G 262-15, LFT 1552, LTT 15991, NLTT 49417, MCC 820
M3 V 0.39 M☉ 26.4 ly

Gliese 1154
LTT 13408, G 13-22, LHS 2531, NLTT 30062, PLX 2817.01, LSPM J1214+0037, 2MASS J12141654+0037263
M4.5 V 0 M☉ 26.4 ly

Gliese 300
L 674-15, LHS 1989, LFT 571, LP 843-1, LTT 3080, NLTT 19136, 2MASS J08124088-2133056, JP11 5131, GJ 300
M3.5 V 0.17 M☉ 26.5 ly

Gliese 686
BD+18 3421, LHS 452, G 170-55, HIC 86287, HIP 86287, L 1278-24, LFT 1363, LTT 15228, NLTT 45173, GJ 686
M1.5 Ve 0.42 M☉ 26.6 ly

L 173-19
NLTT 6772, 2MASS J02003830-5558047, GSC 08485-00936, TIC 231055581
M V 0 M☉ 26.8 ly

Gliese 48
HIP 4856, LHS 131, Ross 318, BD+70 68b, LFT 93, LTT 10362, NLTT 3359, MCC 364, 2MASS J01023213+7140475, Ross 318
M3.5V 0.34 M☉ 26.9 ly

Gliese 54
GKI 3, CD-68 47, CPD-68 41, GALEX 6384743253449642140, LFT 117, LTT 660, LPM 62, LHS 1208, HIC 5496, HIP 5496, 2MASS J01102281-6726425, Gaia DR2 4704272495284592512, NLTT 3945, TIC 52121469, TYC 8855-238-1, NSV 427
M2.5V 0.43 M☉ 26.9 ly

Gliese 54 B
0.3 M☉ 26.9 ly
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Červení trpaslíci zprávy

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
TOI-2257 b represents a unique case in planetary science due to its 35-day orbital period and high eccentricity, which describes how much an orbit deviates from a perfect circle. Located in a sparsely populated region of planetary parameter space, it sits at a critical threshold where the combined effects of stellar radiation and tidal forces - gravitational stresses caused by the host star - begin to lose their influence over the planet. Simulations show that the planet remains near this transi...
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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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Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere
icon3. 10. 2026
iconHvězdy | Exoplanety | Červení trpaslíci | Vesmírný dalekohled Jamese Webba | Atmosféry plane
Image: Observations of TRAPPIST-1 c reveal a likely airless surface without a thick atmosphere
Analysis of four transit observations of TRAPPIST-1 c shows the planet is likely airless. By using a new method to account for stellar activity, researchers ruled out thick carbon dioxide and nitrogen atmospheres for this rocky exoplanet....
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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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