Rote Zwerge | Stellar Catalog

	Mass	Distance
LP 816-60 LP 816-060, HIP 103039, NLTT 50038, TYC 6348-400-1, 2MASS J20523304-1658289	M3.5 V	0.19 M☉	18.3 ly
Gliese 205 Wolf 1453, BD-03° 1123, GJ 205, HD 36395, HIP 25878, LHS 30, SAO 132211, W. B. V. 592, Weisse I, 5h 592, Strb. 1611, Cin. 705, Ci 20=334, G 99-15, LFT 416, LTT 2293, NLTT 15215 PLX 1255, TYC 4770-574-1, 2MASS J05312734-0340356	M1.5 V	0.56 M☉	18.6 ly
Gliese 229 HD 42581, HIP 29295, LHS 1827, NSV 2863, SAO 171334, TYC 5945-765-1, WISE J061034.53-215200.3, GJ 229	M1.5 V	0.58 M☉	18.8 ly
Ross 47 Gliese 213, V1352 Ori, HIP 26857, Ci 20 344, G 102-22, LFT 425, LHS 31, LTT 11704, NLTT 15489, Ross 47, TYC 722-455-1, 2MASS J05420897+1229252	M4 V	0.35 M☉	18.9 ly
33 G. Librae C	M3 V	0.35 M☉	19 ly
Gliese 693 HIP 86990, Ci 20 1061, L 205-128, LFT 1372, LHS 454, LPM 655, LTT 7067, NLTT 45375, PLX 4040, GJ 693	M2 V	0.26 M☉	19.2 ly
Gliese 754 Luyten 347-14, LHS 60, LFT 1469, LTT 7652, NLTT 47673, 2MASS J19204795-4533283, L 347-14, GJ 754	M4.5 V	0.18 M☉	19.3 ly
Gliese 908 BR Piscium, HIP 117473, SAO 128397, PPM 174453, G 29-68, G 31-6, GJ 908, LHS 550, LTT 17014, Lalande 46650, BR Psc	M1V	0.37 M☉	19.3 ly
Gliese 752 Ross 652, Wolf 1055, Van Biesbroecks, VB 10, V1428 Aql, HD 180617, HIP 94761, TYC 472-1252-1, GSC 00472-01252, 2MASS J19165526+051008	M2.5	0.46 M☉	19.3 ly
Gliese 588 CD-40 9712, HIP 76074, LHS 397, LTT 6210, TYC 7844-1976-1, 2MASS J15321302-4116314, GJ 588	M2.5 V	0.46 M☉	19.3 ly
Gliese 752 B	M8 V	0.08 M☉	19.3 ly
33 G. Librae B HD 131976, HN 28B, DENIS J145726.4-212439, GJ 570 B, HIC 73182, HIP 73182, JP11 2550, LFT 1160, LHS 386, LPM 550, LTT 5948, 2MASS J14572643-2124384, NLTT 38871	M1 V	0.55 M☉	19.3 ly
Furuhjelm 46 Gliese 661, HD 155876, LFT 1326, LFT 1327, LTT 15095, LHS 433, NLTT 44362, LTT 15096, LHS 434, NLTT 44363	M3V	0.32 M☉	19.5 ly
Furuhjelm 46 B	M3.5	0.29 M☉	19.5 ly
YZ Canis Minoris Ross 882, Gliese 285, GJ 285, TYC 183-2190-1, YZ CMI, BD+35° 2496, HIP 37766, SAO 63793, G 50-4, G 112-46, LFT 547, LHS 1943, LSPM J0744+0333, LTT 12064, NLTT 18373, PLX 1827, PM 07421+0341	M4 V	0.31 M☉	19.5 ly
279 G. Sagittari B HD 191408B, LHS 486	M4 V	0.24 M☉	19.6 ly
QY Aurigae Gliese 268, Ross 986, QY Aur, HIP 34603, G 87-26, G 07-51, LFT 512, LHS 226, LTT 11987, TYC 2944-1956-1, V* QY Aur	M4.5Ve	0.23 M☉	19.7 ly
QY Aurigae B	M5Ve	0.19 M☉	19.8 ly
Gliese 784 CD−45 13677, HD 191849, HIP 99701, SAO 230110, PPM 325963, Ci 20 1196, LFT 1532, LHS 3531, LPM 730, LTT 7999, NLTT 48880, PLX 4794, PM 20103-4519, TYC 8392-2673-1, 2MASS J20135335-4509506	M0V	0.58 M☉	20.1 ly
Gliese 555 Wolf 1481, HN Lib, BD-11 3759, HIP 71253, Ci 20 870, LFT 1120, LHS 2945, LPM 532, LTT 5759, GJ 555	M3.5 V	0.29 M☉	20.4 ly

Sternname

Mass

Distance

LP 816-60

LP 816-060, HIP 103039, NLTT 50038, TYC 6348-400-1, 2MASS J20523304-1658289

M3.5 V

0.19 M☉

18.3 ly

Gliese 205

Wolf 1453, BD-03° 1123, GJ 205, HD 36395, HIP 25878, LHS 30, SAO 132211, W. B. V. 592, Weisse I, 5h 592, Strb. 1611, Cin. 705, Ci 20=334, G 99-15, LFT 416, LTT 2293, NLTT 15215 PLX 1255, TYC 4770-574-1, 2MASS J05312734-0340356

M1.5 V

0.56 M☉

18.6 ly

Gliese 229

HD 42581, HIP 29295, LHS 1827, NSV 2863, SAO 171334, TYC 5945-765-1, WISE J061034.53-215200.3, GJ 229

M1.5 V

0.58 M☉

18.8 ly

Ross 47

Gliese 213, V1352 Ori, HIP 26857, Ci 20 344, G 102-22, LFT 425, LHS 31, LTT 11704, NLTT 15489, Ross 47, TYC 722-455-1, 2MASS J05420897+1229252

M4 V

0.35 M☉

18.9 ly

33 G. Librae C

M3 V

0.35 M☉

19 ly

Gliese 693

HIP 86990, Ci 20 1061, L 205-128, LFT 1372, LHS 454, LPM 655, LTT 7067, NLTT 45375, PLX 4040, GJ 693

M2 V

0.26 M☉

19.2 ly

Gliese 754

Luyten 347-14, LHS 60, LFT 1469, LTT 7652, NLTT 47673, 2MASS J19204795-4533283, L 347-14, GJ 754

M4.5 V

0.18 M☉

19.3 ly

Gliese 908

BR Piscium, HIP 117473, SAO 128397, PPM 174453, G 29-68, G 31-6, GJ 908, LHS 550, LTT 17014, Lalande 46650, BR Psc

M1V

0.37 M☉

19.3 ly

Gliese 752

Ross 652, Wolf 1055, Van Biesbroecks, VB 10, V1428 Aql, HD 180617, HIP 94761, TYC 472-1252-1, GSC 00472-01252, 2MASS J19165526+051008

M2.5

0.46 M☉

19.3 ly

Gliese 588

CD-40 9712, HIP 76074, LHS 397, LTT 6210, TYC 7844-1976-1, 2MASS J15321302-4116314, GJ 588

M2.5 V

0.46 M☉

19.3 ly

Gliese 752 B

M8 V

0.08 M☉

19.3 ly

33 G. Librae B

HD 131976, HN 28B, DENIS J145726.4-212439, GJ 570 B, HIC 73182, HIP 73182, JP11 2550, LFT 1160, LHS 386, LPM 550, LTT 5948, 2MASS J14572643-2124384, NLTT 38871

M1 V

0.55 M☉

19.3 ly

Furuhjelm 46

Gliese 661, HD 155876, LFT 1326, LFT 1327, LTT 15095, LHS 433, NLTT 44362, LTT 15096, LHS 434, NLTT 44363

M3V

0.32 M☉

19.5 ly

Furuhjelm 46 B

M3.5

0.29 M☉

19.5 ly

YZ Canis Minoris

Ross 882, Gliese 285, GJ 285, TYC 183-2190-1, YZ CMI, BD+35° 2496, HIP 37766, SAO 63793, G 50-4, G 112-46, LFT 547, LHS 1943, LSPM J0744+0333, LTT 12064, NLTT 18373, PLX 1827, PM 07421+0341

M4 V

0.31 M☉

19.5 ly

279 G. Sagittari B

HD 191408B, LHS 486

M4 V

0.24 M☉

19.6 ly

QY Aurigae

Gliese 268, Ross 986, QY Aur, HIP 34603, G 87-26, G 07-51, LFT 512, LHS 226, LTT 11987, TYC 2944-1956-1, V* QY Aur

M4.5Ve

0.23 M☉

19.7 ly

QY Aurigae B

M5Ve

0.19 M☉

19.8 ly

Gliese 784

CD−45 13677, HD 191849, HIP 99701, SAO 230110, PPM 325963, Ci 20 1196, LFT 1532, LHS 3531, LPM 730, LTT 7999, NLTT 48880, PLX 4794, PM 20103-4519, TYC 8392-2673-1, 2MASS J20135335-4509506

M0V

0.58 M☉

20.1 ly

Gliese 555

Wolf 1481, HN Lib, BD-11 3759, HIP 71253, Ci 20 870, LFT 1120, LHS 2945, LPM 532, LTT 5759, GJ 555

M3.5 V

0.29 M☉

20.4 ly

Rote Zwerge nachricht

Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

15. 10. 2026

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

6. 10. 2026

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

3. 10. 2026

Sterne | Exoplaneten | Rote Zwerge | James-Webb-Weltraumteleskop | Planetenatmosphäre

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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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.

Sterne

Sterne sind riesige Kugeln aus heißem Gas, die durch Kernfusion in ihrem Inneren Energie erzeugen und dadurch leuchten. Die meisten Sterne bestehen hauptsächlich aus Wasserstoff und Helium. Im Zentrum eines Sterns verschmelzen Wasserstoffatome aufgrund des hohen Drucks und der Temperatur zu Helium, wobei eine enorme Menge Energie in Form von Licht und Wärme freigesetzt wird.

More about Sterne

Random terms

Sternposition Leuchtkraft Sterntemperatur Sternmasse Sterngröße Sternenalter

	WISE 0855-0714 7.3 ly			Water Cloud and Chemical Modulations in the Coldest Brown Dwarf 17. 10. 2026
	WASP 94 687 ly			A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum 16. 10. 2026
	KELT-2 439 ly			Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity 15. 10. 2026
	TOI-2257 189 ly			The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b 15. 10. 2026
	KELT-18 1032 ly			High-resolution transmission spectroscopy of KELT-18b Metastable helium detection at 1083 nm 14. 10. 2026

Liste der Rote Zwerge

Rote Zwerge nachricht

Research in Rote Zwerge

Frequently Asked Questions about nearby stars

What is the nearest star?

What are the nearest stars to Earth?

What is the solar neighborhood?

How do astronomers measure distances to stars?

Are there any exoplanets orbiting the nearest stars?

Why are the nearest stars important for astronomy and physics?

StellarGuide: Sterne