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Liste der sterne

        Unsere Milchstraße enthält Milliarden von Sternen, von massereichen, hellen Sternen bis hin zu kleinen, lichtschwachen Sternenresten. Manche Sterne existieren allein, viele sind Teil von Doppel- oder Mehrfachsternsystemen. Diese Seite präsentiert eine Liste der sonnennächsten Sterne und hilft so, unsere stellare Umgebung zu kartieren und die Vielfalt der Sterne in unserer Nähe zu verstehen.

Die Liste lässt sich nach Sternkategorien filtern, sodass Sie gezielt nach bestimmten Sterntypen wie Roten Zwergen, sonnenähnlichen Sternen, Weißen Zwergen oder Braunen Zwergen suchen können. Diese flexible Ansicht erleichtert den Vergleich verschiedener Sternpopulationen und die Fokussierung auf interessante Objekte. Obwohl der Schwerpunkt auf nahen Sternen liegt, reicht der Katalog auch über die unmittelbare Nachbarschaft hinaus und bietet so einen umfassenderen Überblick über die Sterntypen in unserer Galaxie.
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Sterne 461-480
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Sternname Mass Distance

V* V816 Her
GJ 4071, Gliese 4071, G 141-29, JNN 280A, L 1209-6, LP 510-15, LTT 15516, NLTT 46898, 2MASS J18424498+1354168, TIC 230345672, USNO-B1.0 1039-00345551
 M5V - 35.7 ly

2MASS J15345704-1418486
TIC 386928810, WISEA J153456.27-141852.6
 M8.6V - 35.7 ly

Gliese 519
G 165-19, GJ 519, BD+36 2393, HIC 66459, HIP 66459, LTT 13964, NLTT 34676, 2MASS J13372875+3543039, TIC 73494569, TYC 2543-201-1, WISEA J133729.04+354303.4
 K7.5Ve - 35.7 ly

DN Draconis
V* DN Dra, GJ 1206, Gliese 1206, G 226-29, HIC 82257, HIP 82257, LP 101-148, 2MASS J16482562+5903228, NLTT 43637, TIC 199666369, TYC 3885-860-1, WD 1647+591, WISE J164825.81+590319.6
 DA4.0 - 35.7 ly

LP 851-346
DENIS J115542.9-222458, 2MASS J11554286-2224586, SIPS J1155-2224, TIC 5630425, WISEA J115542.56-222500.7
 M7.5V - 35.7 ly

LP 271-25
GJ 3849, Gliese 3849, FS 134, LHS 2924, 2MASS J14284323+3310391, NLTT 37480, SDSS J142843.13+331036.8, TIC 286963145, WISEA J142842.93+331031.7
 M9Ve - 35.8 ly

CD-45 1184
LTT 1678, CF 1005, GJ 145, Gliese 145, HIC 16536, HIP 16536, NLTT 11234, 2MASS J03325585-4442070, TIC 79568861, TYC 7574-455-1, UCAC4 227-003357
 M2.5V 0.34 M☉ 35.8 ly

LP 853-12
 - 35.8 ly

WISE J014807.25-720258.7
WISEA J014807.34-720258.7, EQ J0148-7202
 T9.5 - 35.8 ly

HD 115404
BD+17° 2611, GJ 505, Gliese 505, HD 115404, HIC 64797, HIP 64797, SAO 100491, LHS 2713, GC 17981, G 63-18, G 149-71, LFT 988, LTT 13853, NLTT 33527, 2MASS J13165106+1701021, TIC 373765355, TYC 1451-1151-1, WISEA J131651.68+170058.2
 K2V 0.7 M☉ 35.8 ly

Gliese 1129
LHS 273, L 750-52, GJ 1129, LFT 681, LP 788-30, LTT 3578, 2MASS J09444731-1812489, NLTT 22505, TIC 418096656
 M3.5Ve - 35.8 ly

Beta Leonis
Denebola, * bet Leo, Deneb Aleet, β Leonis, 94 Leo, BD+15°2383, FK5 444, GCTP 2738.00, GJ 448, Gliese 448, HD 102647, HIC 57632, HIP 57632, HR 4534, LFT 853, LHS 2462, LTT 13249, SAO 99809, 2MASS J11490366+1434197, TIC 14725877, TYC 870-988-1, USNO-B1.0 1045-00205720
 A3Va 1.8 M☉ 35.9 ly

HD 160346
GJ 688, Gliese 688, HIC 86400, HIP 86400, LTT 15233, NLTT 45197, 2MASS J17391691+0333190, TIC 349491678, TYC 419-1909-1, WISE J173916.79+033317.7, Gaia DR2 4377160604838377600
 K3-V - 35.9 ly

2MASS J1624+0029
SDSS J162414.36+002915.7, TIC 5791302, WISE J162414.09+002915.6, 2MASS J16241436+0029158
 T6V - 35.9 ly

Beta Virginis
Zavijava, Zavijah, Alaraph, Minelauva, β Vir, 5 Virginis, BD+02°2489, FK5 445, HD 102870, HIC 57757, HIP 57757, HR 4540, SAO 119076, LHS 2465, bet Vir, GJ 449, Gliese 449, LFT 854, LTT 13264, 2MASS J11504173+0145528, NLTT 28736, SAO 119076, SDSS J115041.71+014552.7, TIC 366661076, TYC 273-924-1, WISEA J115042.25+014550.1
 F9V 1.4 M☉ 35.9 ly

2MASS J12171110-0311131
SDSS J121711.19-031113.3, TIC 66628168, WISEP J121710.30-031113.2
 T7.5 - 35.9 ly

2MASS J1535+2225
2MASS J15354167+2225254, TIC 258044469, WISE J153541.67+222525.5
 - 35.9 ly

Gliese 438
CD-51 5974, LFT 839, LHS 2447, CF 9268, L 252-28, LTT 4348, NLTT 28348, 2MASS J11431977-5150255, GJ 438, PLX 2709, TIC 93716498, TYC 8227-1613-1
 M1 D 0.4 M☉ 35.9 ly

Ross 1003
Gaia DR2 772430527947893632, GJ 1148, Gliese 1148, LTT 13210, 2MASS J11414471+4245072, LHS 2443, G 122-40, HIP 57050, HIC 57050, LFT 836, LTT 13210, NLTT 28266, TIC 115869504, TYC 3016-1877-1, WISEA J114144.08+424506.2
 M4.0Ve 0.34 M☉ 36 ly

WISEA J2354+0240
WISEA J235402.79+024014.1
 Y1 - 36 ly
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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: Sterne

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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.
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Random terms
SternpositionLeuchtkraftSterntemperaturSternmasseSterngrößeSternenalter

Sternentwicklung

Stars are born and die in various ways depending on their mass, composition, and other factors. The most common life cycle for stars like our Sun involves several key stages.
Stellar evolution visualisation

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