Liste der nächste sterne | Sternenkatalog

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.

	Mass	Distance
Delta Capricorni Aa Deneb Algedi, Deneb Algiedi, Scheddi, δ Cap, Del Cap, 49 Capricorni, BD−16 5943, FK5 819, GJ 837, HD 207098, HIP 107556, HR 8322, SAO 164644, ADS 15314, WDS 21470-1608	A7m III	2 M☉	38 ly
L 308-57 2MASS J06210665-4905379, DENIS J062106.6-490537, TIC 238950307, Gaia DR2 5550620058937466880		-	38 ly
G 41-8 JNN 274, NLTT 20558, 2MASS J08561956+1239500, TIC 437041669, WDS J08563+1239AB, WISE J085619.51+123947.3	M6V C	-	38 ly
LSPM J0602+3910 2MASS J06023045+3910592, TIC 174821904, WISEA J060230.60+391053.3, LSR J0602+3910	L1V	-	38 ly
Gliese 2106 LTT 5557, NLTT 36550, GJ 2106, CD-56 5362, HIC 69454, HIP 69454, 2MASS J14131288-5644314, TIC 407559875, TYC 8673-4534-1, WISEA J141313.30-564429.5	M2V: D	0.5 M☉	38 ly
LSR J2000+3057 2MASS J20000565+3057300, TIC 103245015, WISEA J200006.00+305745.6	M6Ve	-	38.1 ly
L 43-72 NLTT 45898, DENIS J181115.3-785922, 2MASS J18111528-7859227, TIC 276834958, WISEA J181115.56-785919.9	M4.5 D	-	38.1 ly
SSSPM J0829-1309 2MASS J08283419-1309198, DENIS J082834.3-130919, TIC 926898, V* V484 Hya, WISEA J082833.75-130919.5, EQ J0829-1309	L2	-	38.1 ly
Zeta Doradus GJ 189, Gliese 189, * zet Dor, CPD−57° 735, FK5 189, HD 33262, HIP 23693, HIC 23693, HR 1674, SAO 233822, GC 6258, 2MASS J05053067-5728217, TIC 381949122, TYC 8514-2291-1, WDS J05055-5728A	F9VFe-0.5	1.1 M☉	38.1 ly
L 623-94 LHS 3064, DENIS J152212.8-274944, Gliese 2112, GJ 2112, 2MASS J15221293-2749436, NLTT 40004, WISEA J152213.31-274936.3	M3: E	-	38.2 ly
CD-35 2213 NLTT 14841, TSN 1, C* 315, CGCS 908, EUVE J0517-35.3, L 449-1, 2MASS J05172292-3521545, RBS 636, RE J0517-352, TIC 77957301, WDS J05174-3522AB, WISEA J051722.71-352156.4	M4Ve	-	38.2 ly
2MASSW J1506544+132106	L3	-	38.2 ly
Gliese 572 GJ 572, BD+45 2247, G 179-6, G 201-30, HDS 2118A, HIC 73470, HIP 73470, LTT 14455, 2MASS J15005557+4525343, MCC 314, NLTT 39083, TIC 284266904, TYC 3481-1481-1, WISEA J150055.79+452537.7, RX J1500.9+4525 1	M0V	-	38.2 ly
Ross 271 LHS 6399, G 126-61, G 127-6, GJ 851, Gliese 851, HIC 109555, HIP 109555, LFT 1691, LTT 16492, NLTT 53159, 2MASS J22113008+1825341, MCC 74, TIC 258822427, TYC 1685-1853-1, WISEA J221130.34+182536.2	M2V	0.5 M☉	38.2 ly
G 112-21 LHS 1920, Gliese 1097, GJ 1097, HIC 36338, HIP 36338, 2MASS J07284541-0317524, NLTT 17919, TIC 64910894, TYC 4821-2979-1, USNO 130	M3V	-	38.3 ly
WISEA J120604.25+840110.5 WISE J120604.38+840110.6	Y0 C	0.01 M☉	38.3 ly
L 127-97 LHS 160, Gliese 118, GJ 118, HIC 13389, HIP 13389, LFT 237, LTT 1379, NLTT 9248, 2MASS J02522213-6340475, TIC 220526731, TYC 8862-1495-1, WISEA J025223.72-634040.6	M2.5	0.4 M☉	38.3 ly
CD-28 302	M3V	-	38.4 ly
Gaia EDR3 6887029163498137856		-	38.4 ly
BD-05 1737	M2	-	38.5 ly

Sternname

Mass

Distance

Delta Capricorni Aa

Deneb Algedi, Deneb Algiedi, Scheddi, δ Cap, Del Cap, 49 Capricorni, BD−16 5943, FK5 819, GJ 837, HD 207098, HIP 107556, HR 8322, SAO 164644, ADS 15314, WDS 21470-1608

A7m III

2 M☉

38 ly

L 308-57

2MASS J06210665-4905379, DENIS J062106.6-490537, TIC 238950307, Gaia DR2 5550620058937466880

38 ly

G 41-8

JNN 274, NLTT 20558, 2MASS J08561956+1239500, TIC 437041669, WDS J08563+1239AB, WISE J085619.51+123947.3

M6V C

38 ly

LSPM J0602+3910

2MASS J06023045+3910592, TIC 174821904, WISEA J060230.60+391053.3, LSR J0602+3910

L1V

38 ly

Gliese 2106

LTT 5557, NLTT 36550, GJ 2106, CD-56 5362, HIC 69454, HIP 69454, 2MASS J14131288-5644314, TIC 407559875, TYC 8673-4534-1, WISEA J141313.30-564429.5

M2V: D

0.5 M☉

38 ly

LSR J2000+3057

2MASS J20000565+3057300, TIC 103245015, WISEA J200006.00+305745.6

M6Ve

38.1 ly

L 43-72

NLTT 45898, DENIS J181115.3-785922, 2MASS J18111528-7859227, TIC 276834958, WISEA J181115.56-785919.9

M4.5 D

38.1 ly

SSSPM J0829-1309

2MASS J08283419-1309198, DENIS J082834.3-130919, TIC 926898, V* V484 Hya, WISEA J082833.75-130919.5, EQ J0829-1309

38.1 ly

Zeta Doradus

GJ 189, Gliese 189, * zet Dor, CPD−57° 735, FK5 189, HD 33262, HIP 23693, HIC 23693, HR 1674, SAO 233822, GC 6258, 2MASS J05053067-5728217, TIC 381949122, TYC 8514-2291-1, WDS J05055-5728A

F9VFe-0.5

1.1 M☉

38.1 ly

L 623-94

LHS 3064, DENIS J152212.8-274944, Gliese 2112, GJ 2112, 2MASS J15221293-2749436, NLTT 40004, WISEA J152213.31-274936.3

M3: E

38.2 ly

CD-35 2213

NLTT 14841, TSN 1, C* 315, CGCS 908, EUVE J0517-35.3, L 449-1, 2MASS J05172292-3521545, RBS 636, RE J0517-352, TIC 77957301, WDS J05174-3522AB, WISEA J051722.71-352156.4

M4Ve

38.2 ly

2MASSW J1506544+132106

38.2 ly

Gliese 572

GJ 572, BD+45 2247, G 179-6, G 201-30, HDS 2118A, HIC 73470, HIP 73470, LTT 14455, 2MASS J15005557+4525343, MCC 314, NLTT 39083, TIC 284266904, TYC 3481-1481-1, WISEA J150055.79+452537.7, RX J1500.9+4525 1

M0V

38.2 ly

Ross 271

LHS 6399, G 126-61, G 127-6, GJ 851, Gliese 851, HIC 109555, HIP 109555, LFT 1691, LTT 16492, NLTT 53159, 2MASS J22113008+1825341, MCC 74, TIC 258822427, TYC 1685-1853-1, WISEA J221130.34+182536.2

M2V

0.5 M☉

38.2 ly

G 112-21

LHS 1920, Gliese 1097, GJ 1097, HIC 36338, HIP 36338, 2MASS J07284541-0317524, NLTT 17919, TIC 64910894, TYC 4821-2979-1, USNO 130

M3V

38.3 ly

WISEA J120604.25+840110.5

WISE J120604.38+840110.6

Y0 C

0.01 M☉

38.3 ly

L 127-97

LHS 160, Gliese 118, GJ 118, HIC 13389, HIP 13389, LFT 237, LTT 1379, NLTT 9248, 2MASS J02522213-6340475, TIC 220526731, TYC 8862-1495-1, WISEA J025223.72-634040.6

M2.5

0.4 M☉

38.3 ly

CD-28 302

M3V

38.4 ly

Gaia EDR3 6887029163498137856

38.4 ly

BD-05 1737

38.5 ly

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

Liste der sterne

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

Sternentwicklung