Liste der größten Sterne
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Größenvergleich von größten bekannten Sternen mit der Sonne.
Stern | Sonnenradien | |
---|---|---|
VY Canis Majoris | 2100−1800[1] | |
WOH G64 | ~ 2000[2] | |
VV Cephei | 1900−1600 | |
Rho Cassiopeiae | 1680−670 | |
RW Cephei | 1610−1260 | |
V354 Cephei | 1520 | |
KW Sagittarii | 1460 | |
KY Cygni | 1420 | |
My Cephei (Herschels "Granatstern") | 1420 | |
Beteigeuze (Alpha Orionis) | 1000−950[3][4] | |
V509 Cassiopeiae | 910 | |
Antares (Alpha Scorpii) | 820[5] | |
V838 Monocerotis | 800 | |
V382 Carinae | 747 | |
S Pegasi | 580[6] | |
T Cephei | 540[7] | |
S Orionis | 530[8] | |
W Hydrae | 520[9] | |
119 Tauri | 510[10] | |
R Cassiopeiae | 500[11] | |
Wezen (Delta Canis Majoris) | 482 | |
Chi Cygni | 470[12] | |
Ras Algethi (Alpha Herculis) | 460 | |
Eta Carinae | 400 | |
Mira A (Omicron Ceti) | 400 | |
S Doradus | 390 | |
R Doradus | 370 | |
HR Carinae | 350 | |
R Leonis | 350[13] | |
Pistolenstern | 340 | |
Chi Cygni | 300 | |
Epsilon Aurigae B | 295 | |
Deneb (Alpha Cygni) | 220 | |
La Superba (Y Canum Venaticorum) | 215 | |
LBV 1806-20 | 200 | |
6 Cassiopeiae | 190 | |
Epsilon Carinae | 190 | |
Epsilon Aurigae A | 175 | |
Zeta Aurigae | 160[14] | |
Enif (Epsilon Pegasi) | 150 | |
Gacrux (Gamma Crucis) | 113 | |
Albireo A1 (Beta Cygni) | 109 | |
Epsilon Aurigae | 100 | |
Polarstern | 100 | |
Gamma Andromedae | 83 | |
Arneb (Alpha Leporis) | 77 | |
Canopus (Alpha Carinae) | 71 | |
Rigel (Beta Orionis) | 68 | |
R Coronae Borealis | 65 | |
Mintaka (Delta Orionis) | 60 | |
Alnitak (Zeta Orionis) | 60 | |
Mirfak (Alpha Persei) | 60 | |
Mekbuda (Zeta Geminorum) | 60 | |
Eta Aquilae | 60 | |
Eltanin (Gamma Draconis) | 50 | |
Aldebaran (Alpha Tauri) | 43[15] | |
Kochab (Beta Ursae Minoris) | 41 |
Quellennachweise
- ↑ http://arxiv.org/pdf/astro-ph/0610433
- ↑ http://jumk.de/astronomie/sterne-2/woh-g64.shtml
- ↑ http://www.astro.uiuc.edu/~kaler/sow/betelgeuse.html
- ↑ http://www.iop.org/EJ/abstract/1538-3881/135/4/1430/
- ↑ http://adsabs.harvard.edu/abs/1990A&A...230..355R
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10781
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9837
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2512
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=6127
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2526
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10947
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107
- ↑ http://arxiv.org/abs/astro-ph/0411133
- ↑ http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2180
- ↑ http://adsabs.harvard.edu/abs/2005astro.ph..2181R
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