Lyssterke stjerner
Wikimedia-listeartikkel
Dette er ei liste over mest lyssterke stjerner på nattehimmelen som sett frå jorda.
T stor. (mV) |
Eigennamn | Bayernemning | Avstand (ly) | Spektralklasse |
---|---|---|---|---|
−26.74 | Sola | 0.000 016 | G2 V | |
−1.46 | Sirius | α CMa | 8.6 | A1 V, DA2 |
−0.74 | Canopus | α Car | 310 | F0 Ib |
−0.27 (0.01 + 1.33) | Rigil Kent, Toliman[1] | α Cen AB (α1,2 Cen) | 4.4 | G2 V, K1 V |
−0.05 | Arcturus | α Boo | 37 | K0 III |
0.03 (−0.02 - 0.07var) | Vega | α Lyr | 25 | A0 Va |
0.08 (0.03 - 0.16var) | Capella | α Aur | 42 | K0 III, G1 III |
0.13 (0.05 - 0.18var) | Rigel | β Ori | 860 | B8 Ia |
0.34 | Procyon | α CMi | 11 | F5 IV-V |
0.46 (0.40 - 0.46var) | Achernar | α Eri | 140 | B6 Vep |
0.50 (0.2 - 1.2var) | Betelgeuse | α Ori | [2] | 640M2 Iab |
0.61 | Agena, Hadar | β Cen | 350 | B1 III |
0.76 | Altair | α Aql | 17 | A7 V |
0.76 (1.33 + 1.73) | Acrux | α Cru | 320 | B0.5 IV, B1 V |
0.86 (0.75 - 0.95var) | Aldebaran | α Tau | 65 | K5 III |
0.96 (0.6 - 1.6var) | Antares | α Sco | 600 | M1.5 Iab, B3 V |
0.97 (0.97 - 1.04var) | Spica | α Vir | 260 | B1 III-IV, B2 V |
1.14 | Pollux | β Gem | 34 | K0 III |
1.16 | Fomalhaut | α PsA | 25 | A3 V |
1.25 (1.21 - 1.29var) | Deneb | α Cyg | 2,600 | A2 Ia |
1.25 (1.23 - 1.31var) | Mimosa, Becrux | β Cru | 350 | B0.5 II, B2 V |
1.39 | Regulus | α Leo | 77 | B7 V |
1.50 | Adara, Adhara | ε CMa | 430 | B2 Iab: |
1.62 | Shaula | λ Sco | 700 | B2 IV |
1.62 (1.98 + 2.97) | Castor | α Gem | 52 | Am, A1 V |
1.64 | Gacrux | γ Cru | 88 | M3.5 III |
1.64 | Bellatrix | γ Ori | 240 | B2 III |
1.65 | El Nath | β Tau | 130 | B7 III |
1.69 | Miaplacidus | β Car | 110 | A1 III |
1.69 (1.64 - 1.74var) | Alnilam | ε Ori | 2,000 | B0 Ia |
1.72 (1.81 - 1.87var + 4.27) | Suhail, Regor | γ1,2 Vel | 840 | WC8, O7.5e |
1.74 | Alnair | α Gru | 100 | B7 IV |
1.77 | Alioth | ε UMa | 81 | A1 III-IVp kB9 |
1.77 | Alnitak | ζ Ori A | 820 | O9.7 Ib, O9 III, B0 II-IV |
1.79 | Dubhe | α UMa | 120 | G9 III, A7.5 |
1.80 | Mirfak | α Per | 590 | F5 Ib |
1.82 | Wezen | δ CMa | 1,800 | F8 Ia |
1.84 | Sargas | θ Sco | 270 | F0 II |
1.85 | Kaus Australis | ε Sgr | 140 | B9.5 III |
1.86 | Avior | ε Car | 630 | K3 III, B2 Vp |
1.86 | Benetnasch, Alkaid | η UMa | 100 | B3 V |
1.90 (1.89 - 1.94var) | Menkalinan | β Aur | 100 | A1mIV+A1mIV |
1.91 | Atria | α TrA | 420 | K2 IIb-IIIa |
1.92 | Alhena | γ Gem | 100 | A1.5 IV+ |
1.94 | Påfuglen | α Pav | 180 | B2 IV |
1.96 (1.99 - 2.39var + 5.57) | - | δ Vel | 80 | A1 Va(n), F2-F5 |
1.98 | Mirzam | β CMa | 500 | B1 II-III |
2.00 | Alfard | α Hya | 180 | K3 II-III |
1.98 (1.86 - 2.13var) | Polaris | α UMi | 430 | F8 Ib |
2.00 | Hamal | α Ari | 66 | K1 IIIb |
2.08 (2.37 + 3.64) | Algieba | γ1 Leo | 130 | K0 III, G7 IIIb |
2.02 | Deneb Kaitos, Diphda | β Cet | 96 | K0 III |
2.05 | Nunki, Sadira | σ Sgr | 220 | B2.5 V |
2.06 | Menkent | θ Cen | 61 | K0 III |
2.05 (2.01 - 2.10var) | Mirach | β And | 200 | M0III |
2.06 | Alpheratz, Sirrah | α And | 97 | B8 IV |
2.07 | Rasalhague | α Oph | 47 | A5 V |
2.08 | Kochab | β UMi | 130 | K4 III |
2.09 | Saiph | κ Ori | 720 | B0 Iab: |
2.11 | Denebola | β Leo | 36 | A3 Va |
2.12 (2.1 - 3.39var) | Algol | β Per | 93 | B8 V |
2.15 (2.0 - 2.3var) | - | β Gru | 170 | M5 III |
2.17 | Muhlifain | γ Cen | 130 | A1IV, (A0III/A0III) |
2.21 | Aspidiske, Turais | ι Car | 690 | A9 Ib |
2.21 (2.14 - 2.30var) | Suhail | λ Vel | 570 | K4.5 Ib-II |
2.23 (2.21 - 2.32var) | Alphecca, Gemma | α CrB | 75 | A0 V, G5 V |
2.23 (2.23 - 2.35var) | Mintaka | δ Ori | 900 | B0 III, O9 V |
2.23 | Sadr | γ Cyg | 1,500 | F8 Ib |
2.23 | Eltanin | γ Dra | 150 | K5 III |
2.24 | Schedar | α Cas | 230 | K0 IIIa |
2.25 | Naos | ζ Pup | 1,100 | O4 If(n)p |
2.26 | Almach | γ And | 350 | K3 IIb, B9.5 V, B9.5 V, A0 V |
2.27 | Mizar | ζ1 UMa | 78 | A2 Vp, A2 Vp, A1m, A5 V |
2.28 (2.25 - 2.31var) | Caph | β Cas | 54 | F2 III |
2.29 | Izar | ε Boo | 202 | K0 II-III, A2 V |
2.30 (2.29 - 2.34var) | Men, Kakkab | α Lup | 550 | B1.5 III |
2.30 (2.29 - 2.31var) | - | ε Cen | 380 | B1III |
2.31 (1.6 - 2.32var) | Dschubba | δ Sco | 400 | B0.3 IV |
2.31 | Wei | ε Sco | 65 | K1 III |
2.35 (2.30 - 2.41var) | Marfikent | η Cen | 310 | B1.5Vne |
2.37 | Merak | β UMa | 79 | A1 IVps |
2.38 | Ankaa, Nair al Zaurak | α Phe | 77 | K0.5 IIIb |
2.39 | Girtab | κ Sco | 460 | B1.5 III |
2.40 (0.7 - 3.0var) | Enif | ε Peg | 670 | K2 Ib |
2.42 (2.31 - 2.74var) | Scheat | β Peg | 200 | M2.5 II-IIIe |
2.43 | Sabik | η Oph | 49 | A1 V, A3 V |
2.44 | Phecda | γ UMa | 84 | A0Ve |
2.45 | Aludra | η CMa | 2,000[3] | B5 Ia |
2.46 | Markeb | κ Vel | 540 | B2 IV |
2.47 (1.6 - 3.0var) | Tsih, Navi | γ Cas | 610 | B0.5 IVpe |
2.48 | Markab | α Peg | 140 | B9 III |
2.48 | Gienah | ε Cyg | 72 | K0 III-IV |
2.50 | Acrab | β Sco | 404 | B1V, B2V |
Kjelder
endre- Denne artikkelen bygger på «List of brightest stars» frå Wikipedia på engelsk, den 6. juli 2016.
- Wikipedia på engelsk oppgav desse kjeldene:
- ↑ Kunitzsch P., & Smart, T., A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations, Cambridge, Sky Pub. Corp., 2006, p. 27
- ↑ Graham M. Harper, Alexander Brown, and Edward F. Guinan, (April 2008). «A New VLA-Hipparcos Distance to Betelgeuse and its Implications» (PDF). The Astronomical Journal (IOP Publishing) 135 (4,): 1430–1440. Bibcode:2008AJ....135.1430H. doi:10.1088/0004-6256/135/4/1430. Henta 10. juli 2010.
- ↑ van Leeuwen, F. (November 2007). «Validation of the new Hipparcos reduction». Astronomy and Astrophysics 474 (2): 653–664. Bibcode:2007A&A...474..653V. arXiv:0708.1752. doi:10.1051/0004-6361:20078357.