Stars

The 25 brightest stars

  Star Name RA Dec App.
(abs.) 
vis.
mag.*
Distance (Ly) Spectral Type
     
(1980.0)

(1980.0)
     
    The Sun     -26.72
(4.85)
  G2V
1 Alpha CMa Sirius 06 44.2 -16 42 -1.46
(+1.4)
8.7 A1V
2 Alpha Car Canopus 06 23.5 -52 41 - -0.72
(-3.1)
98.0 F0Ib-II
3 Alpha Boo Arcturus 14 14.8 +19 17 -0.06
(-0.3)
36.0 K2IIIp
4 Alpha Cen Rigil Kent 14 38.4 -60 46 0.01
(+4.4)
4.2 G2V
5 Alpha Lyr Vega 18 36.2 +38 46 0.04
(+0.5)
26.5 A0V
6 Alpha Aur Capella 05 15.2 +45 59 0.05
(-0.6)
45.0 G8III?
7 Beta Ori Rigel 05 13.6 -08 13 0.14
(-7.1)
900.0 B8Ia
8 Alpha CMi Procyon 07 38.2 +05 17 0.37
(+2.6)
11.4 F5IV-V
9 Alpha Ori Betelgeuse 05 54.0 +07 24 0.41
(-5.6)
520.0 M2Iab
10 Alpha Eri Achenar 01 37.0 -57 20 0.51
(-2.3)
118.0 B3Vp
11 Beta Cen Hadar 14 02.4 -60 16 0.63
(-5.2)
490.0 B1III
12 Alpha Aql Altair 19 49.8 +08 49 0.76
(+2.2)
16.5 A7IV-V
13 Alpha Tau Aldebaran 04 34.8 +16 28 0.86
(-0.7)
68.0 K5III
14 Alpha Vir Spica 13 24.1 -11 03 0.91
(-3.3)
220.0 B1V
15 Alpha Sco Antares 16 28.2 -26 23 0.92
(-5.1)
520.0 M1Ib
16 Alpha PsA Fomalhaut 22 56.5 -29 44 1.15
(+2.0)
22.6 A3V
17 Beta Gem Pollux 07 44.1 +28 05 1.16
(+1.0)
35.0 K0III
18 Alpha Cyg Deneb 20 40.7 +45 12 1.26
(-7.1)
1600.0 A2Ia
19 Beta Cru   12 46.6 -59 35 1.28
(-4.6)
490.0 B0.5III
20 Alpha Leo Regulus 10 07.3 +12 04 1.36
(-0.7)
84.0 B7V
21 Alpha Cru Acrux 12 25.4 -62 59 1.39
(-3.9)
370.0 B0.5IV
22 Epsilon CMa Adhara 06 57.8 -28 57 1.48
(-5.1)
680.0 B2II
23 Lambda Sco Shaula 17 32.3 -37 05 1.60
(-3.3)
310.0 B1V
24 Gamma Ori Bellatrix 05 24.0 +06 20 1.64
(-4.2)
470.0 B2III
25 Beta Tau Elnath 05 25.0 +28 36 1.65
(-3.2)
300.0 B7III


*App. vis. mag. = Apparent visual magnitude
 Abs. vis. mag. = Absolute visual magnitude

Notes

Sirius is the brightest star in the sky. Sirius B is a white dwarf, as is Procyon B. They have about the same mass as the Sun but are only about one fiftieth of its diameter.

Apart from the Sun, Alpha Cen is the closest star in the sky. It has two components A and B which are close together and can only be seen separately in a small telescope. The third component, called Proxima, which is a faint star well separated from A and B is the closest of the three.

The spectral types indicate the temperature and luminosity of the star. The temperatures, from hottest to coolest run from classes O to M in the order O-B-A-F-G-K-M. In each class there are subclasses from 0 to 9. The luminosities are indicated by roman numerals with I being a supergiant, III a giant and V a dwarf.

The brightest known stars in our galaxy are very luminous red supergiants. They have spectral types M0-8 Ia+ and absolute magnitudes of -9 to -10 (about 4,000,000 times as bright as the Sun). They are believed to have masses about 30 times that of the Sun.

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