With regard to mass, size, and intrinsic brightness, the Sun is a typical star. Its approximate mass is 2 × 1030 kg (about 330,000 Earth masses), its approximate radius 700,000 km (430,000 miles), and its approximate luminosity 4 × 1033 ergs per second (or equivalently 4 × 1023 kilowatts of power). Other stars often have their respective quantities measured in terms of those of the Sun.
The table lists data pertaining to the 20 brightest stars, or, more precisely, stellar systems, since some of them are double (binary stars) or even triple stars. Successive columns give the name of the star, its brightness expressed in units called visual magnitudes and the spectral type or types (see below Classification of spectral types) to which the star or its components belong, the distance in light-years (a light-year being the distance that light waves travel in one Earth year: 9.46 trillion km, or 5.88 trillion miles), and the visual luminosity in terms of that of the Sun. All the primary stars (designated as the A component in the table) are intrinsically as bright as or brighter than the Sun; some of the companion stars are fainter.
| The 20 brightest stars | |||||||
| name | visual magnitude1 and spectral type | distance in light-years2 | visual luminosity relative to the Sun | ||||
| A3 | B3 | A3 | B3 | ||||
| Sirius | –1.44 | A1 V | 8.44 | DA 2 | 8.6 | 20.2 | 0.00226 |
| Canopus | –0.73 | F0 Ib | 312 | 1,390 | |||
| Arcturus | –0.05 | K1.5 III | 36.7 | 102.5 | |||
| Alpha Centauri | 0.00 | G2 V | 1.35 | K1 V | 4.4 | 1.41 | 0.405 |
| Vega | 0.03 | A0 V | 25.3 | 45.2 | |||
| Capella | 0.084 | G6 III | 1.1 | G2 III | 42.2 | 120 | 46.9 |
| Rigel | 0.18 | B8 Ia | 7.6 | B5 | 773 | 36,800 | 39.6 |
| Procyon | 0.40 | F5 IV-V | 10.70 | DZ | 11.4 | 6.54 | 0.00072 |
| Achernar | 0.45 | B3 Vp | 144 | 993 | |||
| Betelgeuse | 0.45 (var.) | M2 lab | 427 | 8,770 | |||
| Beta Centauri | 0.58 | B1 III | 3.8 | B2 (uncertain) | 526 | 1180 | 607 |
| Altair | 0.76 | A7 V | 16.8 | 10.1 | |||
| Aldebaran | 0.87 | K5 III | 13 | M2 V | 65.1 | 138 | 0.00194 |
| Spica | 0.98 | B1 V | 3.1 | B3 V | 262 | 2,020 | 287 |
| Antares | 1.06 (var.) | M1.5 lab | 5.37 | B2.5 V | 604 | 9,980 | 188 |
| Pollux | 1.16 | K0 III | 96.7 | 234 | |||
| Fomalhaut | 1.17 | A3 V | 6.49 | K4 V | 25.1 | 15.5 | 0.116 |
| Beta Crucis | 1.25 | B0.5 III | 352 | 2,860 | |||
| Deneb | 1.25 | A2 Ia | 3,230 | 240,000 | |||
| Alpha Crucis | 1.40 | B0.5 IV | 2.09 | B3 V | 321 | 2,250 | 1,108 |
| 1Negative magnitudes are brightest, and one magnitude difference corresponds to a difference in brightness of 2.5 times; e.g., a star of magnitude –1 is 10 times brighter than one of magnitude 1.5. 2One light-year equals about 9.46 trillion km. 3A and B are brighter and fainter components, respectively, of star. A multiple system is ranked by the brightness of its A component. 4Combined magnitudes of A and B. |
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Many stars vary in the amount of light they radiate. Stars such as Altair, Alpha Centauri A and B, and Procyon A are called dwarf stars; their dimensions are roughly comparable to those of the Sun. Sirius A and Vega, though much brighter, also are dwarf stars; their higher temperatures yield a larger rate of emission per unit area. Aldebaran A, Arcturus, and Capella A are examples of giant stars, whose dimensions are much larger than those of the Sun. Observations with an interferometer (an instrument that measures the angle subtended by the diameter of a star at the observer’s position), combined with parallax measurements (which yield a star’s distance; see below Determining stellar distances), give sizes of 12 and 22 solar radii for Arcturus and Aldebaran A. Betelgeuse and Antares A are examples of supergiant stars. The latter has a radius some 300 times that of the Sun, whereas the variable star Betelgeuse oscillates between roughly 300 and 600 solar radii. Several of the stellar class of white dwarf stars, which have low luminosities and high densities, also are listed in the table. Sirius B is a prime example, having a radius one-thousandth that of the Sun, which is comparable to the size of Earth. Among other notable stars in the table, Rigel A is a young supergiant in the constellation Orion, and Canopus is a bright beacon in the Southern Hemisphere often used for spacecraft navigation.
Embryonic-stars-in-the-Eagle-Nebula-This-detail-of-aEmbryonic stars in the Eagle Nebula (M16, NCG 6611)[Credits : Photo AURA/STScI/NASA/JPL (NASA photo # STScI-PRC95-44b)]
Light-curve-of-Algol-an-eclipsing-variable-or-eclipsing-binaryLight curve of Algol (Beta Persei), an eclipsing variable, or eclipsing binary, star system. The …[Credits : Encyclopædia Britannica, Inc.]
Schematic-spectrum-luminosity-correlation-of-spiral-arm-stars-in-theSchematic spectrum–luminosity correlation (Hertzsprung–Russell diagram) of spiral-arm …[Credits : From Astrophysical Journal, reproduced by permission of the American Astronomical Society]
Colour-magnitude-diagram-for-an-old-globular-cluster-made-upColour-magnitude (Hertzsprung-Russell) diagram for an old globular cluster made up of Population II …[Credits : From Astrophysical Journal, reproduced by permission of the American Astronomical Society]
Eta-CarinaeEta Carinae.[Credits : Photo AURA/STScI/NASA/JPL (NASA photo # STScI-PRC96-23a)]
N81-and-new-stars-observed-by-the-Hubble-Space-TelescopeN81 and new stars, observed by the Hubble Space Telescope.[Credits : Photo AURA/STScI/NASA/JPL (NASA photo # STScI-PR98-25)]
Centre-of-the-Orion-Nebula-Astronomers-have-identified-some-700Centre of the Orion Nebula (M42).[Credits : Photo AURA/STScI/NASA/JPL (NASA photo # STScI-PRC95-45a)]
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