This article is about the brightness of stars as seen from Earth (apparent magnitude). For intrinsic luminosity of stars (absolute magnitude), seeList of most luminous stars.
Most stars on this list appear bright from Earth because they are nearby, not because they are intrinsicallyluminous. For a list which compensates for the distances, converting theapparent magnitude to theabsolute magnitude, see thelist of most luminous stars.
Some majorasterisms, which feature many of the brightest stars in thenight sky
TheSun is the brightest star as viewed fromEarth, at −26.78 mag. The second brightest isSirius at −1.46 mag. For comparison, the brightest non-stellar objects in theSolar System have maximum brightnesses of:
Any exact order of the visual brightness of stars is not perfectly defined for four reasons:
Stellar brightness is based on theapparent visual magnitude as perceived by the human eye, from the brightest stars of 1st magnitude to the faintest at 6th magnitude. Since the invention of the optical telescope and the documenting of binary stars and multiple star systems, stellar brightness could be expressed as eitherindividual (separate) ortotal (combined) magnitude. The table is ordered by combined magnitude of all naked eye components appearing as if they were single stars. Such multiple star systems are indicated by parentheses showing the individual magnitudes of component stars bright enough to make a detectable contribution. For example, thebinary star systemAlpha Centauri has the total or combined magnitude of −0.27, while its two component stars have magnitudes of +0.01 and +1.33.[3]
New or more accuratephotometry, standard filters, or adopting differing methods using standard stars can measure stellar magnitudes slightly differently. This may change the apparent order of lists of bright stars. The table shows measured V magnitudes, which use aspecific filter that closely approximates human vision. However, other kinds of magnitude systems do exist based on different wavelengths, some well away from the distribution of the visible wavelengths of light, and these apparent magnitudes vary dramatically in the different systems.[4] For example,Betelgeuse has the K-band (infrared) apparent magnitude of −4.05.[5]
Some stars, likeBetelgeuse andAntares, arevariable stars, changing their magnitude over days, months or years. In the table, the range of variation is indicated with the symbol "var". Single magnitude values quoted for variable stars come from a variety of sources. Magnitudes shown in the table are either when the stars are at maximum brightness, which is repeated for every cycle (e.g. the eclipsing binary Algol); or, if the variations are small, a simple average magnitude. For red variable stars, specifying a single maximum brightness is often difficult because each cycle produces a different maximum brightness; this is thought to be caused by poorly understood pulsations instellar evolution processes. Such quoted stellar brightness is sometimes based on theaverage maximum apparent magnitude[6] from estimated maxima over many observed light-curve cycles, sometimes spanning across centuries. Results often quoted in the literature are not necessarily straightforward and may differ in expressing an alternate value for a singular maximum brightness or as a range of values.
A few selected stars, thought to be uniformly fixed in brightness, are used asstandard stars.[which?] These standard stars have carefully determined magnitudes that have been analysed over many years, and are often used to determine other stars' magnitudes or their stellar parameters using comparatively consistent scales.[7]
The source of magnitudes cited in this list is the linked Wikipedia articles. This basic list is a catalog of what Wikipedia itself documents. References can be found in the individual articles.
^Zombeck, Martin V. (2007).Handbook of space astronomy and astrophysics (Third ed.). Cambridge, UK: Cambridge University Press. pp. 75,144–145.ISBN978-0-521-78242-5.
^Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
