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  2. Absolute magnitude - Wikipedia

    en.wikipedia.org/wiki/Absolute_magnitude

    For example, a star of absolute magnitude M V = 3.0 would be 100 times as luminous as a star of absolute magnitude M V = 8.0 as measured in the V filter band. The Sun has absolute magnitude M V = +4.83. [1] Highly luminous objects can have negative absolute magnitudes: for example, the Milky Way galaxy has an absolute B magnitude of about −20 ...

  3. V1500 Cygni - Wikipedia

    en.wikipedia.org/wiki/V1500_Cygni

    AAVSO light curve for Nova Cygni 1975. The dates given are Julian day numbers.. V1500 Cygni or Nova Cygni 1975 was a bright nova occurring in 1975 in the constellation Cygnus.It had the second highest intrinsic brightness of any nova of the 20th century, exceeded only by CP Puppis in 1942.

  4. Beta Aurigae - Wikipedia

    en.wikipedia.org/wiki/Beta_Aurigae

    Download QR code; Print/export Download as PDF; Printable version; In other projects Wikidata item; Appearance. ... Absolute magnitude (M V) 0.674 / 0.777 [3] Orbit [7]

  5. Apparent magnitude - Wikipedia

    en.wikipedia.org/wiki/Apparent_magnitude

    The absolute magnitude M, of a star or astronomical object is defined as the apparent magnitude it would have as seen from a distance of 10 parsecs (33 ly). The absolute magnitude of the Sun is 4.83 in the V band (visual), 4.68 in the Gaia satellite's G band (green) and 5.48 in the B band (blue).

  6. V1054 Ophiuchi - Wikipedia

    en.wikipedia.org/wiki/V1054_Ophiuchi

    The brightest and most massive of these five stars is V1054 Ophiuchi A. The close binary subsystem V1054 Ophiuchi B is more massive than V1054 Ophiuchi A, however, its total visual magnitude is 0.1 mag fainter than V1054 Ophiuchi A's visual magnitude. [3] The total apparent magnitude of the V1054 Ophiuchi A-Bab triple subsystem is 9.02. [3] [10]

  7. Albireo - Wikipedia

    en.wikipedia.org/wiki/Albireo

    Download QR code; Print/export ... Absolute magnitude (M V) −0.25 [6] Albireo B; Radial velocity (R v) ... (121.3 +0.9 −1 ...

  8. Vega - Wikipedia

    en.wikipedia.org/wiki/Vega

    In effect, the magnitude scale has been calibrated so that the magnitude of these stars is the same in the yellow, blue and ultraviolet parts of the electromagnetic spectrum. [49] Thus, Vega has a relatively flat electromagnetic spectrum in the visual region—wavelength range 350–850 nanometers , most of which can be seen with the human eye ...

  9. Phase curve (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Phase_curve_(astronomy)

    Because the orbit of Mars is considerably eccentric its brightness at opposition can range from magnitude3.0 to −1.4. [14] The minimum brightness is about magnitude +1.6 [14] when Mars is on the opposite site of the Sun from the Earth. Rotational variations can elevate or suppress the brightness of Mars by 5% and global dust storms can ...