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data. Epsilon Pegasi (Latinised from ε Pegasi, abbreviated Epsilon Peg, ε Peg), formally named Enif / ˈiːnɪf /, is the brightest star in the northern constellation of Pegasus. With an average apparent visual magnitude of 2.4, [3] this is a second-magnitude star that is readily visible to the naked eye. The distance to this star can be ...
Eta Pegasi or η Pegasi, formally named Matar / ˈ m eɪ t ɑːr /, [11] [12] is a binary star in the constellation of Pegasus. The apparent visual magnitude of this star is +2.95, [2] making it the fifth-brightest member of Pegasus. Based upon parallax measurements, the distance to this star is about 214 light-years (66 parsecs) from the Sun. [1]
Beta Pegasi is a semi-regular variable with a period of 43.3 days [5] and a brightness that varies from magnitude +2.31 to +2.74 (averaging 2.42). [3] It is losing mass at a rate at or below 10 −8 times the Sun's mass per year, which is creating an expanding shell of gas and dust with a radius of about 3,500 times the Sun's radius (16 ...
Gamma Pegasi is a star in the constellation of Pegasus, located at the southeast corner of the asterism known as the Great Square. It has the formal name Algenib / æ l ˈ dʒ iː n ɪ b /; [14] [15] the Bayer designation Gamma Pegasi is Latinized from γ Pegasi and abbreviated Gamma Peg or γ Peg.
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Zeta Pegasi. Zeta Pegasi or ζ Pegasi, formally named Homam (/ ˈhoʊmæm /), [11][12] is a single [13] star in the northern constellation of Pegasus. With an apparent visual magnitude of +3.4, [2] this star is bright enough to be seen with the naked eye and is one of the brighter members of Pegasus. Parallax measurements place it at a distance ...