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Epsilon Pegasi (Latinised from ε Pegasi, abbreviated Epsilon Peg, ε Peg), formally named Enif / ˈ iː n ɪ f /, 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.
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.
Messier 15 or M15 (also designated NGC 7078 and sometimes known as the Great Pegasus Cluster) is a globular cluster in the constellation Pegasus. It was discovered by Jean-Dominique Maraldi in 1746 and included in Charles Messier 's catalogue of comet -like objects in 1764.
Zeta Pegasi or ζ Pegasi, formally named Homam (/ ˈ h oʊ m æ m /), [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.
Located at a distance of 77 million light-years with a redshift of 0.00555, it is an active galaxy with a supermassive black hole at its core. Its characteristic emission lines are produced by gas moving at high speeds around the central black hole. [58] Pegasus is also noted for its more unusual galaxies and exotic objects.
51 Pegasi / Helvetios. 51 Pegasi (abbreviated 51 Peg), formally named Helvetios / hɛlˈviːʃiəs /, [12] is a Sun-like star located 50.6 light-years (15.5 parsecs) from Earth in the constellation of Pegasus. It was the first main-sequence star found to have an exoplanet (designated 51 Pegasi b, officially named Dimidium) orbiting it.