NGC 777

Galaxy in the constellation Triangulum From Wikipedia, the free encyclopedia

NGC 777 is an elliptical galaxy in the constellation of Triangulum. It was discovered by William Herschel on September 12, 1784. It has a weak active nucleus of type Seyfert 2 or LINER 2,[4] implying that the central region is obscured. When observed in radio waves the galaxy has a bright nucleus from which emerge small two radio jets about 18 kpc across. The jets are of Fanaroff–Riley class I.[5] It may be an outlying member of galaxy cluster Abell 262.[6]

Quick facts Observation data (J2000 epoch), Constellation ...
NGC 777
NGC 777
Observation data (J2000 epoch)
ConstellationTriangulum
Right ascension2h 00m 14.907s[1]
Declination31° 25 46[1]
Redshift0.016708[1]
Heliocentric radial velocity5,015 km/s[2]
Distance189 million ly (58.075 mpc)[2]
Apparent magnitude (V)12[3]
Characteristics
TypeE1[3]
Apparent size (V)2.5' x 2.0'[3]
Other designations
CGCG 503-67, MCG 5-5-38, PGC 7584, UGC 1476
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