NGC 1428 is a peculiar galaxy of an uncertain morphology; either an elliptical or lenticular galaxy located approximately 65 million light-years away from Earth. It was discovered by astronomer Julius Schmidt, at that time director of the National Observatory of Athens, on January 19, 1865. The discovery was made using a 6 ft refractor, and it was published ten years later. It is a member of the Fornax Cluster. 40 known globular clusters have been observed surrounding NGC 1428 along with 23 observed planetary nebulae.
Physical characteristics NGC 1428 is host to a nuclear star cluster with an estimated mass ranging from 1.4 × 107 to 2.2 × 107 M☉. It is thought that this nuclear star cluster which surrounded by a nuclear stellar disk formed from multiple instances of gas acrecction and subsequent episodes of star formation. The presence of counter-rotating population of stars suggests the occurrence of mergers that occurred in the opposite direction of the rotation of NGC 1428. The galaxy has a supermassive black hole with an estimated mass of 4.1 × 107 M☉.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1428 at Wikimedia Commons
NGC 1428 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


