NGC 428 | |
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![]() Hubble image of NGC 428. | |
Observation data (J2000.0 epoch) | |
Constellation | Cetus [1] |
Right ascension | 01h 12m 55,709s [2] |
Declination | +00° 58′ 53.69″ [2] |
Distance | 48 mly [3] |
Apparent magnitude (B) | 12.1 [2] |
Characteristics | |
Type | SAB(s)m [4] |
Other designations | |
NGC 428 • UGC 763 • PGC 4367 • Z 385.28 • MCG + 00-04-36 • IRAS 01103 + 0043 • 2MASX J01125570 + 0058536 • GC 238 • H 2.622 • HIPASS J0112 + 00 [2] |
NGC 428 is a barred spiral galaxy in the constellation of Cetus (The Sea Monster), with its spiral structure distorted and warped, possibly the result of the collision of two galaxies. [3] There appears to be a substantial amount of star formation occurring within NGC 428 and it lacks well defined arms — a telltale sign of a galaxy merger. [3] In 2015 the Hubble Space Telescope made a close-up shot of the galaxy with its Advanced Camera for Surveys and its Wide Field and Planetary Camera 2. [1] The structure of NGC 428 has been compared to NGC 5645. [4]
NGC 428 was discovered by William Herschel in December 1786. [3] A type Ia supernova designated SN2013ct was discovered May 11, 2013, within the galaxy by Stuart Parker of the Backyard Observatory Supernova Search (BOSS) project in Australia and New Zealand. [3] [5]
Smoker et al. reported in 1996 on the NGC 428 field, with the HI tail and LSB dwarf 0110+008, assessing star formation properties based on molecule density distributions, and concluded that the tail formation most likely originated through tidal interactions between two galaxies. [6]