| NGC 1528 | |
|---|---|
NGC 1528 (open cluster on the left) and nearby SH2-209 (nebula on the right) | |
| Observation data (J2000 epoch) | |
| Right ascension | 04h 15m 30.72s |
| Declination | +51° 13′ 04.8″ |
| Distance | 3,110 ± 500 ly (954 ± 154 pc) |
| Apparent magnitude (V) | 6.4 |
| Apparent dimensions (V) | 18′ |
| Physical characteristics | |
| Estimated age | 110 Ma |
| Other designations | NGC 1528, Cr 47 |
| Associations | |
| Constellation | Perseus |
NGC 1528 is an open cluster of stars in the northern constellation of Perseus. It was discovered by the German-British astronomer William Herschel in 1790. This cluster is located in the north-eastern part of the constellation, just under 3 degrees north of μ Persei. Less than 1.5° to the southeast is the open cluster NGC 1545 (m = 6.2). The NGC 1528 is clearly visible with 10x50 binoculars. 165 stars are recognised as members of NGC 1528, the brightest of which has apparent magnitude 8.7.