NGC 1496
| Offener Sternhaufen NGC 1496 | |
|---|---|
| Der offene Sternhaufen NGC 1496 (SDSS) | |
| AladinLite | |
| Sternbild | Perseus |
| Position Äquinoktium: J2000.0 | |
| Rektaszension | 04h 04m 31,9s [1] |
| Deklination | +52° 39′ 41″ [1] |
| Erscheinungsbild | |
| Klassifikation | II 1 p [2] |
| Helligkeit (visuell) | 9,6 mag [3] |
| Rötung (Farbexzess E(B-V)) | 1,422 [1] |
| Physikalische Daten | |
| Zugehörigkeit | Milchstraße |
| Entfernung [4] | 4.012 Lj (1.230 pc) |
| Geschichte | |
| Entdeckt von | John Herschel |
| Entdeckungszeit | 8. November 1831 |
| Katalogbezeichnungen | |
| NGC 1496 • C 0400+524 • OCl 396 • Cr 44 • Lund 122 • GC 798 • h 310 • | |
NGC 1496 ist ein offener Sternhaufen im Sternbild Perseus und hat eine Winkelausdehnung von 3,0' und eine scheinbare Helligkeit von +9,6 mag. Er wurde am 8. November 1831 von dem britischen Astronomen John Frederick William Herschel entdeckt.[5]
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