IC 360
| Emissionsnebel | |
|---|---|
| IC 360 | |
  | |
| AladinLite | |
| Sternbild | Stier |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 04h 09m 02,5s [1] |
| Deklination | +26° 07′ 52″ [1] |
| Erscheinungsbild | |
| Winkelausdehnung | 180' × 100'[2] |
| Ionisierende Quelle | |
| Physikalische Daten | |
| Geschichte | |
| Entdeckung | Edward Barnard |
| Datum der Entdeckung | 6. Dezember 1893 |
| Katalogbezeichnungen | |
| IC 360 • | |
IC 360 ist ein Emissionsnebel im Sternbild Taurus auf der Ekliptik. Das Objekt ist ein Teil des äußeren Plejadennebels und wurde im Jahre 1893 vom US-amerikanischen Astronomen Edward Barnard entdeckt.[3]
Einzelnachweise
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