NGC 2030
| Emissionsnebel | ||
|---|---|---|
| NGC 2030 | ||
 | ||
| NGC 2030 mit dem Supernovaüberrest SNR B0535-66.0 | ||
  | ||
| AladinLite | ||
| Sternbild | Schwertfisch | |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | ||
| Rektaszension | 05h 34m 59,7s [1] | |
| Deklination | −67° 33′ 23″ [1] | |
| Erscheinungsbild | ||
| Ionisierende Quelle | ||
| Physikalische Daten
| ||
| Zugehörigkeit | Große Magellansche Wolke | |
| Geschichte | ||
| Entdeckung | John Herschel | |
| Datum der Entdeckung | 23. Dezember 1834 | |
| Katalogbezeichnungen | ||
| NGC 2030 • GC 1233 • h 2910 • ESO 56-EN156 | ||
NGC 2030 ist ein Emissionsnebel in der Großen Magellanschen Wolke im Sternbild Dorado. Das Objekt wurde am 23. Dezember 1834 von dem britischen Astronomen John Herschel entdeckt.[2]
Einzelnachweise
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