NGC 248

Emissionsnebel
NGC 248
JWST-NIR-Aufnahme
JWST-NIR-Aufnahme
NGC 248
AladinLite
Sternbild Tukan
Position
ÄquinoktiumJ2000.0, Epoche: J2000.0
Rektaszension 00h 46m 19,6s [1]
Deklination −73° 23′ 21″ [1]
Erscheinungsbild
Scheinbare Helligkeit (visuell) mag
Scheinbare Helligkeit (B-Band) mag
Winkelausdehnung 1′,3 × 1′,0[1]
Ionisierende Quelle
Bezeichnung
Typ
Physikalische Daten

Zugehörigkeit Kleine Magellansche Wolke[2]
Entfernung 200.000 Lj
Geschichte
Entdeckung John Herschel
Datum der Entdeckung 11. April 1834
Katalogbezeichnungen
 NGC 248 • GC 133 • h 2344 • ESO 29-EN8

NGC 248 ist ein Emissionsnebel im Sternbild Tukan. Er wurde am 11. April 1834 von dem britischen Astronomen John Frederick William Herschel entdeckt.[3]

Der Nebel befindet sich in der Kleinen Magellanschen Wolke.

Quellen

  1. a b SIMBAD-Datenbank
  2. NASA/IPAC Extragalactic Database
  3. Seligman

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