NGC 248
| Emissionsnebel | |
|---|---|
| NGC 248 | |
 (c) ESA/Hubble, CC BY 4.0 | |
| Abbildung des Emissionsnebels NGC 248 aus Aufnahmen des Hubble-Weltraumteleskops | |
| AladinLite | |
| Sternbild | Tukan |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 00h 46m 19,6s [1] |
| Deklination | -73° 23′ 21″ [1] |
| Erscheinungsbild | |
| Winkelausdehnung | 1′,3 × 1′,0 [1] |
| Ionisierende Quelle | |
| Physikalische Daten | |
| Zugehörigkeit | Kleine Magellansche Wolke [2] |
| Geschichte | |
| Entdeckung | J. F. W. 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.
Der Nebel befindet sich in der Kleinen Magellanschen Wolke.
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NGC248 - HST - Heic1623a.tif
(c) ESA/Hubble, CC BY 4.0
This glowing nebula, named NGC 248, is located within the Small Magellanic Cloud, a satellite galaxy of the Milky Way and about 200 000 light-years from Earth. The nebula was observed with Hubble’s Advanced Camera for Surveys in September 2015, as part of a survey called the Small Magellanic cloud Investigation of Dust and Gas Evolution (SMIDGE).
(c) ESA/Hubble, CC BY 4.0
This glowing nebula, named NGC 248, is located within the Small Magellanic Cloud, a satellite galaxy of the Milky Way and about 200 000 light-years from Earth. The nebula was observed with Hubble’s Advanced Camera for Surveys in September 2015, as part of a survey called the Small Magellanic cloud Investigation of Dust and Gas Evolution (SMIDGE).
Coordinates Position (RA): 0 45 22.85 Position (Dec): -73° 22' 43.90" Field of view: 2.22 x 2.22 arcminutes Orientation: North is 3.1° right of vertical
Colours & filters Band Wavelength Telescope Optical g 475 nm Hubble Space Telescope ACS Optical V 550 nm Hubble Space Telescope ACS Optical H-Alpha 658 nm Hubble Space Telescope ACS Optical I 814 nm Hubble Space Telescope ACS.