NGC 248
| Emission nebula | |
|---|---|
|  NGC 248 taken  as part of a survey called the Small Magellanic cloud Investigation of Dust and Gas Evolution (SMIDGE).[1] | |
| Observation data: J2000 epoch | |
| Right ascension | 00h 45m 24.1s[2] | 
| Declination | −73° 22′ 44.4″ | 
| Distance | 200,000 ly | 
| Constellation | Tucana | 
| Physical characteristics | |
| Radius | 30x10 ly | 
| Designations | LHA 115-N 13, DEM S 16[3] | 
NGC 248 is an emission nebula in the constellation Tucana. It is in the Small Magellanic Cloud.[3] It was discovered in 1834 by the astronomer John Frederick William Herschel. NGC 248 is about 60 light-years long and 20 light-years wide.
See also
References
- ^ "Festive nebulae light up Milky Way Galaxy satellite". www.spacetelescope.org. Retrieved 21 December 2016.
- ^ Frommert, Hartmut. "NGC 248". spider.seds.org. Retrieved 21 December 2016.
- ^ a b "NGC 248". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-24.
External links
 Media related to NGC 248 at Wikimedia Commons Media related to NGC 248 at Wikimedia Commons
 
