NGC 248 explained

NGC 248
Type:emission
Epoch:J2000
Ra:[1]
Dist Ly:200,000
Constellation:Tucana
Radius Ly:30x10
Names:LHA 115-N 13, DEM S 16

NGC 248 is an emission nebula in the constellation Tucana. It is in the Small Magellanic Cloud.[2] 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

Notes and References

  1. Web site: Frommert. Hartmut. NGC 248. spider.seds.org. 21 December 2016.
  2. NGC 248. 2021-02-24.