Jump to content

NGC 248

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Monkbot (talk | contribs) at 20:53, 12 January 2021 (Task 18 (cosmetic): eval 2 templates: hyphenate params (2×);). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

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 ascension00h 45m 24.1s[2]
Declination−73° 22′ 44.4″
Distance200,000 ly
ConstellationTucana
See also: Lists of nebulae

NGC 248 is an emission nebula in the Constellation Tucana. 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

  1. ^ "Festive nebulae light up Milky Way Galaxy satellite". www.spacetelescope.org. Retrieved 21 December 2016.
  2. ^ Frommert, Hartmut. "NGC 248". spider.seds.org. Retrieved 21 December 2016.
  • Media related to NGC 248 at Wikimedia Commons