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NGC 1491
Emission nebula
The nebula NGC 1491
Observation data: J2000 epoch
Subtype H II region
Right ascension04h 03m 15.9s [1]
Declination+51° 18′ 54″ [1]
Distance3.02 ± 0.6  kpc (9,800 ± 2,000  ly) [1]  ly
Constellation Perseus
DesignationsCed 25, LBN 704, LBN 706, Sharpless 2-206 [1]
See also: Lists of nebulae

NGC 1491, also known as LBN 794, SH2-206 or Fossil Footprint Nebula, is an emission type bright nebula located about 9,800 light years away from Earth in the constellation of Perseus. [1] The nebula gets its deep red coloration due to many massive stars (such as BD+50 866) embedded within NGC 1491 producing large amounts of ultraviolet radiation and ionizing the hydrogen gas that makes up the nebula. [2] [3]

Gallery

References

  1. ^ a b c d e "NGC 1491". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 February 2017.
  2. ^ "Emission Nebula NGC 1491". noirlab.edu. Retrieved 2023-11-26.
  3. ^ "NGC 1491". Stargazers Lounge. 2021-03-08. Retrieved 2023-11-26.

External links

  • Media related to NGC 1491 at Wikimedia Commons