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IC 1296

From Wikipedia, the free encyclopedia

IC 1296
IC 1296, as seen by Spitzer
Observation data
Right ascension18h 53m 18s
Declination+33° 03’ 59”
Surface brightness23.63 mag/arcsec^2
Other designations
IC 1296,

UGC 11374, PGC 62532, CGCG 201-040, MCG +06-41-022, 2MASX J18531883+3303596,

2MASS J18531884+3303599

IC 1296 is an extremely faint barred spiral galaxy of Hubble-type SBbc in the constellation Lyra in the northern sky. It is estimated to be 238 million light-years from the Milky Way and about 120,000 light-years in diameter.[1]

IC 1296 is only 4 arc minutes away from the well-known Ring Nebula in the night sky.[2] Planetary nebulae and galaxies are rarely observed together because planetary nebulae are galactic objects and are concentrated toward our galactic center, where extragalactic objects - such as distant galaxies - are rarely observed due to absorption by gas and dust.

The astronomical object was discovered on October 2, 1893, by Edward Emerson Barnard. In August 2013, supernova SN2013ev[3] was discovered in the southern spiral arm of IC 1296.[4]

The Ring Nebula. IC 1296 is visible as the faint galaxy to the right.

See also

External links

References

  1. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-06-06.
  2. ^ "Ring Nebula (Messier 57) | Deep⋆Sky Corner". www.deepskycorner.ch. Retrieved 2024-06-06.
  3. ^ "IC 1296", Wikipedia (in German), 2024-04-29, retrieved 2024-06-06
  4. ^ "Revised IC Data for IC 1296". spider.seds.org. Retrieved 2024-06-06.
This page was last edited on 6 June 2024, at 19:22
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