IC 289

Nebula in the constellation Cassiopeia From Wikipedia, the free encyclopedia

IC 289 is a planetary nebula in the constellation Cassiopeia.[3] It was discovered by Lewis Swift in early September 1888. It lies close to the 10th magnitude star BD +60° 0631. N.J. Martin described IC 289 as "A nice, faint round planet like planetary nebula. The uniform oval disc shows some irregularity in brightness but is not obviously brighter at the edge."[citation needed]

Right ascension03h 10m 19.3017s[1]
Declination+61° 19 00.914[1]
Distance5,190 ± 500 ly (1,592 ± 153 pc)[2] ly
ConstellationCassiopeia
Quick facts Emission nebula, Observation data: J2000.0 epoch ...
IC 289
Emission nebula
Planetary nebula
As seen by Hubble
Observation data: J2000.0 epoch
Right ascension03h 10m 19.3017s[1]
Declination+61° 19 00.914[1]
Distance5,190 ± 500 ly (1,592 ± 153 pc)[2] ly
ConstellationCassiopeia
DesignationsIRAS 03062+6107, 2MASS J03101930+6119009, ARO 86, Hb 1, VV 9, RL 67, Lan 496, NSV 1056, GSC2 N313033135782[1]
See also: Lists of nebulae
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The central star of the planetary nebula is an O-type star with a spectral type of O(H).[4]

References

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