by Diego Barucco

IC 289

J2000
RA: 03h 10m 19,2s
Dec: +61° 19' 01"
Mag. 9,20
Surface bright: 10,87
Dim.: 42" x 28 "
Central star: 15,90
Constellation: Cassiopea

Discovery: Lewis Swift 2 set. 1888, identified as PN by Edwin Hubble in 1921
Distance: 1,434 kpc
Radius: 0,128 pc

View images
View observations
View professional images

IC 289 is a faint nebula in Cassiopea constellation and it hasn't been object of consideration by astronomers for years. Average telescopes show it as a faint ellipse with a clearly visible anular structure. Large telescopes can help the observer to show variation of brightness on the ring, best shown in photos. Old studies reveal that IC 289 has a bipolar toroid structure, where its toroid is exactly its main ring. Fainter lobes are shown, not so far from the ring, on the minor ellipse axis direction. That could be an evidence that its polar axis is tilted from our visual direction. Recent color images show central regions partially red. That's because of an important Halpha emission, probably associated with a shell or a strip that wraps the central structure, the same as it happens in NGC 7662 and NGC 7008.

Interesting level: ****

Bibliography
Narrow-band imagery of three planetary nebulae - A2, IC 289 and M 1-75 - Hua, C. T. - Astronomy and Astrophysics (ISSN 0004-6361), vol. 193, no. 1-2, March 1988, p. 273-280


English traslation: Renzo Ruisi

Update: Martedì, Dicembre 18, 2007 8:43 PM

 

Google