by Diego Barucco

NGC 6720
M57
"Ring Nebula"

J2000
RA:18h 53m 35,65s
Dec: +33° 01' 40,2"
Mag. 9,70
Surface bright : 9,94
Dim.: 86" x 63"
Central star : 15,29
Constellation: Lyra

Discovery: Antoine Daquier gen. 1779
Distance: 0,87 kpc
Radius: 0,146 pc

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NGC 6720, also known as M 57, the "Ring Nebula", is surely the most known PN of the sky and the most representative object of this type. Finding and spotting this object in the summer sky is very easy, and its ease of view surely contributes to its fame. Its typical shape (it's like a smoke ring in the sky!) makes it one of the most photogenic object of its kind, with the famous bright ring.
Phisically, this PN is not so young anymore, and its central star is not so bright to ionize completely all the gases. Surprisingly, the Ring nebula is not so simple as it may seem: it's not only a bubble of gas. It's indeed a bipolar PN with lobes' axis directed toward us. So the ring structure is the equatorial toroid...a real ring in the space!

Interesting level : *

Essential bibliography
The Three-Dimensional Ionization Structure and Evolution of NGC 6720, The Ring Nebula - O'Dell, C. R.; Sabbadin, F.; Henney, W. J. - The Astronomical Journal, Volume 134, Issue 4, pp. 1679-1692 (2007)

Investigating the Haloes of Planetary Nebulae - Part Four - NGC6720 the Ring Nebula - Bryce, M.; Balick, B.; Meaburn, J. - R.A.S. MONTHLY NOTICES V.266, NO. 3/FEB1, P. 721, (1994)


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English traslation: Renzo Ruisi

Update: Giovedì, Dicembre 13, 2007 2:54 PM

 

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