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Ambiguous sentence
From the article:
- The image reveals two 'caps' of less ionised material at the edge of the nebula
Should it be read as that the material in these regions are less ionised compared to other regions; or that the concentration of ionised particles is lower, or something else?
If it is singly ionized nitrogen; does it have to be mentioned at all? In such case it is already mentioned in the text that green represents singly ionized nitrogen. Gunnar Larsson 19:03, 14 September 2006 (UTC)
Images
Why have they suddenly all disappeared? Several beautiful NASA public domain images have been deleted for no apparent reason.
- The question has been here for a month, and no explanation offered.... were they just deleted for fun, then? 81.179.65.38 00:22, 23 December 2006 (UTC)
- You don't want to have too many images--that's what Wikimedia Commons is for. I will add one more, though. It certainly is a beautiful thing.--MrFish 18:55, 7 May 2009 (UTC)
Age
Could someone please explain the discrepancy between the distance of 3300lj and the stated upper limit of the age for NGC6543 of only 1000 years? We would not be able to see this nebula if those values were correct. —Preceding unsigned comment added by 80.187.102.108 (talk) 12:22, 8 May 2011 (UTC)
This Article is an Utter Shambles
I've read this article three times now, and have found more than fifty mistakes here. Most of the facts are either mixed-up, incorrect or just plainly misconstrued. Note: Anyone reading the Wiki article on Planetary Nebula could fix these errors!!
Even many of the cited references don't actually say what is written here. Worst, most of the references are either out of date, or are not primary sources. I.e. SIMBAD quotes Stanghellini, L.; Shaw, R.A., Villaver, E., “The Magellanic cloud calibration of the Galactic planetary nebula distance scale.”, AJ., 689, 194 (2008), saying this distance is 1623 parsecs (1.62 kpc.)being 5323 light-years, rounded to 5300 light years NOT 3000!!
Paragraph 3
1) "The intricacy of the structure may be caused in part by material ejected from a binary central star, but as yet, there is no direct evidence that the central star has a companion."
What? Theory says that the shapes could be caused a binary star, but the majority planetaries we observe have not detected a binary star. Much of the problems are due to the distances to planetary nebulae!
2) "Also, measurements of chemical abundances reveal a large discrepancy between measurements done by two different methods, the cause of which is uncertain."
Again this is mostly due to distance, especially mostly as chemical abundance comes from spectra. Worst, What two methods? Is this any less more problematic to NGC 6543 compared to other planetary nebulae?
3) "Hubble Telescope observations revealed a number of faint rings around the Eye, which are spherical shells ejected by the central star in the distant past. The exact mechanism of those ejections, however, is unclear."
This applies to the majority of planetary nebulae, not just NGC 6543! The shells are not caused by ejections but by variable mass loss rates in the so-called superwinds, they are likely formed by snowplough theory, where the wind encounters the slower material forming them into multiple shells.
Paragraph 3 should be deleted, unless it can be proven to apply to NGC 6543. Else it should be in the Planetary Nebula page.
Under "General information" this article refers to Moore (2007) three times. I.e. Moore,S.L.(2007),"Observing the Cat’s Eye Nebula", Journal of the British Astronomical Association 117 (5): 279–280, Bibcode:2007JBAA..117R.279M
Yet the reference article does not mention 'surface brightness' nor anything about the "high declination" as stated!
Amazingly much of this article and the problems here stems from User:Worldtraveller between 2nd January 2005 to 5th September 2006 (He has not posted since 3rd March 2007. His User talk:Worldtraveller says retired.
Solution. Unless there is strong objection, much if this article needs revision and need to be written clearly to distinguish between facts relating to directly to NGC 6543 and planetary nebulae in general. I.e. The article is about NGC 6543 NOT planetary nebulae as a subject. Arianewiki1 (talk) 21:10, 31 October 2014 (UTC)
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