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Wikipedia:Featured article candidates/61 Cygni/archive1

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61 Cygni

61 Cygni (edit | talk | history | links | watch | logs)

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Nominator(s): -The Herald the joy of the LORDmy strength 14:53, 18 March 2015 (UTC)[reply]

This article is about a visual binary system in the constellation Cygnus. The article seems to meet all the criteria for a FA and I have made still more updation and minor fixes so as to meet the criteria. The article is currently a GA and the article have undergone major expansion after that. Top editors aren't active now and RJHall retired a little while ago. Still, I have done much to make it meet to the criteria. -The Herald the joy of the LORDmy strength 14:53, 18 March 2015 (UTC)[reply]

Review – The article is in decent shape, although perhaps a little short. Here are a few observations:

  • The 'absolute magnitude' values in the infobox need a proper citation; just computing them isn't enough. (Kervella et al. (2008) give the absolute bolometric magnitudes for the two stars; it might be better to use that field instead.)
  • The article needs to explain the meaning of the name '61 Cygni'. For example, where did it originate?
  • The meaning of 'K5 V' and 'K7 V' needs to be clarified, as the reader might not be familiar with the MK notation and its connection to the statement "K class (orange) main sequence stars".
  • The Observation history section should use consistent units for the parallax and be consistent about labeling parallax measurements.
  • The final two sentences of the Observation history section needs a citation.
  • The term 'old-disk stars' needs to be explained.
Done now..-The Herald the joy of the LORDmy strength 04:27, 21 March 2015 (UTC)[reply]
  • Perhaps you could use this reference to note whether an infrared excess has (or has not) been found.
  • You could also use Table 7 in this reference to speak to the stellar habitable zones around the two stars.
Still couldn't get it. Please link it to the page itself...-The Herald the joy of the LORDmy strength 15:03, 20 March 2015 (UTC)[reply]
It is part of a PDF document. Have you tried reading the arXiv article and scrolling down to near the end? Praemonitus (talk) 21:22, 20 March 2015 (UTC)[reply]
I read it but it seems to me like there aren't any IR excess as they say much about GJ 581, GJ 667C, and GJ 876 M-dwarfs. GJ 820 has its name only in the table. So should I include in the article that there aren't any IR excess? Plus, I couldn't deduce from them that there are any habitable zones either. -The Herald the joy of the LORDmy strength 04:27, 21 March 2015 (UTC)[reply]
Yes, the absence of a detectable IR excess is still of interest because it tells the reader something about the state of the system. The reference for the habitability radii is in a separate bullet above. Praemonitus (talk)
I think the same is explained in Refining planetary boundaries section. Right? -The Herald the joy of the LORDmy strength 07:51, 23 March 2015 (UTC)[reply]

Thanks. Praemonitus (talk) 16:20, 18 March 2015 (UTC)[reply]

ST11
  • The entire "Distance" section is a huge eyesore and frankly unimportant. Readers aren't going to care about every single distance estimate published, and are only going to care about the most accurate one, which is already present in the infobox. I'd remove the whole section.
  • If I'm understanding you correctly, you're saying that the table helps show how the parallax method works. There's two things wrong with that: I don't see how the table conveys that at all, and such info would not be appropriate for this article but rather for the parallax article. The approximations of pi is different, since the increasing approximations of pi has been a subject of intense study itself, and well, pi is much more important to everyday life than this single star. StringTheory11 (t • c) 15:21, 19 March 2015 (UTC)[reply]
But is the removal of the section necessary to result in further shortening of the article? -The Herald the joy of the LORDmy strength 04:27, 21 March 2015 (UTC)[reply]
I agree that the section isn't needed because all it conveys is the fact that the instrumentation is growing more accurate as time passes. It doesn't tell the reader anything new about the stars. If you absolutely have to retain it, I'd suggest moving it to the end of the article (as an appendix) so that it doesn't disrupt the flow. Praemonitus (talk) 16:40, 21 March 2015 (UTC)[reply]
Done..-The Herald the joy of the LORDmy strength 07:47, 22 March 2015 (UTC)[reply]
  • Both stars in the system are rather typical variable stars (BY Dra and flare). However, I'm not seeing magnitude ranges anywhere in this article for either star, which are absolutely necessary.
Now included..-The Herald the joy of the LORDmy strength 04:27, 21 March 2015 (UTC)[reply]

StringTheory11 (t • c) 15:26, 19 March 2015 (UTC)[reply]

  • Overall though, this article is pretty good. It is admittedly somewhat short, but that's not a problem; it's better to have only clear, concise, and relevant information and it covers its topic well.

StringTheory11 (t • c) 19:25, 18 March 2015 (UTC)[reply]

  • Question. In which book/document did Giuseppe Piazzi first demonstrate its large proper motion. Shouldn't that be somewhere in the reference? I couldn't find any reference to it. --Siddhant (talk) 21:21, 20 March 2015 (UTC)[reply]
I felt it very first. Still searching.....-The Herald the joy of the LORDmy strength 04:27, 21 March 2015 (UTC)[reply]
Done..-The Herald the joy of the LORDmy strength 04:42, 21 March 2015 (UTC)[reply]
Great! Since a complete scan of the book is available on Google Books, shouldn't that be linked to (while of course mentioning that the text is in Italian)? Do we know the page number on which 61 Cygni is mentioned (though I agree, that it might be too much to ask for)? --Siddhant (talk) 09:13, 21 March 2015 (UTC)[reply]
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