Talk:Upsilon Andromedae c: Difference between revisions

	Upsilon Andromedae c has been listed as one of the Natural sciences good articles under the good article criteria. If you can improve it further, please do so. If it no longer meets these criteria, you can reassess it.
Article milestones Date Process Result July 13, 2006 Good article nominee Listed September 18, 2008 Good topic candidate Promoted February 23, 2009 Good article reassessment Kept February 11, 2015 Good topic removal candidate Demoted Current status: Good article

This article is rated GA-class on Wikipedia's content assessment scale. It is of interest to the following WikiProjects:

Astronomy: Astronomical objects Low‑importance This article is within the scope of WikiProject Astronomy, which collaborates on articles related to Astronomy on Wikipedia.AstronomyWikipedia:WikiProject AstronomyTemplate:WikiProject AstronomyAstronomy articles Low This article has been rated as Low-importance on the project's importance scale. This article is supported by WikiProject Astronomical objects, which collaborates on articles related to astronomical objects.

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After review, I've determined that this article meets the qualifications for GA status. It is well written, well referenced, and comprehensive. I'm "Mass Passing" this article along with 9 others. The entire list is below. If new developments arise that would effect the references or comprehensiveness of this article, it may affect the others as well.

• 55 Cancri b
• 55 Cancri c
• 55 Cancri d
• 55 Cancri e
• 16 Cygni
• 16 Cygni Bb
• Upsilon Andromedae
• Upsilon Andromedae b
• Upsilon Andromedae c
• Upsilon Andromedae d

Keep up the good work. These articles are ideal "good articles". They can't be FA, because there is no way for them to get long enough, but they are as comprehensive and complete as possible, and represent a good effort on the part of the editors. Feel free to message me if you have any questions about my rationale. Phidauex 18:18, 14 July 2006 (UTC)[reply]

are Upsilon Andromedae c and d confirmed exoplanets? thanks.--190.21.202.38 (talk) 21:26, 13 May 2008 (UTC)[reply]

As part of the WikiProject Good Articles, we're doing sweeps to go over all of the current GAs and see if they still meet the GA criteria. I'm specifically going over all of the "Planets and Moons" articles. I believe the article currently meets the criteria and should remain listed as a Good article. I have made several minor corrections throughout the article. Altogether the article is well-written and is still in great shape after its passing in 2006. Continue to improve the article making sure all new information is properly sourced and neutral. I would recommend going through all of the citations and updating the access dates and fixing any dead links. If you have any questions, let me know on my talk page and I'll get back to you as soon as I can. I have updated the article history to reflect this review. Happy editing! --Nehrams2020 (talk) 08:27, 24 February 2009 (UTC)[reply]

I know that the distinguishing low-mass brown dwarfs from high-mass planets is rather difficult, but If the planet mass is 13.98 then it should be qualified as a brown dwarf star. Is it not true? —Preceding unsigned comment added by Donlevone (talk • contribs) 21:07, 23 November 2010 (UTC)[reply]

Why are we using a radial velocity minimum mass (1.98 Jupiter masses), as opposed to the astrometrically-derived true mass (13.98 Jupiter masses)? 46.126.76.193 (talk) 07:39, 24 November 2012 (UTC)[reply]

There is a move discussion in progress on Talk:Upsilon Andromedae d which affects this page. Please participate on that page and not in this talk page section. Thank you. —RMCD bot 02:59, 17 December 2015 (UTC)[reply]