Talk:HD 217107 b

From Wikipedia, the free encyclopedia

This is the talk page for discussing improvements to the HD 217107 b article.
Please sign and date your posts by typing four tildes (~~~~). Put new text under old text. Click here to start a new topic. New to Wikipedia? Welcome! Ask questions, get answers. This is not a forum for general discussion about the article's subject.	Be polite Assume good faith No personal attacks Be welcoming	Article policies No original research Neutral point of view Verifiability

	HD 217107 b has been listed as one of the Natural sciences good articles under the good article criteria. If you can improve it further, please do. If it no longer meets these criteria, you can delist it, or ask for a reassessment.
April 25, 2006 Good article nominee Listed

	Portal This article is within the scope of WikiProject Astronomy, which collaborates on articles related to astronomy, and WikiProject Astronomical Objects, which collaborates on articles related to astronomical objects.
GA	This article has been rated as GA-Class on the assessment scale.
Help with this template This article has been rated but has no comments. If appropriate, please review the article and leave comments here to identify the strengths and weaknesses of the article and what work it will need.

[edit] Redirected

All extrasolar planets are sectioned in it's stars artical. The only time exoplanets are made into there own artical is if they are of big news and of public intrest (i.e. OGLE-2005-BLG-390Lb, 51 Pegasi b, HD 188753 Ab). These planets are not of any of these standerds, why should they be treeted with royalty. They should be in the star's artical as of wiki rules and tradition. — HurricaneDevon @ 03:13, 25 April 2006 (UTC)