Talk:Rho Cassiopeiae

From Wikipedia, the free encyclopedia

WikiProject Astronomy 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.
Stub This article has been rated as Stub-Class on the assessment scale.

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.
This article has been automatically assessed as Stub-Class by WikiProject Astronomy because it uses a stub template.
  • If you agree with the assessment, please remove {{WPAstronomy}}'s auto=yes parameter from this talk page.
  • If you disagree with the assessment, please change it by editing the class parameter of the {{WPAstronomy}} template, removing {{WPAstronomy}}'s auto=yes parameter from this talk page, and removing the stub template from the article.

[edit] Accuracy

I filled in the starbox template with the most accurate information I could find, but it conflicts with the text to a significant degree. — RJH 23:40, 10 March 2006 (UTC)


[edit] near future?

"Astronomers predict Rho Cassiopeiae may become a supernova in the near future because it will soon have consumed most of its nuclear fuel."

What is considered "near future" in the context of this article? Stellar relative near future or human-lifespan relative near future? Other? A tangible number would help clarify. —Preceding unsigned comment added by Zerotta (talk • contribs) 16:18, 5 February 2008 (UTC)