Jump to content

Talk:Gas dwarf

Page contents not supported in other languages.
From Wikipedia, the free encyclopedia

This is the current revision of this page, as edited by Cewbot (talk | contribs) at 08:16, 2 February 2024 (Maintain {{WPBS}} and vital articles: 1 WikiProject template. Create {{WPBS}}. Keep majority rating "Redirect" in {{WPBS}}. Remove 1 same rating as {{WPBS}} in {{WPAstronomy}}.). The present address (URL) is a permanent link to this version.

(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)

Merge with the Mini-Neptune article?

[edit]

There's already an article for mini-Neptune planets, and it's clear that both articles are referring to the same type of object (i.e. planets of sub-ice giant mass with significant envelopes of hydrogen, helium, and higher-mass volatiles). The mini-Neptune article even lists the term 'gas dwarf' as a synonym.

Each article has some information that the other doesn't though (like the metallicity-based distinctions listed in this one), so I think it makes sense to just take the best elements of each article and merge them.--203.57.211.237 (talk) 06:22, 1 January 2017 (UTC)[reply]