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 | The contents of the Gas dwarf page were merged into Mini-Neptune on 6 November 2019 and it now redirects there. For the contribution history and old versions of the merged article please see its history. |
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)
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| This redirect does not require a rating on Wikipedia's
content assessment scale. It is of interest to the following WikiProjects: | ||||||||||
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| The contents of the Gas dwarf page were merged into Mini-Neptune on 6 November 2019 and it now redirects there. For the contribution history and old versions of the merged article please see its history. |
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)