Talk:Habitability of G-type main-sequence star systems
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 | This article contains a translation of Habitabilidad en sistemas de enanas amarillas from es.wikipedia. (1084717175 et seq.) |
 | On 4 June 2025, it was proposed that this article be moved from Habitability of yellow dwarf systems to Habitability of G-type main-sequence star systems. The result of the discussion was moved. |
Translated?
[edit]Sofia Spinelli, just to be clear, this article was translated from the corresponding article on the Spanish Wikipedia? It should be tagged as such if that's the case. TornadoLGS (talk) 04:04, 27 April 2022 (UTC)
Requested move 4 June 2025
[edit]- The following is a closed discussion of a requested move. Please do not modify it. Subsequent comments should be made in a new section on the talk page. Editors desiring to contest the closing decision should consider a move review after discussing it on the closer's talk page. No further edits should be made to this discussion.
The result of the move request was: moved. Moved as an uncontested request with minimal participation. If there is any objection within a reasonable time frame, please ask me to reopen the discussion; if I am not available, please ask at the technical requests page. (closed by non-admin page mover) Jeffrey34555 (talk) 03:02, 19 June 2025 (UTC)
Habitability of yellow dwarf systems → Habitability of G-type main-sequence star systems – Consistency with other pages + "Yellow dwarf" is a misnomer, see G-type main-sequence star#Description. 21 Andromedae (talk) 22:32, 4 June 2025 (UTC) — Relisting. Jeffrey34555 (talk) 03:21, 12 June 2025 (UTC)