Wikipedia:Good article reassessment/Stellar rotation/1
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The following discussion is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.
- Article (edit | visual edit | history) · Article talk (edit | history) · Watch • Watch article reassessment page • GAN review not found
- Result: A second opinion seems to support this article not being up to GA standards with suggestions given for improvement. Bgsu98 (Talk) 21:24, 29 November 2025 (UTC) [reply ]
Uncited statements, including entire paragraphs. Z1720 (talk) 15:30, 9 November 2025 (UTC) [reply ]
- The article is okay, but I think it is weak on some topics and missing coverage of others. I would expect to see the article discuss Be stars and shell stars in the context of mass loss due to rapid rotation. It should expand on gravity darkening, and discuss the effect of metallicity on the evolution of rotation.[1] As stars evolve into giants, the expansion should impact the rotation. What about stars that have a more rapid internal spin rate?[2] Finally, it can discuss the impact of planets (such as hot Jupiters) on stellar rotation. Praemonitus (talk) 23:40, 20 November 2025 (UTC) [reply ]
The discussion above is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.