| This is the talk page for discussing improvements to the Sun article. This is not a forum for general discussion of the subject of the article. |
Article policies
|
| Find sources: Google (books · news · scholar · free images · WP refs) · FENS · JSTOR · TWL |
| Archives: 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11Auto-archiving period: 3 months |
| This article is written in British English, which has its own spelling conventions (colour, travelled, centre, defence, artefact, analyse) and some terms may be different or absent from other varieties of English. According to the relevant style guide, this should not be changed without broad consensus. |
| Sun is a featured article; it (or a previous version of it) has been identified as one of the best articles produced by the Wikipedia community. Even so, if you can update or improve it, please do so. | ||||||||||||||||||||||||||||
| Sun is part of the Solar System series, a featured topic. This is identified as among the best series of articles produced by the Wikipedia community. If you can update or improve it, please do so. | ||||||||||||||||||||||||||||
| This article appeared on Wikipedia's Main Page as Today's featured article on March 20, 2006, and on March 20, 2025. | ||||||||||||||||||||||||||||
| ||||||||||||||||||||||||||||
| This It is of interest to the following WikiProjects: | |||||||||||||||||||||||||||||||||||||||||||||||
| |||||||||||||||||||||||||||||||||||||||||||||||
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
I can’t see the image fully ~2026-93758-4 (talk) 15:52, 11 February 2026 (UTC)
This edit request has been answered. Set the |answered= parameter to no to reactivate your request. |
Under the Sun#Formation heading there is the following text. This edit should be made to add a link to a relevant article:
| − | The stars [[HD 162826]] and [[HD 186302]] share similarities with the Sun and are hypothesised to be | + | The stars [[HD 162826]] and [[HD 186302]] share similarities with the Sun and are hypothesised to be [[solar sibling]]s, formed in the same molecular cloud as the Sun. |
The stars HD 162826 and HD 186302 share similarities with the Sun and are hypothesised to be solar siblings, formed in the same molecular cloud as the Sun. Ronjohnbonpon (talk) 19:11, 21 July 2026 (UTC)
I find it very hard to believe that the sun at present contains more hydrogen and less helium than at the time it was formed. After all it spent a few billion years converting hydrogen into helium See Sun#Composition ~2026-42779-07 (talk) 21:30, 1 August 2026 (UTC)
This edit request has been answered. Set the |answered= parameter to no to reactivate your request. |
In the Physical characteristics tab.
Please change the Volume value from 1.412×1018 km3 to 1.410×1018 km3.So that it correlated with the existing Equatorial radius value of 695,700 km. ~2026-43091-55 (talk) 23:07, 5 August 2026 (UTC)
these values should not be considered the true solar/planetary properties. They should be understood as conversion values only.Johnjbarton (talk) 02:26, 6 August 2026 (UTC)
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.