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Wikipedia:Articles for deletion/Qatar-3

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The following discussion is an archived debate of the proposed deletion of the article below. Please do not modify it. Subsequent comments should be made on the appropriate discussion page (such as the article's talk page or in a deletion review). No further edits should be made to this page.

The result was merge from Qatar-3b. (non-admin closure) ~ Aseleste (t, e | c, l) 08:08, 14 April 2021 (UTC)[reply]

Qatar-3 (edit | talk | history | protect | delete | links | watch | logs | views) – (View log)
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Fails WP:NASTRO. The only published research appears to be the discovery paper for a non-notable hot-Jupiter exoplanet (Qatar-3b, fairly longstanding article but possible also not notable). No popular coverage. Lithopsian (talk) 14:36, 26 March 2021 (UTC)[reply]

Qatar-3b (edit | talk | history | protect | delete | links | watch | logs | views)
Note: This discussion has been included in the list of Astronomy-related deletion discussions. Lithopsian (talk) 14:36, 26 March 2021 (UTC)[reply]
Relisted to generate a more thorough discussion and clearer consensus.
Relisting comment: A decision about which way round the merger should be would be useful here.
Please add new comments below this notice. Thanks, Black Kite (talk) 19:24, 6 April 2021 (UTC)[reply]
    • Is *anyone* arguing that the star and planet articles should be merged, and the merged article should be named after the planet? If so, what should be done in situations where there is a non-notable star that has several notable planets?PopePompus (talk) 19:30, 6 April 2021 (UTC)[reply]
    • I don't see how the title of the merged article is relevant for the AfD. In any case, this was discussed in WikiProject Astronomy, and the consensus was to merge under the star's name, as it can be done consistently for all exoplanets. Tercer (talk) 19:36, 6 April 2021 (UTC)[reply]
    • I agree completely. So I think we should just start merging the articles in situations like this one without having any AfD or related discussion at all. This situation pops up again and again, prompting the same multi-week discussion amongst the same people. Let's just merge them as soon as we notice them, on our own without discussion (be bold!) and if people complain we can then have a discussion about that.PopePompus (talk) 21:48, 6 April 2021 (UTC)[reply]
  • How is a star with a notable planet not therefore itself notable? Given the countless number of stars, aside from being unusually big or serving as an historical reference point in the sky, what else would serve as a point of notability? BD2412 T 00:42, 7 April 2021 (UTC)[reply]
    • Well in my opinion, the issue is not whether the star is notable. It's how articles about stars with exoplanets should be organized. We have seen a number of articles about stars which would not be notable were it not for the fact that they have exoplanets. Those pages tend to repeat much of the information that is also available in the separate article about the exoplanet, because that information has to be repeated to establish the notability of the star. So why not put the information about the star and all of its planets in a single article? That will reduce the amount of duplicated text and references (which makes it easier to keep the articles current and mutually consistent in the future), and provide a single place to find all the info about an entire stellar system. Since very little is known about most individual exoplanets at this point, and additional information is apt to be gathered very slowly, a single article about the entire system is not apt to be excessively long. I see no point in maximizing the number of separate Wikipedia articles by making a set of articles each of which has the minimum amount of notability to survive a AfD debate. Let's choose quality over quantity.PopePompus (talk) 01:05, 7 April 2021 (UTC)[reply]
    Notability is established by the existence of secondary and tertiary sources as described at WP:GNG. This policy is not easy to apply to astronomical objects and there is a specific policy giving guidelines about how to assess notability for them. I have argued that the policy is difficult to apply to exoplanets and it has certainly been widely ignore, but the basics are still there: being the subject of multiple non-trivial published works. The policy specifically describes that notability is not inherited, that is something is not notable purely because of association with something else which is notable. Hence a star is not necessarily notable because it has a notable planet. Looking again at the policy, notability is not established by the properties of the planet or star and especially not just by its existence, but by the attention paid to it in reliable sources. Again, this works better for people, fiction, etc. than to massive balls of rock or plasma in space, but it is how Wikipedia works. If an exoplanet, for example, has particularly unusual properties of some sort then it will generally have some coverage in at least multiple peer-reviewed journals, and hopefully some more general media also. All this doesn't necessarily resolve this discussion, but it does answer the question you asked. Lithopsian (talk) 13:59, 7 April 2021 (UTC)[reply]
  • Merge per PopePompus. Riteboke (talk) 08:00, 14 April 2021 (UTC)[reply]
  • Note: Qatar-3b has been added to facilitate the close with XFDcloser. ~ Aseleste (t, e | c, l) 08:05, 14 April 2021 (UTC)[reply]
The above discussion is preserved as an archive of the debate. Please do not modify it. Subsequent comments should be made on the appropriate discussion page (such as the article's talk page or in a deletion review). No further edits should be made to this page.