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{{DISPLAYTITLE:'''<span style="font-family:arial"><span><span style="color:#1c3587;">User talk:SpaceImplorer</span><span style="color:#1c877c;">ExplorerImplorer</span>'''}}
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Copyright



Hi - I just reviewed Ackermannviridae ↗, and I'm afraid I cut out a section of it because it was basically word-for-word the same as the source. It's really tricky when you're working from a single source to come up with your own phrasing, and I didn't want to attempt a redraft myself because I don't have the requisite subject-matter knowledge to come up with appropriate alternative language, but I thought I'd better let you know. You can find out more about our copyright policy at COPYVIO ↗. Thanks <span style="font-family:Impact;color:#294;">Girth</span><span style="font-family:Impact;color:#42c;">Summit</span><sub style="font-family:script;color:blue;"> (blether)</sub> 19:52, 4 March 2020 (UTC)

List of virus species



I appreciate the enthusiasm on List of virus species ↗. However, I reverted your changes as the viruses you added are not currently accepted as species at the International Committee on Taxonomy of Viruses ↗, which is the source listed in the citation for the list. It doesn't mean they are bad articles or aren't 'real' viruses, just that they shouldn't be on the list. I know that the ICTV members are voting on the updated taxonomy now, and will ratify and publish it soon. When that happens, the list here should be updated with the new information and will likely have some of the new species you are interested in. Cheers! --awkwafaba (📥) 19:09, 10 March 2020 (UTC)

Recent changes



25px|alt=Information icon ↗ Hello. While we appreciate your attempts to help keep scientific classifications on Wikipedia thorough and up-to-date, {{#if:|your recent edit to the code at {{{1}}}|one of your recent edits}} doesn't fit the format required for the taxonomy templates to function properly, and it has been reverted or removed. Please have a look at the automatic taxobox documentation ↗ where you can find answers to frequently-asked questions as well as guidelines for tweaking the taxonomy templates. If you need further assistance, consider asking for assistance ↗. If you wish to make test edits, please do them in the sandbox ↗. Thank you.<!-- Template:Uw-taxonomy1 --> --awkwafaba (📥) 18:23, 11 March 2020 (UTC)

March 2020



25px|alt=Information icon ↗ Hello, and thank you for your contributions to Wikipedia. A page you recently created, :Kepler-298 ↗, may not conform to some of Wikipedia's guidelines ↗ for new pages, so it has been moved to Draft:Kepler-298 ↗ where you can continue to work on it. Please consider using the Article Wizard ↗ or the Articles for Creation ↗ procedure. For more information about creating articles, you may want to read "Your first article ↗". You may also want to read our introduction page ↗ to learn more about contributing. Please add the body text of the article in your first submission or shortly after; articles without infoboxes are eligible for speedy deletion under criterion A3 ↗ after 10 minutes. <!-- Template:uw-articletodraft --> <b><span style="color:#E68A00;">Passenger</span><span style="color:#4C6680;">pigeon</span> ↗ (<span style="color:grey;">talk</span>)</b> 22:15, 13 March 2020 (UTC)

March 2020



25px|alt=Information icon ↗ Thank you for your contributions ↗ to Wikipedia. Regarding your edits to :List of largest exoplanets ↗, please use the preview ↗ button before you save your edit; this helps you find any errors you have made and prevents clogging up recent changes ↗ and the page history ↗, as well as helping prevent edit conflicts ↗. Below the edit box is a '''Show preview''' button. Pressing this will show you what the article will look like without actually saving it.
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Thank you. <!-- Template:uw-preview --> Jessicapierce (talk) 22:58, 14 March 2020 (UTC)

SDSS J140821.67+025733.2 ↗ moved to draftspace



An article you recently created, SDSS J140821.67+025733.2 ↗, does not have enough sources and citations as written to remain published. It needs more citations from reliable ↗, independent sources ↗. <small>(? ↗)</small> Information that can't be referenced should be removed (verifiability ↗ is of central importance ↗ on Wikipedia). I've moved your draft to draftspace ↗ (with a prefix of "<code>Draft:</code>" before the article title) where you can incubate the article with minimal disruption. When you feel the article meets Wikipedia's general notability guideline ↗ and thus is ready for mainspace, please click on the "Submit your draft for review!" button at the top of the page. Minorax (talk) 15:44, 17 March 2020 (UTC)

Guidelines for adding new planets



I noticed you added 4 planets to List of exoplanets discovered in 2020 ↗. While all of these are planets previously not reported in wikipedia lists, several points are need to be addressed to improve the quality of your contributions:

Trurle (talk) 23:01, 26 March 2020 (UTC)

Disambiguation link notification for April 6



Hi. Thank you for your recent edits. An automated process has detected that when you recently edited List of mountains by elevation ↗, you added a link pointing to the disambiguation page Laram Q'awa ↗ ([//dispenser.info.tm/~dispenser/cgi-bin/dablinks.py/List_of_mountains_by_elevation check to confirm]&nbsp;|&nbsp;[//dispenser.info.tm/~dispenser/cgi-bin/dab_solver.py/List_of_mountains_by_elevation?client=notify fix with Dab solver]). Such links are usually incorrect ↗, since a disambiguation page is merely a list of unrelated topics with similar titles. <small>(Read the FAQ{{*}} Join us at the DPL WikiProject ↗.)</small>

It's OK to remove this message. Also, to stop receiving these messages, follow these opt-out instructions. Thanks, DPL bot (talk) 08:21, 6 April 2020 (UTC)

Taxonomy errors



Some recent edits at Template:Taxonomy/Mimiviridae ↗ appear to have caused errors ("Lua error in Module:Autotaxobox at line 156: attempt to index a nil value") at:
Also, Template:Taxonomy/Megavirales ↗ seems to be unfinished. Please fix the problems soon or revert your changes because the errors need to be removed. Johnuniq (talk) 09:11, 6 April 2020 (UTC)

Your contributed article, :Full list of minor planets ↗


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{{Quote box|quote=<p>If this is the first article that you have created, you may want to read the guide to writing your first article ↗.</p><p>You may want to consider using the Article Wizard ↗ to help you create articles.</p>|width=20%|align=right}}
Hello, I noticed that you recently created a new page, ''':Full list of minor planets ↗'''. First, thank you for your contribution; Wikipedia relies solely on the efforts of volunteers such as you. Unfortunately, the page you created covers a topic on which we already have a page – ''':List of minor planets ↗'''. Because of the duplication, your article has been tagged for speedy deletion ↗. Please note that this is not a comment on you personally and we hope you will continue helping to improve Wikipedia. If the topic of the article you created is one that interests you, then perhaps you would like to help out at :List of minor planets ↗. If you have new information to add, you might want to discuss it at the article's talk page ↗.

If you think the article you created should remain separate, you may '''contest the nomination''' by visiting the page ↗ and clicking the button labelled "Contest this speedy deletion". This will give you the opportunity to explain why you believe the page should not be deleted. However, be aware that once a page is tagged for speedy deletion, it may be deleted without delay. Please do not remove the speedy deletion tag from the page yourself, but do not hesitate to add information in line with Wikipedia's policies and guidelines ↗. If the page is deleted, and you wish to retrieve the deleted material for future reference or improvement, then please contact the {{Querylink|Special:Log|qs=type=delete&page=Full+list+of+minor+planets|deleting administrator}}, or if you have already done so, you can place a request here ↗. Additionally if you would like to have someone review articles you create before they go live so they are not nominated for deletion shortly after you post them, allow me to suggest the article creation process ↗ and using our search feature to find related information we already have in the encyclopedia. Try not to be discouraged. Wikipedia looks forward to your future contributions.<!-- Template:Db-csd-notice-custom --> MrClog (talk) 10:31, 7 April 2020 (UTC)

April 2020


25px|alt=Information icon ↗ Welcome ↗ to Wikipedia. It might not have been your intention, but you removed a speedy deletion ↗ tag from :Full list of minor planets ↗, a page you have created yourself. If you believe the page should not be deleted, you may contest the deletion by clicking on the button that says: '''Contest this speedy deletion''' which appears inside the speedy deletion notice. This will allow you to make your case '''''on the talk page ↗'''''. Administrators will consider your reasoning before deciding what to do with the page. Thank you.<!-- Template:uw-speedy1 --> MrClog (talk) 10:59, 8 April 2020 (UTC)

Speedy deletion ↗ nomination of :Draft:Kepler-298 ↗


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{{Quote box|quote=<p>If this is the first article that you have created, you may want to read the guide to writing your first article ↗.</p><p>You may want to consider using the Article Wizard ↗ to help you create articles.</p>|width=20%|align=right}}
Hello, and welcome to Wikipedia. This is a notice that the page you created, :Draft:Kepler-298 ↗, was tagged as a test page under section G2 of the criteria for speedy deletion ↗ and has been or soon may be deleted. Please use the sandbox ↗ for any other tests you want to do. Take a look at the welcome page ↗ if you would like to learn more about contributing to our encyclopedia.

If you think this page should not be deleted for this reason, you may '''contest the nomination''' by visiting the page ↗ and clicking the button labelled "Contest this speedy deletion". This will give you the opportunity to explain why you believe the page should not be deleted. However, be aware that once a page is tagged for speedy deletion, it may be deleted without delay. Please do not remove the speedy deletion tag from the page yourself, but do not hesitate to add information in line with Wikipedia's policies and guidelines ↗. If the page is deleted, and you wish to retrieve the deleted material for future reference or improvement, then please contact the {{Querylink|Special:Log|qs=type=delete&page=Draft%3AKepler-298|deleting administrator}}, or if you have already done so, you can place a request here ↗. <!-- Template:Db-test-notice --><!-- Template:Db-csd-notice-custom --> Golem08 (talk) 14:46, 10 April 2020 (UTC)
:I have contested the deletion of this draft, so it will not be speedily deleted. Best, MrClog (talk) 21:03, 10 April 2020 (UTC)

UY Scuti


Please don't remove references from articles, especially with no explanation, as you did at UY Scuti ↗. And please don't then edit the data without providing a new reference. You edits could be interpreted as disruptive, especially when repeated across multiple articles. Lithopsian (talk) 19:00, 1 June 2020 (UTC)

Disambiguation link notification for June 3



An automated process has detected that when you recently edited V538 Carinae ↗, you added a link pointing to the disambiguation page Carina ↗ ([//dispenser.info.tm/~dispenser/cgi-bin/dablinks.py/V538_Carinae check to confirm]&nbsp;|&nbsp;[//dispenser.info.tm/~dispenser/cgi-bin/dab_solver.py/V538_Carinae?client=notify fix with Dab solver]).

(Opt-out instructions.) --DPL bot (talk) 08:21, 3 June 2020 (UTC)

July 2020


25px|alt=Information icon ↗ Hello, I'm Tarl N.. Your recent edit(s) to the page :Messier 87 ↗ appear to have added incorrect information, so they have been removed for now. If you believe the information was correct, please cite a reliable source ↗ or discuss your change on the article's talk page. If you would like to experiment, please use the sandbox ↗. If you think I made a mistake, or if you have any questions, you can leave me a message on my talk page. Thank you. <!-- Template:uw-error1 --> <b style="color:green">Tarl N.</b> (<span style="color:teal">discuss</span>) 16:28, 2 July 2020 (UTC)

25px|alt=Information icon ↗ Hello, I'm CLCStudent. I noticed that you recently removed content without adequately explaining why. In the future, it would be helpful to others if you described your changes to Wikipedia with an accurate edit summary ↗. If this was a mistake, don't worry; the removed content has been restored. If you would like to experiment, please use the sandbox ↗. If you think I made a mistake, or if you have any questions, you can leave me a message on my talk page ↗. Thanks.<!-- Template:uw-delete1 --> CLCStudent (talk) 13:00, 15 July 2020 (UTC)

Your draft article, Draft:Taxonomy/Megavirales ↗


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Hello, SpaceImplorerExplorerImplorer. It has been over six months since you last edited the Articles for Creation ↗ submission or Draft ↗ page you started, "Megavirales ↗".

In accordance with our policy that Wikipedia is not for the indefinite hosting of material deemed unsuitable for the encyclopedia mainspace ↗, the draft has been deleted. If you plan on working on it further and you wish to retrieve it, you can request its undeletion by following the instructions at this link ↗. An administrator will, in most cases, restore the submission so you can continue to work on it.

Thanks for your submission to Wikipedia, and happy editing. <!-- Template:Db-draft-deleted --><!-- Template:Db-csd-deleted-custom --> <span style="font-family:Papyrus; color:#800080;">'''''L'''''iz</span> <sup style="font-family: Times New Roman; color: #006400;">'''''Read!''''' ↗ '''''Talk!'''''</sup> 00:03, 7 October 2020 (UTC)

Your draft article, Draft:Kepler-298 ↗


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Hello, SpaceImplorerExplorerImplorer. It has been over six months since you last edited the Articles for Creation ↗ submission or Draft ↗ page you started, "Kepler-298 ↗".

In accordance with our policy that Wikipedia is not for the indefinite hosting of material deemed unsuitable for the encyclopedia mainspace ↗, the draft has been deleted. If you plan on working on it further and you wish to retrieve it, you can request its undeletion by following the instructions at this link ↗. An administrator will, in most cases, restore the submission so you can continue to work on it.

Thanks for your submission to Wikipedia, and happy editing. <!-- Template:Db-draft-deleted --><!-- Template:Db-csd-deleted-custom --> <span style="font-family:Papyrus; color:#800080;">'''''L'''''iz</span> <sup style="font-family: Times New Roman; color: #006400;">'''''Read!''''' ↗ '''''Talk!'''''</sup> 00:14, 11 October 2020 (UTC)

ArbCom 2020 Elections voter message



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Ways to improve PMMR 62



Hello, SpaceImplorerExplorerImplorer,

Thank you for creating PMMR 62 ↗.

I have tagged the page ↗ as having some issues to fix, as a part of our page curation process ↗ and note that:

{{Quote|1=see WP:NASTRO ↗ for notability guidline}}

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Graeme Bartlett (talk) 22:15, 17 March 2021 (UTC)

Autopatrolled rights



For what it's worth, contrary to your user page statement, you do ''not'' have autopatrolled rights. See here ↗. <b style="color:green">Tarl N.</b> (<span style="color:teal">discuss</span>) 18:20, 26 April 2021 (UTC)

:Category:LGGS objects ↗ has been nominated for deletion



<div class="floatleft" style="margin-bottom:0">48px|alt=|link= ↗</div>''':Category:LGGS objects ↗''' has been nominated for deletion. A discussion is taking place to decide whether this proposal complies with the categorization ↗ guidelines. If you would like to participate in the discussion, you are invited to add your comments at '''the category's entry ↗''' on the categories for discussion ↗ page.<!-- Template:Cfd-notify--> Thank you. Lithopsian (talk) 19:16, 28 May 2021 (UTC)

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Page moves



In the future, if a page needs to move to a location where there is already a page and/or redirect, please use WP:RM/TR ↗ to ask an administrator or page mover to handle it; copying and pasting within Wikipedia purely for the purposes of moving a page has long been deprecated and creates all sorts of issues. Primefac (talk) 12:35, 30 November 2021 (UTC)

List of largest known stars ↗



Consider this your final warning for the List of largest known stars; this edit summary ↗ makes it sound like you didn't even read the source, let alone the fact that it ''was'' in the correct section. Continue reverting without actually checking things and you will be blocked from editing the page. Primefac (talk) 17:09, 11 May 2022 (UTC)

:I '''''did''''' read the source and I had mistaken it for the Milky Way section and I did realise that it was after that although I couldn't change the edit summary, it is that simple. Also, I'm not trying to vandalise Wikipedia and I '''am''' trying to improve it. Another thing is that it does not make sense to call it my ''"final warning"'' because this is only my first warning for this page ever (at least on my user talk). '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#0000ff">SpaceImplorer</span><span style="color:#00ffff">ExplorerImplorer</span> (<span style="color:#0000ff">ta</span><span style="color:#00ffff">lk</span>)</span>''' 17:13, 11 May 2022 (UTC)

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LMC/SMC + M31/M33 red supergiants



Did you email the authors of https://ui.adsabs.harvard.edu/abs/2022arXiv221114147M/abstract ↗ to obtain the full tables? Could you send them to me? <span style="font-family:times;background-color:black;padding:2px 3px 2px 3px"><span style="color:#ffc08c">VY Canis Majoris</span></span> (talk) 08:45, 2 January 2023 (UTC)

:All the stars are in the article. For the lower luminosity stars go to pages 29-32 and for the higher luminosity stars go to pages 34-35 (in the arXiv version). '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#0000ff">SpaceImplorer</span><span style="color:#00ffff">ExplorerImplorer</span> (<span style="color:#0000ff">ta</span><span style="color:#00ffff">lk</span>)</span>''' 09:15, 2 January 2023 (UTC)

Your submission at Articles for creation ↗: PGC 2933 ↗ has been accepted


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Your submission at Articles for creation ↗: AZ Cygni ↗ has been accepted


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Template val



I reverted your change at HV 11417 ↗, where you replaced the {{tl|val}} template with a number containing a comma for the thousands separator. The reason we use the val template is that not everyone uses commas for digit grouping - in some regions, the comma is a decimal marker (among English-speaking nations, South Africa). In others, the commas go at different intervals (see Decimal separator#Digit grouping ↗). The compromise is to use a thin space separator every three digits before the decimal, which is accomplished by the val template. Regards, <b style="color:green">Tarl N.</b> (<span style="color:teal">discuss</span>) 07:06, 11 February 2023 (UTC)

Your submission at Articles for creation ↗: Y Cygni ↗ (February 20)


<div style="border: solid 1px #FCC; background-color: #F8EEBC; padding: 0.5em 1em; color: #000; margin: 1.5em; width: 90%;"> 50px|left ↗Your recent article submission to Articles for Creation ↗ has been reviewed! Unfortunately, it has not been accepted at this time.<nowiki> </nowiki>The reason left by InterstellarGamer12321 was:

{{divbox|gray|3=This submission is not adequately supported by reliable sources ↗. ''Reliable'' sources are required so that information can be verified ↗. If you need help with referencing, please see Referencing for beginners ↗ and Citing sources ↗.|}}<!--
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-->&nbsp;The comment the reviewer left was:

{{divbox|blue|3=The Observation history section is entirely unsourced, while the Characteristics section is empty. More references are needed to establish notability.}} Please check the submission for any additional comments left by the reviewer. You are encouraged to edit the submission to address the issues raised and resubmit ''after they have been resolved''.
{{clear}}

<b>InterstellarGamer12321</b> (<span style="color:#157710;">talk</span> &#124; <span style="color:#e00000;">contribs</span> ↗) 12:07, 20 February 2023 (UTC)</div><!--Template:AfC decline-->

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<!-- Template:Afd notice --></div> Lithopsian (talk) 14:11, 27 June 2023 (UTC)

Regarding the 90,000 Lsol estimate for Stephenson 2 DFK 1



This estimate is not accurate, it only considers a small range of fluxes (12-25 μm). This luminosity as well as the 630,000 Lsol one get the value from integrating the spectral energy distribution, which basically means the area under the curve of the flux as a function of wavelength. Since the 90,000 Lsol estimate only considers a narrow range of wavelength space, it only encapsulates a small fraction of the total area, and hence underestimates the luminosity. Pretty sure the 630,000 Lsol value also uses the same IRAS photometry, but also considers the full wavelength range so does not underestimate the luminosity. <span style="font-family:times;background-color:black;padding:2px 3px 2px 3px"><span style="color:#ffc08c">VY Canis Majoris</span></span> (talk) 19:50, 11 July 2023 (UTC)

:I am not underestimating the luminosity. I was quite sure it was not so accurate, but it was the best one I could find. Read what I stated in the talk page. '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#0000ff">SpaceImplorer</span><span style="color:#00ffff">ExplorerImplorer</span></span>''' 12:08, 12 July 2023 (UTC)
::The 90,000 Lsol value is still an underestimate even if it seems more plausible, it cannot be used. Even assuming the star is foreground its kinematic distance only reduces to 5.1 kpc, reducing its logL to 5.57 or 5.69 for Humphreys' estimate. <span style="font-family:times;background-color:black;padding:2px 3px 2px 3px"><span style="color:#ffc08c">VY Canis Majoris</span></span> (talk) 15:46, 12 July 2023 (UTC)
:::I do agree that it is an underestimate (and I don’t use that luminosity anymore). The distance is still uncertain and the star not well studied. The {{solar luminosity|277,000|fmt=commas}} calculation I mentioned was only based on an assumed extinction. I would therefore say that a logL of 5.57-5.69 is possible but the star needs further research for there to be higher certainty and if it is a red supergiant, the logL is somewhere in the range of 5 to more than 5.6'''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#0000ff">SpaceImplorer</span><span style="color:#00ffff">ExplorerImplorer</span></span>''' 16:00, 12 July 2023 (UTC)

CS1 error on List of smallest exoplanets ↗


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Addressing the spectral types of VY Canis Majoris and radius regarding them



I see that on the VY Canis Majoris page, you stated the value of 2,069 solar radii for VY Canis Majoris is based off an effective temperature inconsistent with its spectral type.

However, VY Canis Majoris is said to have spectral types of M3, M4.5, M2.5, and M5e Ia.

The different spectral types would affect the temperature, and therefore the radius.

We know for certain it's an irregular pulsating variable star.

While the radius of 1,420 solar radii falls within the current theoretical limit for a star's radius in our theory of stellar evolution, pulsations mean the radius changes and that's more true for radial pulsations.

Whether its size ranges from 1,300 to 1,540 (in addition to the margin of error for its calculated radius) or up to 2,069 solar radii (in addition to cool-end of estimates adopted temperature of 2,800 K and a luminosity of 237,000 x that of the Sun) in its pulsations, very little detail was explained in your statement with hardly anything addressed.

The explanation for the edit was somewhat confusing though, just saying. Eric Nelson27 (talk) 10:31, 4 December 2023 (UTC)

:The original paper in with 2800 K in 1996 does still have extremely low and obsolete effective temperatures for many stars and includes enormous luminosities. It is better to use a physically possible one, rather than an outdated and spurious one. '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#0000ff">SpaceImplorer</span><span style="color:#00ffff">ExplorerImplorer</span></span>''' 10:58, 4 December 2023 (UTC)
::I see and agree. Eric Nelson27 (talk) 14:28, 4 December 2023 (UTC)

List of largest known stars ↗



<div notice" style="background:transparent; margin:0.5em auto; width:100%;">
25px|link= ↗Thank you for your contributions ↗ to Wikipedia ↗. You have reverted ↗ my edit at List of largest stars ↗, because you thought my edit was breaching the WP:SYNTHESIS ↗ rule. Although using two different sources to calculate a radius seems to violate the Synthesis rule, it actually doesn't.

<br />A WP:SYNTHESIS violation happens only to original research ↗ by synthesis, not to synthesis per se. See Wikipedia:What SYNTH is not#SYNTH is not just any synthesis ↗. Calculating a radius of a star using its angular diameter and radius is not considered original research ↗, because simple calculations (it is a simple calculation that can be easily made using a template) are not original research per WP:CALC ↗. Therefore, if it is not original research (according to WP:CALC), it is not WP:SYNTHESIS.

Thanks! InTheAstronomy32 (talk) 19:57, 30 April 2024 (UTC)
</div>
:A statement by you does not make something true. WP:SYNTHESIS ↗ applies to the use of "facts" from two different sources to derive a third "fact", even if the calculation is trivial. Hence, a radius derived using a distance from one source and an angular radius from a different source violate WP:SYNTHESIS ↗, even though the calculation is trivial. If you feel differently, take it to a wider audience such as e project talk page. Lithopsian (talk) 17:31, 20 May 2024 (UTC)
::It appears that you are misinterpreting this rule. First of all, WP:SYNTH doesn't necessarily refer to using two or more sources:{{tq|"Similarly, do not combine different parts of one source to reach or imply a conclusion not explicitly stated by the source"}}. Then, all articles that have calculated radii from a luminosity and effective temperature (common in Star-like articles) would be breaching WP:SYNTHESIS, but it doesnt, because routine calculations ↗ are not considered original research, hence are not WP:SYNTHESIS ↗. The radius can be calculated using {{tl|Solar radius calculator}} or the equation Diameter (AU) = AD ↗ (arcsec) × Distance (pc). InTheAstronomy32 (talk) 12:07, 21 May 2024 (UTC)
::It only violates the letter, not the spirit ↗ of the policy. The WP:No original research ↗ policy was made to make all content in the articles verifiable, and the radius itself is verifiable. InTheAstronomy32 (talk) 12:10, 21 May 2024 (UTC)

Radius of UY Scuti



Where i can find the radius of UY Scuti ({{solar radius|909}}) in the Healy et al. 2023 reference? In your edit summary, you said the data can only be accessed in the Github table (https://github.com/SNEWS2/candidate_list?tab=readme-ov-file ↗), but in this link there are several files and folders, which make it difficult to find which one is correct. InTheAstronomy32 (talk) 19:49, 23 May 2024 (UTC)

:Go to <code>data/Final_RSG_Catalog_8_10_2023.csv</code>. '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 20:47, 23 May 2024 (UTC)
::Thanks. The GitHub file is practically unreadable because it is in .csv ↗ format, so I downloaded it and put it in a spreadsheet editor that automatically converts csv files to tables. InTheAstronomy32 (talk) 22:15, 23 May 2024 (UTC)
::I uploaded the spreadsheet at Mega (<nowiki>https://mega.nz/file/Dbw1zSbS#DkSsykTYmCDEWrFZbQHEaGKSLjDsQQuHFq3SKo-yVmY</nowiki>). While the authors of the paper don't place data at VizieR it will be useful. InTheAstronomy32 (talk) 22:58, 23 May 2024 (UTC)

Your submission at Articles for creation ↗: List of most massive star clusters ↗ has been accepted


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Emdashes



Why so few em dashes? Are you scared of them? Polygnotus (talk) 04:22, 21 December 2025 (UTC)

A question



Greetings, i am owner of Phoenicis Studio, and, recently, GoldSaturn (administrator of a team) suggested me a your work about sizes of composite particles (https://docs.google.com/spreadsheets/d/1n1BIivw13od6ttrZ3MW-_RpoYUXK3h6E/edit?usp=drivesdk&ouid=105487786821132977354&rtpof=true&sd=true). I wanted to ask you, which formula you used to determine that? If there is any constants, can you show me its values and also units that was used in there.
Write back soon. Vizier other accoun t (talk) 16:24, 24 June 2026 (UTC)

:One that isn't correct. You can find reliable charge and magnetic radii in scientific literature elsewhere. '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 17:10, 24 June 2026 (UTC)
::Sorry, but i need direct formula. The reason is that im trying to calculate size of recently discovered composite particles and there is no papers at all for most of particles (im talking about resonances and exotic ones btw), so please
::Also i noticed that your results is consistent for most proper sizes, so it is correct actually Vizier other accoun t (talk) 10:37, 25 June 2026 (UTC)
:::And yes, can you just give me formula First Vizier other accoun t (talk) 14:11, 25 June 2026 (UTC)
:::I'm pretty sure it can only be determined experimentally. And the formula used for that spreadsheet still isn't right, even if it is consistent with a few.
:::I found one formula but I am not sure if it applies for particles other than a proton or neutron:
:::<math><r_{E}^2>=-6\frac{dG_{E}(Q^2)}{dQ^2}|_{Q^2=0}</math>
:::Where G<sub>E</sub>(Q<sup>2</sup>) is the Sachs electric form factor. I'm still trying to figure out how to solve it though. '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 19:38, 27 June 2026 (UTC)
:::I will also note that the radius of a hadron can be defined using the distribution of multiple different properties and will yield different results depending on the one you choose. Charge is the most commonly used one I have seen but doesn't apply in the way you would expect for neutral particles. '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 20:03, 27 June 2026 (UTC)
::::Thanks! Vizier other accoun t (talk) 07:57, 28 June 2026 (UTC)
:::::I will also mention that the formula for the Sachs electric form factor is
:::::<math>G_{E}(Q^{2})=F_{1}(Q^{2})+\tau F_{2}(Q^{2})</math>,
:::::where <math>\tau=\frac{Q}{4m_{p}^{2}}</math>.
:::::I still cannot find any functions to deduce the Dirac and Pauli form factors. (F<sub>1</sub>(Q<sup>2</sup>) and F<sub>2</sub>(Q<sup>2</sup>)) '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 15:07, 30 June 2026 (UTC)
:::::{{strikethrough|I found another formula here ↗ derived by modelling a simple harmonic oscillator to describe any interaction between baryons:}}
:::::{{strikethrough|<math>\frac{\frac{\sqrt{m_{1}(n+1)}}{k_{1}}+\frac{\sqrt{m_{2}(m+1)}}{k_{2}}+\frac{\sqrt{m_{3}(l+1)}}{k_{3}}}{3}</math>,}}
:::::{{strikethrough|where ''m''<sub>i</sub> is the mass, n, m and l are integers to represent excitations, and ''k''<sub>i</sub> is a constant. The three added functions are for the individual quarks.}}
:::::{{strikethrough|There are values of k given in the paper for the individual quarks, however they do not seem to be reliable. I calculated rough values for them, although I will try refining them tomorrow.}}
:::::'''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 23:10, 30 June 2026 (UTC)
:::::{{strikethrough|Here are the new values that I calculated:}}
:::::{{strikethrough|I also made a calculator with sources here ↗. I also noticed that the values given in there are mostly reliable considering the quarks' mass-energies, however they do not seem to make much of a difference to the final radius. (Do tell me if you find any major discrepancies with literature) The sum of the n, m and l values should be equal to ''J<sup>P</sup>''{{snd}}1/2. For baryons with ''J<sup>P</sup>'' values greater than 3/2, use the average of all the possible radii that involve the correct energy. (In this case use the other formula which does use mass-energies given in the paper)}} '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 10:43, 1 July 2026 (UTC)
::::::Thanks! I will try to test it tomorrow. Vizier other accoun t (talk) 14:01, 1 July 2026 (UTC)
:::::::{{strikethrough|Another thing that I will add is that the values for ''k''<sub>i</sub> are highly uncertain but that it doesn't influence the radius by a significant amount.}} '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 16:35, 1 July 2026 (UTC)
:::::::I just checked the paper's author's other work and he appears to be a pseudoscientist who thinks that stellar-mass black holes somehow don't exist, so I wouldn't trust that formula. His works, including the one I mentioned, were published in viXra, which is for research that generally wouldn't be publishable elsewhere. '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 16:55, 1 July 2026 (UTC)
:::::::I will also mention that you can't calculate the radius of a baryon based on simple quantum harmonic oscillators. It doesn't even consider relativistic effects or additional effects due to the strong force, which are very significant in such environments. I unfortunately fell for it as my knowledge of quantum mechanics is currently quite limited. (Can you also please take that into account when asking these types of questions) '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 17:39, 1 July 2026 (UTC)
:::::::This should have been obvious to me before, but accurately calculating it based on lattice QCD requires supercomputer simulations. I can give you some radii from literature here though:
:::::::{| class="wikitable sortable"
|+veiny ahh dih
! Symbol
! Radius (fm)
! Quantity
|-
|p
|{{val|0.84075|0.00064}} https://physics.nist.gov/cgi-bin/cuu/Value?rp ↗
|Charge
|-
|n
|{{val|0.864|0.009|0.008}} https://pdg.lbl.gov/2026/listings/rpp2026-list-n.pdf ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Lambda0}}}}
|{{val|0.681|0.002}} https://arxiv.org/pdf/2208.14802 ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Charmed Lambda+}}}}
|0.78 https://arxiv.org/pdf/1712.00730 ↗
|Charge
|-
|{{math|{{SubatomicParticle|Sigma+}}}}
|{{val|0.81|0.03|0.03}} https://arxiv.org/pdf/1401.5862 ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Sigma-}}}}
|{{val|0.78|0.07|0.08}} https://arxiv.org/pdf/hep-ex/0106053 ↗, {{val|1.02|0.03|0.04}} https://arxiv.org/pdf/1401.5862 ↗
|Charge, Magnetic moment
|-
|{{math|{{SubatomicParticle|Charmed Sigma++}}}}
|{{val|0.484|0.037|0.040}}, {{val|0.834|0.087|0.097}} https://arxiv.org/pdf/1310.5915 ↗
|Charge, Magnetic moment
|-
|{{math|{{SubatomicParticle|Charmed Sigma0}}}}
|{{val|0.806|0.075|0.082}} https://arxiv.org/pdf/1310.5915 ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Xi0}}}}
|{{val|0.73|0.03|0.04}} https://arxiv.org/pdf/1401.5862 ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Xi-}}}}
|{{val|0.66|0.04|0.04}} https://arxiv.org/pdf/1401.5862 ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Double Charmed Xi++}}}}
|{{val|0.377|0.012|0.012}} https://arxiv.org/pdf/1310.5915 ↗
|Charge
|-
|{{math|{{SubatomicParticle|Double Charmed Xi+}}}}
|{{val|0.375|0.016|0.016}} https://arxiv.org/pdf/1310.5915 ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Charmed Omega0}}}}
|{{val|0.595|0.044|0.047}} https://arxiv.org/pdf/1310.5915 ↗
|Magnetic moment
|-
|{{math|{{SubatomicParticle|Double Charmed Omega+}}}}
|{{val|0.207|0.025|0.028}}, {{val|0.385|0.025|0.028}} https://arxiv.org/pdf/1310.5915 ↗
|Charge, Magnetic moment
|-
|{{math|{{SubatomicParticle|Delta++}}}}
|1.048https://inspirehep.net/files/2c7d3fa511e61f93c7a5590f64243ecd ↗
|Charge
|-
|{{math|{{SubatomicParticle|Omega-}}}}
|{{val|0.590|0.043|0.046}}, {{val|0.567|0.014|0.014}} https://arxiv.org/pdf/1006.0558 ↗
|Charge, Magnetic moment
|-
|{{math|{{SubatomicParticle|Pion+-}}}}
|{{val|0.659|0.004}} https://academic.oup.com/ptep/article/2020/8/083C01/5891211 ↗
|Charge
|-
|{{math|{{SubatomicParticle|Pion0}}}}
|{{val|0.52|0.02}} https://arxiv.org/pdf/2410.17570 ↗
|Mass
|-
|{{math|{{SubatomicParticle|Eta}}}}
|{{val|0.68|0.02}} https://arxiv.org/pdf/1203.5756 ↗
|Charge
|-
|{{math|{{SubatomicParticle|Charmed Eta}}}}
|{{val|0.25|0.00|0.00}} https://arxiv.org/pdf/nucl-th/0612069 ↗
|Charge
|-
|{{math|{{SubatomicParticle|Kaon+-}}}}
|{{val|0.5747|0.0024}} https://arxiv.org/pdf/1203.5756 ↗
|Charge
|-
|{{math|{{SubatomicParticle|D+}}}}
|0.510 https://www.mccollege.edu.in/upload/faculty/1670260173.pdf ↗
|Charge
|-
|{{math|{{SubatomicParticle|Strange D+}}}}
|0.465 https://www.mccollege.edu.in/upload/faculty/1670260173.pdf ↗
|Charge
|-
|{{math|{{SubatomicParticle|B+}}}}
|0.732 https://www.mccollege.edu.in/upload/faculty/1670260173.pdf ↗
|Charge
|-
|{{math|{{SubatomicParticle|Rho+}}}}
|{{val|0.75|0.03|0.03}}, {{val|0.72|0.03|0.04}} https://www.mccollege.edu.in/upload/faculty/1670260173.pdf ↗
|Charge, Colour charge
|-
|{{math|{{SubatomicParticle|J/Psi}}}}
|{{val|0.26|0.00|0.00}} https://arxiv.org/pdf/nucl-th/0612069 ↗
|Charge
|-
|{{math|{{SubatomicParticle|Kaon*+}}}}
|0.66 https://arxiv.org/pdf/nucl-th/0612069 ↗
|Charge
|} '''<span style="font-family:arial;background-color:white;padding:2px 3px 2px 3px"><span style="color:#1c3587">SpaceImplorer</span><span style="color:#1c877c">ExplorerImplorer</span></span>''' 20:28, 1 July 2026 (UTC)