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		<title>&gt;Loooke: /* Parameter documentation */ name isn&#039;t required (it defaults to the page title)</title>
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		<updated>2025-03-04T01:49:42Z</updated>

		<summary type="html">&lt;p&gt;&lt;span class=&quot;autocomment&quot;&gt;Parameter documentation: &lt;/span&gt; name isn&amp;#039;t required (it defaults to the page title)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Documentation subpage}}&lt;br /&gt;
&amp;lt;!-- PLEASE ADD CATEGORIES AND INTERWIKIS AT THE BOTTOM OF THIS PAGE --&amp;gt;&lt;br /&gt;
Infobox for articles on [[globular cluster]]s.&lt;br /&gt;
&lt;br /&gt;
==Usage==&lt;br /&gt;
Fields should generally be directly from the source, such as [[SIMBAD]].  Wikilinks and expansion of abbreviations are acceptable.&lt;br /&gt;
&lt;br /&gt;
===Example infobox===&lt;br /&gt;
{{Infobox globular cluster&lt;br /&gt;
| name = {{{name}}}&lt;br /&gt;
| image = {{{image}}}&lt;br /&gt;
| caption = {{{caption}}}&lt;br /&gt;
| credit = {{{credit}}}&lt;br /&gt;
| epoch = {{{epoch}}}&lt;br /&gt;
| class = {{{class}}}&lt;br /&gt;
| constellation = {{{constellation}}}&lt;br /&gt;
| ra = {{{ra}}}&lt;br /&gt;
| dec = {{{dec}}}&lt;br /&gt;
| dist_ly = {{{dist_ly}}}&lt;br /&gt;
| dist_pc = {{{dist_pc}}}&lt;br /&gt;
| appmag_v = {{{appmag_v}}}&lt;br /&gt;
| size_v = {{{size_v}}}&lt;br /&gt;
| absmag_v = {{{absmag_v}}}&lt;br /&gt;
| mass_msol = {{{mass_msol}}}&lt;br /&gt;
| mass_kg = {{{mass_kg}}}&lt;br /&gt;
| radius_arcminsec = {{{radius_arcminsec}}}&lt;br /&gt;
| radius_ly = {{{radius_ly}}}&lt;br /&gt;
| radius_pc = {{{radius_pc}}}&lt;br /&gt;
| radius_tidal_arcminsec = {{{radius_tidal_arcminsec}}}&lt;br /&gt;
| radius_tidal_ly = {{{radius_tidal_ly}}}&lt;br /&gt;
| radius_tidal_pc = {{{radius_tidal_pc}}}&lt;br /&gt;
| v_hb = {{{v_hb}}}&lt;br /&gt;
| metal_fe = {{{metal_fe}}}&lt;br /&gt;
| metal_z = {{{metal_z}}}&lt;br /&gt;
| age = {{{age}}}&lt;br /&gt;
| notes = {{{notes}}}&lt;br /&gt;
| names = {{{names}}}&lt;br /&gt;
}}&lt;br /&gt;
The following parameters can be used to create a globular cluster infobox. Please remove any parameters that are not likely to be useful.&lt;br /&gt;
&amp;lt;syntaxhighlight lang=&amp;quot;wikitext&amp;quot; style=&amp;quot;overflow:auto&amp;quot;&amp;gt;{{Infobox globular cluster&lt;br /&gt;
| name =&lt;br /&gt;
| image =&lt;br /&gt;
| caption =&lt;br /&gt;
| credit =&lt;br /&gt;
| epoch = &lt;br /&gt;
| class =&lt;br /&gt;
| constellation =&lt;br /&gt;
| ra = &lt;br /&gt;
| dec = &lt;br /&gt;
| dist_ly = &lt;br /&gt;
| dist_pc =&lt;br /&gt;
| appmag_v =&lt;br /&gt;
| size_v =&lt;br /&gt;
| absmag_v=&lt;br /&gt;
| mass_msol =&lt;br /&gt;
| mass_kg =&lt;br /&gt;
| radius_arcminsec =&lt;br /&gt;
| radius_ly =&lt;br /&gt;
| radius_pc =&lt;br /&gt;
| radius_tidal_arcminsec =&lt;br /&gt;
| radius_tidal_ly =&lt;br /&gt;
| radius_tidal_pc =&lt;br /&gt;
| v_hb =&lt;br /&gt;
| metal_fe = &lt;br /&gt;
| metal_z = &lt;br /&gt;
| age = &lt;br /&gt;
| notes =&lt;br /&gt;
| names =&lt;br /&gt;
}}&amp;lt;/syntaxhighlight&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Parameter documentation ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;font-size:90%; margin:auto; width:100%;&amp;quot;&lt;br /&gt;
! Field &lt;br /&gt;
! Description&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;name&amp;#039;&amp;#039;&lt;br /&gt;
| Common name of the globular cluster. If not specified, defaults to the page title.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;image&amp;#039;&amp;#039;&lt;br /&gt;
| Photograph of the cluster. Preferably this should be a wide shot to show most/all of the globular cluster rather than a view from within it. Include the &amp;quot;File:&amp;quot; prefix and a width of 300px. If uploading a new image, please put them on [[Wikimedia Commons|Commons]] so they can be easily used by the other language Wikipedias.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;caption&amp;#039;&amp;#039;&lt;br /&gt;
| Description of the photograph in the &amp;#039;&amp;#039;image&amp;#039;&amp;#039; field.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;credit&amp;#039;&amp;#039;&lt;br /&gt;
| Per [[MOS:CREDITS]], credits for the image in the infobox are discouraged since the infobox should only contain key facts of the article&amp;#039;s subject.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;epoch&amp;#039;&amp;#039;&lt;br /&gt;
| The [[astronomical epoch]] of the cluster coordinates (below). Normally this is &amp;lt;nowiki&amp;gt;[[J2000]]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;class&amp;#039;&amp;#039;&lt;br /&gt;
| The [[Shapley–Sawyer Concentration Class]] of the cluster.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;constellation&amp;#039;&amp;#039;&lt;br /&gt;
| A link to the [[constellation]] where this cluster is located.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;ra&amp;#039;&amp;#039;&lt;br /&gt;
| The [[right ascension]] coordinate of the cluster midpoint. The {{tl|RA}} or {{tl|Deg2HMS}} templates should be used here. For example: {{tlx|RA|hh|mm|ss.dd}} or {{tlx|Deg2HMS|dd.ddd|sup{{=}}yes}}.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;dec&amp;#039;&amp;#039;&lt;br /&gt;
| The [[declination]] coordinate of the cluster midpoint. The {{tl|DEC}} template should be used here. For example: {{tlx|DEC|±dd|mm|ss.d}}.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;dist_ly&amp;#039;&amp;#039;&lt;br /&gt;
| This is an estimate of the cluster&amp;#039;s distance from the Solar System in [[light year]]s. The distances can be combined into a single field as: {{tlx|Convert|d.dd|kly|kpc|abbr&amp;amp;#61;off|lk&amp;amp;#61;on|sigfig&amp;amp;#61;1}}.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;dist_pc&amp;#039;&amp;#039;&lt;br /&gt;
| This should be the same distance as dist_ly using [[parsec]] as the units. A parsec is equal to 3.2616 light years.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;appmag_v&amp;#039;&amp;#039;&lt;br /&gt;
| The [[apparent magnitude]] of the cluster.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;size_v&amp;#039;&amp;#039;&lt;br /&gt;
| This gives the angular diameter, usually in [[arc minute]]s or [[arc second]]s.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;absmag_v&amp;#039;&amp;#039;&lt;br /&gt;
| This gives the V-band absolute magnitude.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;mass_msol&amp;#039;&amp;#039;&lt;br /&gt;
| The estimated total mass in [[solar mass]]es.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;mass_kg&amp;#039;&amp;#039;&lt;br /&gt;
| The same value as above, using kilograms as units. A solar mass is equal to {{nowrap|2 × 10&amp;lt;sup&amp;gt;30&amp;lt;/sup&amp;gt; kg}}.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;radius_arcminsec&amp;#039;&amp;#039;&lt;br /&gt;
| The [[subtended angle|angle subtended]] by the radius, in [[arcminute]]s or [[arcseconds]].&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;radius_ly&amp;#039;&amp;#039;&lt;br /&gt;
| The ly and pc radii can be combined into a single field as: {{tlx|Convert|d.dd|ly|pc|abbr&amp;amp;#61;on|lk&amp;amp;#61;on|sigfig&amp;amp;#61;1}}.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;radius_pc&amp;#039;&amp;#039;&lt;br /&gt;
| This should be the same distance as &amp;#039;&amp;#039;radius_ly&amp;#039;&amp;#039; using [[parsec]] as the units. A parsec is equal to 3.2616 light years.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;radius_tidal_arcminsec&amp;#039;&amp;#039;&lt;br /&gt;
| The [[subtended angle|angle subtended]] by the tidal radius, in [[arcminute]]s or [[arcseconds]] (specify).&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;radius_tidal_ly&amp;#039;&amp;#039;&lt;br /&gt;
|This is the [[Roche limit]] of the cluster, beyond which stars and material are effectively removed from the cluster. Typically given as either the instantaneous value or an average of its [[perigalactic]] and [[apogalactic]] values.&amp;lt;br&amp;gt;&lt;br /&gt;
The ly and pc radii can be combined into a single field as: {{tlx|Convert|d.dd|ly|pc|abbr&amp;amp;#61;on|lk&amp;amp;#61;on|sigfig&amp;amp;#61;1}}.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;radius_tidal_pc&amp;#039;&amp;#039;&lt;br /&gt;
| This should be the same distance as &amp;#039;&amp;#039;radius_tidal_ly&amp;#039;&amp;#039; using [[parsec]] as the units. A parsec is equal to 3.2616 light years.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;v_hb&amp;#039;&amp;#039;&lt;br /&gt;
| The visual magnitude of the [[horizontal branch]] stars in the cluster.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;metal_fe&amp;#039;&amp;#039;&lt;br /&gt;
| The [[metallicity]] as a logarithmic abundance of [[iron]] relative to [[hydrogen]], as compared to the Sun.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;metal_z&amp;#039;&amp;#039;&lt;br /&gt;
| The [[metallicity]] as a logarithmic abundance of elements other than [[hydrogen]] and [[helium]], relative to hydrogen, as compared to the Sun.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;age&amp;#039;&amp;#039;&lt;br /&gt;
| The estimated age of the cluster, usually listed in &amp;lt;nowiki&amp;gt;[[Gigayear|Gyr]]&amp;lt;/nowiki&amp;gt; (billions of years).&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;notes&amp;#039;&amp;#039;&lt;br /&gt;
| Additional details of significance.&lt;br /&gt;
|-&lt;br /&gt;
|&amp;#039;&amp;#039;names&amp;#039;&amp;#039;&lt;br /&gt;
| A comma separated list of used alternative cluster names. These are names that are commonly used in scholarly journal articles, such as the [[New General Catalogue]] (NGC) name.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
* {{tl|Cite journal}}&lt;br /&gt;
* {{tl|Cite web}}&lt;br /&gt;
* {{tl|Infobox galaxy}}&lt;br /&gt;
* {{tl|Infobox cluster}}&lt;br /&gt;
&lt;br /&gt;
&amp;lt;includeonly&amp;gt;{{basepage subpage|&lt;br /&gt;
&amp;lt;!-- CATEGORIES HERE, THANKS --&amp;gt;&lt;br /&gt;
[[Category:Astronomy infobox templates|Globular cluster]]&lt;br /&gt;
}}&amp;lt;/includeonly&amp;gt;&lt;/div&gt;</summary>
		<author><name>&gt;Loooke</name></author>
	</entry>
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