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	<title>Tensegrity - Revision history</title>
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	<updated>2026-05-29T17:43:02Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<title>en&gt;Monkbot: /* Bibliography */Task 6h: add |script-title=; replace {{xx icon}} with |language= in CS1 citations; clean up language icons;</title>
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		<updated>2014-11-19T13:59:11Z</updated>

		<summary type="html">&lt;p&gt;&lt;span class=&quot;autocomment&quot;&gt;Bibliography: &lt;/span&gt;&lt;a href=&quot;/index.php?title=User:Monkbot/Task_6:_CS1_language_support&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;User:Monkbot/Task 6: CS1 language support (page does not exist)&quot;&gt;Task 6h&lt;/a&gt;: add |script-title=; replace {{xx icon}} with |language= in CS1 citations; clean up language icons;&lt;/p&gt;
&lt;a href=&quot;https://en.formulasearchengine.com/index.php?title=Tensegrity&amp;amp;diff=285740&amp;amp;oldid=2146&quot;&gt;Show changes&lt;/a&gt;</summary>
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	<entry>
		<id>https://en.formulasearchengine.com/index.php?title=Tensegrity&amp;diff=2146&amp;oldid=prev</id>
		<title>en&gt;Rjwilmsi: Journal cites, added 1 DOI using AWB (9904)</title>
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		<updated>2014-02-03T19:50:26Z</updated>

		<summary type="html">&lt;p&gt;Journal cites, added 1 DOI using &lt;a href=&quot;/index.php?title=Testwiki:AWB&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;Testwiki:AWB (page does not exist)&quot;&gt;AWB&lt;/a&gt; (9904)&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Starbox begin&lt;br /&gt;
 | name = Alpha Herculis&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox image &lt;br /&gt;
 | image = [[File:Hercules Historical View.png|250px]]&lt;br /&gt;
 | caption = Historical view of the [[Hercules (constellation)|Hercules]] constellation showing Rasalgethi as the &amp;#039;&amp;#039;&amp;#039;α&amp;#039;&amp;#039;&amp;#039; star and &amp;quot;Head of the Kneeler&amp;quot;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox observe&lt;br /&gt;
 | epoch    = J2000&lt;br /&gt;
 | ra       = {{RA|17|14|38.80}}&amp;lt;ref name=aaa323_L49/&amp;gt;&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;SIMBAD&amp;quot;/&amp;gt;&lt;br /&gt;
 | dec      = {{DEC| +14|23|25.0}}&amp;lt;ref name=aaa323_L49/&amp;gt;&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;SIMBAD&amp;quot;/&amp;gt;&lt;br /&gt;
 | appmag_v = 2.9137 / 5.4&amp;lt;ref name=aaa323_L49/&amp;gt;&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;/&amp;gt;&lt;br /&gt;
 | constell = [[Hercules (constellation)|Hercules]]&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox character&lt;br /&gt;
 | class    = M5IIvar / (G5III+F2V)&lt;br /&gt;
 | b-v      = 1.45&amp;lt;ref name=&amp;quot;JOHNSON&amp;quot;/&amp;gt;&lt;br /&gt;
 | u-b      = 1.01&amp;lt;ref name=&amp;quot;JOHNSON&amp;quot;/&amp;gt;&lt;br /&gt;
 | variable = Semiregular&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox astrometry&lt;br /&gt;
 | prop_mo_ra  = -6.71&amp;lt;ref name=aaa323_L49/&amp;gt;&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;SIMBAD&amp;quot;/&amp;gt;&lt;br /&gt;
 | prop_mo_dec = 32.78&amp;lt;ref name=aaa323_L49/&amp;gt;&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;/&amp;gt;&amp;lt;ref name=&amp;quot;SIMBAD&amp;quot;/&amp;gt;&lt;br /&gt;
 | parallax = 9.07&lt;br /&gt;
 | p_error  = 1.32&lt;br /&gt;
 | parallax_footnote = &amp;lt;ref name=aaa323_L49/&amp;gt;&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;/&amp;gt;&lt;br /&gt;
 |absmag_v  = -2.30&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox detail &lt;br /&gt;
 | mass   = {{nowrap|2.15 ± 0.22}}&amp;lt;ref name=aaa465_2_593/&amp;gt;&lt;br /&gt;
 | radius = 387&amp;lt;ref name=aaa465_2_593/&amp;gt;&lt;br /&gt;
 | luminosity = 8,300&amp;lt;ref name=aaa465_2_593/&amp;gt;&lt;br /&gt;
 | temperature = 2,800&amp;lt;ref name=aaa465_2_593/&amp;gt;&lt;br /&gt;
 | metal  = &lt;br /&gt;
 | gravity = {{nowrap|−0.41 ± 0.19}}&amp;lt;ref name=aaa465_2_593/&amp;gt;&lt;br /&gt;
 | rotational_velocity = &lt;br /&gt;
 | age    = &lt;br /&gt;
}}&lt;br /&gt;
{{Starbox catalog&lt;br /&gt;
 |names=Ras Algethi, Rasalgethi, [[Bayer designation|α Her]], [[Flamsteed designation|64&amp;amp;nbsp;Her]], [[Harvard Revised catalogue|HR]]&amp;amp;nbsp;6406, [[Bonner Durchmusterung|BD]]&amp;amp;nbsp;+14° 3207, [[Henry Draper Catalogue|HD]]&amp;amp;nbsp;156014J, [[Hipparcos catalogue|HIP]]&amp;amp;nbsp;84345, [[Smithsonian Astrophysical Observatory Star Catalog|SAO]]&amp;amp;nbsp;102680, [[Catalog of Components of Double and Multiple Stars|CCDM]]&amp;amp;nbsp;J17146+1424AB, [[American Association of Variable Star Observers|AAVSO]]&amp;amp;nbsp;1710+14&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox reference&lt;br /&gt;
 | Simbad=HD+156014J&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox end}}&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Alpha Herculis&amp;#039;&amp;#039;&amp;#039; (α Her, α Herculis) is a multiple [[star system]] in the [[constellation]] [[Hercules (constellation)|Hercules]].  It has the traditional name &amp;#039;&amp;#039;&amp;#039;Rasalgethi&amp;#039;&amp;#039;&amp;#039; or &amp;#039;&amp;#039;&amp;#039;Ras Algethi&amp;#039;&amp;#039;&amp;#039; ({{lang-ar|رأس الجاثي ra&amp;#039;s al-jaθiyy}} &amp;#039;&amp;#039;Head of the Kneeler&amp;#039;&amp;#039;), and the [[Flamsteed designation]] &amp;#039;&amp;#039;&amp;#039;64 Herculis&amp;#039;&amp;#039;&amp;#039;.&amp;lt;ref name=&amp;quot;BBC1&amp;quot;&amp;gt;{{cite web&lt;br /&gt;
  |title=Constellations: Hercules &amp;#039;the Strongman&amp;#039;&lt;br /&gt;
  |publisher=The BBC (British Broadcasting Corporation)&lt;br /&gt;
  |author=Kurt Vonnegut&lt;br /&gt;
  |url=http://www.bbc.co.uk/dna/h2g2/A29778916&lt;br /&gt;
  |accessdate=2010-11-14}}&amp;lt;/ref&amp;gt;  The traditional name &amp;quot;Head&amp;quot; comes from the fact that in antiquity Hercules was depicted upside down on the constellation maps.&lt;br /&gt;
&lt;br /&gt;
The term &amp;#039;&amp;#039;ra&amp;#039;s al-jaθiyy&amp;#039;&amp;#039; or &amp;#039;&amp;#039;&amp;#039;Ras al Djathi&amp;#039;&amp;#039;&amp;#039; was appeared in the catalogue of stars in the &amp;#039;&amp;#039;Calendarium&amp;#039;&amp;#039; of [[Al Achsasi al Mouakket]], which was translated into [[Latin]] as &amp;#039;&amp;#039;&amp;#039;Caput Ingeniculi&amp;#039;&amp;#039;&amp;#039;.&amp;lt;ref&amp;gt;{{cite journal&lt;br /&gt;
 | last=Knobel | first=E. B.&lt;br /&gt;
 | title=Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket&lt;br /&gt;
 | journal=Monthly Notices of the Royal Astronomical Society&lt;br /&gt;
 | volume=55 | page=429 |date=June 1895&lt;br /&gt;
 | bibcode=1895MNRAS..55..429K }}&amp;lt;/ref&amp;gt; &lt;br /&gt;
&lt;br /&gt;
In [[Chinese astronomy]], Rasalgethi is called 帝座, [[Pinyin]]: Dìzuò, meaning &amp;#039;&amp;#039;	Emperor&amp;#039;s Seat&amp;#039;&amp;#039;, because this star is marking itself and stand alone in &amp;#039;&amp;#039;Emperor&amp;#039;s Seat&amp;#039;&amp;#039; asterism, [[Heavenly Market enclosure]] (see : [[Chinese constellation]]).&amp;lt;ref&amp;gt;{{zh icon}} [http://aeea.nmns.edu.tw/2006/0606/ap060625.html AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 25 日]&amp;lt;/ref&amp;gt; 帝座 (Dìzuò) was westernized into &amp;#039;&amp;#039;&amp;#039;Ti Tso&amp;#039;&amp;#039;&amp;#039; by R.H. Allen, with the same meaning &amp;lt;ref&amp;gt;[http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Hercules*.html Richard Hinckley Allen: Star Names — Their Lore and Meaning: Hercules]&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Properties ==&lt;br /&gt;
The angular diameter of the red giant, α&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; Her, has been measured with an [[interferometer]] as&lt;br /&gt;
34&amp;amp;nbsp;±&amp;amp;nbsp;0.8 [[arcsecond|mas]], or 0.034&amp;amp;nbsp;arcseconds.&amp;lt;ref name=&amp;quot;BENSON&amp;quot;&amp;gt;{{cite journal &lt;br /&gt;
 | author=Benson, J. A.; Dyck, H. M.; Mason, W. L.; Howell, R. R.; Ridgway, S. T.; Dixon, D. J. &lt;br /&gt;
 | title=The infrared angular diameter of Alpha Herculis measured with a Michelson interferometer  &lt;br /&gt;
 | journal=Astronomical Journal &lt;br /&gt;
 |date=December 1991&lt;br /&gt;
 | volume=102 &lt;br /&gt;
 | pages=2091–2097&lt;br /&gt;
 | doi= 10.1086/116033&lt;br /&gt;
 | bibcode=1991AJ....102.2091B }}&amp;lt;/ref&amp;gt; At an estimated distance of 110 [[parsec]]s from [[Hipparcos]],&amp;lt;ref name=aaa323_L49/&amp;gt;&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;/&amp;gt;&amp;lt;ref name=GSM/&amp;gt; this corresponds to a radius of about 280 million kilometers (or 170 million miles), which is roughly 400[[Solar radius|R&amp;lt;sub&amp;gt;☉&amp;lt;/sub&amp;gt;]] or 1.87 [[astronomical unit|AU]].&amp;lt;ref name=&amp;quot;NOTERADIUS&amp;quot; group=&amp;quot;note&amp;quot;&amp;gt;To determine the Rasalgheti&amp;#039;s radius in terms of solar units, the calculations begin with the formula for [[angular diameter]] as follows:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{smallmatrix} {\delta} = \frac{d_R}{D_R}\end{smallmatrix}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039;δ&amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039; equals Rasalgheti&amp;#039;s angular diameter in [[arcseconds]], &amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039;d&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039; the star&amp;#039;s &amp;#039;&amp;#039;&amp;#039;d&amp;#039;&amp;#039;&amp;#039;iameter in [[Astronomical Unit|AU]], and &amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039;D&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039;  the &amp;#039;&amp;#039;&amp;#039;D&amp;#039;&amp;#039;&amp;#039;istance from Earth in parsecs.  If we know the angular diameter and the Distance, then we can solve for &amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039;d&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;#039;&amp;#039;&amp;#039;&amp;#039;&amp;#039; as follows:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{smallmatrix}d_R = \delta \cdot D_R = {0.034} \cdot 110.0 = 3.740 AU \end{smallmatrix}&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
To obtain Rasalgheti&amp;#039;s  radius:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{smallmatrix}R_R = {\left ( {\frac {d_R}{2}} \right )} = {\left ( {\frac {3.740}{2}} \right )} = 1.870 AU \end{smallmatrix}&amp;lt;/math&amp;gt;.&lt;br /&gt;
Converting into Solar units, 1 [[Astronomical Unit|AU]] = 149,597,871&amp;amp;nbsp;km and the mean radius of the [[Sun]] = 696,000&amp;amp;nbsp;km, hence the calculation:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\begin{smallmatrix}d_B = {\left ( 1.87 AU \right )} {\left ( {\frac {149,597,871 km}{696,000 km}} \right )} = 280,000,000 km = 402 R_{\odot} \end{smallmatrix}&amp;lt;/math&amp;gt; (rounded).&amp;lt;/ref&amp;gt; If Rasalgheti were at the center of our [[Solar System]] its radius would extend past the orbit of [[Mars]] at 1.5 [[astronomical unit|AU]] but not quite as far as the [[asteroid belt]].  The red giant is estimated to have started its life with about 7-8 [[solar mass]]es.&amp;lt;ref name=&amp;quot;KALER&amp;quot;/&amp;gt;  Like most [[Stellar classification#Class M|type M]] stars near the end of their lives, Rasalgethi is experiencing a high degree of [[stellar mass loss]] creating a sparse, gaseous envelope that extends at least 90 [[astronomical unit]]s.&amp;lt;ref&amp;gt;{{cite journal&lt;br /&gt;
  | last=Deutsch &lt;br /&gt;
  | first=Armin J. &lt;br /&gt;
  | title=The Circumstellar Envelope of Alpha Herculis&lt;br /&gt;
  | journal=Astrophysical Journal &lt;br /&gt;
  |date=March 1956&lt;br /&gt;
  | volume=123 &lt;br /&gt;
  | pages=210–227&lt;br /&gt;
  | doi=10.1086/146152&lt;br /&gt;
  | bibcode=1956ApJ...123..210D}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Star system ==&lt;br /&gt;
When viewed through a telescope, this system is resolved into two components designated α&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; and α&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;. These two components are more than 500 [[astronomical units]] apart, with an estimated orbital period of approximately 3600 years. α&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt; is a relatively massive red [[bright giant]]. α&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; is actually a [[double star]] system with a primary yellow giant star and a secondary, yellow-white dwarf star. (These components are sometimes designated α Herculis A, Ba and Bb, respectively.)&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
*[[List of largest known stars]]&lt;br /&gt;
*[[Lists of stars]] in the constellation [[List of stars in Hercules|Hercules]]&lt;br /&gt;
*[[Betelgeuse#Circumstellar dynamics|Betelgeuse mass loss]]&lt;br /&gt;
*[[Stellar classification#Spectral types|Spectral types F, G &amp;amp; M]]&lt;br /&gt;
&lt;br /&gt;
== Notes ==&lt;br /&gt;
&amp;lt;references group=&amp;quot;note&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
{{reflist|refs=&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=aaa465_2_593&amp;gt;{{citation | last1=Schröder | first1=K.-P. | last2=Cuntz | first2=M. | title=A critical test of empirical mass loss formulas applied to individual giants and supergiants | journal=Astronomy and Astrophysics | volume=465 | issue=2 | pages=593–601 |date=April 2007 | doi=10.1051/0004-6361:20066633 | bibcode=2007A&amp;amp;A...465..593S |arxiv = astro-ph/0702172 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;KALER&amp;quot;&amp;gt;{{cite web | title=RASALGETHI (Alpha Herculis) | publisher=University of Illinois | first1=James B. | last1=Kaler | url=http://stars.astro.illinois.edu/sow/rasalgethi.html | accessdate=2007-03-07 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;JOHNSON&amp;quot;&amp;gt;{{cite journal | last1=Johnson | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewski | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Comm. Lunar Plan. Lab. | volume=4 | pages=99 | year=1966 | bibcode=1966CoLPL...4...99J }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;SIMBAD&amp;quot;&amp;gt;{{cite web | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=alpha+her&amp;amp;NbIdent=1&amp;amp;Radius=2&amp;amp;Radius.unit=arcmin&amp;amp;submit=submit+id | title =SIMBAD query result:NAME RASALGETHI -- Semi-regular pulsating Star | publisher =Centre de Données astronomiques de Strasbourg | accessdate = 2010-09-26 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=aaa323_L49&amp;gt;{{citation | last1=Perryman | first1=M. A. C. | last2=Lindegren | first2=L. | last3=Kovalevsky | first3=J. |  last4=et al. | title=The Hipparcos Catalogue | journal=Astronomy and Astrophysics | volume=323 |date=July 1997 | pages=L49–L52 | bibcode=1997A&amp;amp;A...323L..49P}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;LEEUWEN&amp;quot;&amp;gt;{{cite journal | title=Hipparcos, the New Reduction | last1=van Leeuwen | first1=F |date=November 2007 | publisher=[[Centre de Données astronomiques de Strasbourg]] | pages=653 | issue=2 | volume=474 | doi=10.1051/0004-6361:20078357 | journal=Astronomy and Astrophysics | bibcode=2007A&amp;amp;A...474..653V |arxiv = 0708.1752 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=GSM&amp;gt;{{citation | last=Perryman | first=Michael | title=The Making of History&amp;#039;s Greatest Star Map | location=Heidelberg | publisher=Springer-Verlag | year=2010 | doi=10.1007/978-3-642-11602-5}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
*An Atlas of the Universe: [http://www.atlasoftheuniverse.com/orbits.html Multiple Star Orbits]&lt;br /&gt;
*Upside down Hercules showing Rasalgethi as the head: [http://www.ne.jp/asahi/stellar/scenes/seiza_e/her.htm Hercules]&lt;br /&gt;
&lt;br /&gt;
{{Sky|17|14|38.858|+|14|23|25.20|1000000}}&lt;br /&gt;
{{Stars of Hercules}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Double stars]]&lt;br /&gt;
[[Category:Hercules (constellation)]]&lt;br /&gt;
[[Category:Bayer objects|Herculis, Alpha]]&lt;br /&gt;
[[Category:Flamsteed objects|Herculis, 64]]&lt;br /&gt;
[[Category:Triple star systems]]&lt;br /&gt;
[[Category:Stars with proper names]]&lt;br /&gt;
[[Category:M-type bright giants]]&lt;br /&gt;
[[Category:G-type giants]]&lt;br /&gt;
[[Category:F-type main-sequence stars]]&lt;br /&gt;
[[Category:Objects within 1000 ly of Earth]]&lt;/div&gt;</summary>
		<author><name>en&gt;Rjwilmsi</name></author>
	</entry>
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