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#REDIRECT [[Sun]] |
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{{Template for discussion/dated|page=Sun|link=Wikipedia:Templates for discussion/Log/2014 June 26#Template:Sun|type=inline|help=off}} |
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{| class="infobox" style="width: 20em;" |
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|+ style="font-size:larger;" | '''The Sun''' [[Image:Sun symbol.svg|25px]] |
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| colspan="2" style="text-align:center; background: #000000;" | [[File:The_Sun_by_the_Atmospheric_Imaging_Assembly_of_NASA's_Solar_Dynamics_Observatory_-_20100819.jpg|290px]] |
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! bgcolor="#FCC857" colspan="2" align=center | '''Observation data''' |
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| Mean distance<br/><small>from [[Earth]]</small> |
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| {{val|1.496|e=8|u=km}}<br/><small>8 min 19 s at [[speed of light|light speed]]</small> |
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|- |
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| [[Apparent magnitude|Visual brightness]] (''V'') |
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| −26.74<ref name=nssdc> |
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{{cite web |
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|last=Williams |first=D. R. |
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|date=1 July 2013 |
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|title=Sun Fact Sheet |
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|url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html |
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|publisher=[[NASA]] |
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|accessdate=2013-08-12 |
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}}</ref> |
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|- |
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| [[Absolute magnitude]] |
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| 4.83<ref name=nssdc /> |
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|- |
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| [[Spectral classification]] |
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| G2V |
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|- |
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| [[Metallicity]] |
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| ''Z'' = 0.0122<ref> |
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{{cite journal |
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|last1=Asplund |first1=M. |
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|last2=Grevesse |first2=N. |
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|last3=Sauval |first3=A. J. |
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|year=2006 |
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|title=The new solar abundances - Part I: the observations |
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|journal=[[Communications in Asteroseismology]] |
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|volume=147 |pages=76–79 |
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|bibcode=2006CoAst.147...76A |
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|doi=10.1553/cia147s76 |
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}}</ref> |
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|- |
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| [[Angular size]] |
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| 31.6–32.7′<ref> |
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{{cite web |
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|title=Eclipse 99: Frequently Asked Questions |
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|url=http://education.gsfc.nasa.gov/eclipse/pages/faq.html |
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|publisher=[[NASA]] |
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|accessdate=2010-10-24 |
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}}</ref> |
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|- |
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| Adjectives |
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| Solar |
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! bgcolor="#FCC857" colspan="2" align=center | '''[[Orbit]]al characteristics''' |
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| Mean distance<br/><small>from [[Milky Way]] core</small> |
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| ≈ {{val|2.7|e=17|u=km}}<br/><small>{{val|27200|u=[[light-year]]s}}</small> |
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|- |
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| [[Galaxy|Galactic]] period |
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| (2.25–2.50){{e|8}} [[julian year (astronomy)|a]] (years) |
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|- |
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| [[Velocity]] |
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| ≈ {{val|220|u=km/s}} <small>(orbit around the center of the Galaxy)</small> <br />≈ {{val|20|u=km/s}} <small>(relative to average velocity of other stars in stellar neighborhood)</small> <br />≈ {{val|370|u=km/s}}<ref> |
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{{cite journal |
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|last=Hinshaw |first=G. |
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|author2=''et al.'' |
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|year=2009 |
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|title=Five-year Wilkinson Microwave Anisotropy Probe observations: data processing, sky maps, and basic results |
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|journal=[[The Astrophysical Journal Supplement Series]] |
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|volume=180 |issue=2 |pages=225–245 |
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|arxiv=0803.0732 |
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|bibcode=2009ApJS..180..225H |
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|doi=10.1088/0067-0049/180/2/225 |
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}}</ref> <small>(relative to the [[Cosmic microwave background radiation#CMBR dipole anisotropy|cosmic microwave background]])</small> |
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|- |
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! bgcolor="#FCC857" colspan="2" align=center | '''Physical characteristics''' |
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|- |
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<!--This was not the mean diameter. | Mean diameter |
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| {{val||u=km}} |
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|- --> |
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| Equatorial [[radius]] |
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| {{val|696342|65|u=km}}<ref name=arxiv1203_4898> |
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{{cite journal |
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|last1=Emilio |first1=M. |
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|last2=Kuhn |first2=J. R. |
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|last3=Bush |first3=R. I. |
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|last4=Scholl |first4=I. F. |
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|year=2012 |
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|title=Measuring the Solar Radius from Space during the 2003 and 2006 Mercury Transits |
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|journal=[[The Astrophysical Journal]] |
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|volume=750 |issue=2 |page=135 |
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|arxiv=1203.4898 |
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|bibcode=2012ApJ...750..135E |
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|doi=10.1088/0004-637X/750/2/135 |
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}}</ref> <br/><small>109 × Earth<small/><ref name=sse/> |
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|- |
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| Equatorial [[circumference]] |
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| {{val|4.379|e=6|u=km}}<ref name=sse/><br/><small>109 × Earth<small/><ref name=sse> |
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{{cite web |
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|title=Solar System Exploration: Planets: Sun: Facts & Figures |
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|url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=Facts&System=Metric |
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|archiveurl=http://web.archive.org/web/20080102034758/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=Facts&System=Metric |
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|archivedate=2008-01-02 |
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|publisher=[[NASA]] |
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}}</ref> |
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|- |
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| [[Flattening]] |
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| {{val|9|e=-6}} |
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|- |
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| [[Surface area]] |
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| {{val|6.09|e=12|u=km2}}<ref name=sse/><br/><small>{{val|12000}} × Earth</small><ref name=sse/> |
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|- |
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| [[Volume]] |
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| {{val|1.41|e=18|u=km3}}<ref name=sse/><!-- NASA source has "1.412 x 10^18 km^3" which is 1.412 × 10^27 m^3 (basic arithmetic, also verified using the formula for volume of a sphere), but the Sun is not a sphere, and their radius is off a bit from what we have above, so we need to at least round a bit--><br/><small>{{val|1300000}} × Earth</small> |
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|- |
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| [[Mass]] |
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| {{val|1.98855|.00025|e=30|u=kg}}<ref name=nssdc/><br/><small>{{val|333000}} × Earth</small><ref name=nssdc/><!-- NASA Sun Fact Sheet states 333,000, a figure coherent with data already present in en.wiki --> |
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|- |
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| [[Density|Average density]] |
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| {{val|1.408|e=3|u=kg/m3}}<ref name=nssdc/><ref name=sse/><ref> |
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{{cite web |
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|last=Ko |first=M. |
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|year=1999 |
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|title=Density of the Sun |
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|url=http://hypertextbook.com/facts/1999/MayKo.shtml |
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|editor=Elert, G. |
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|work=The Physics Factbook |
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}}</ref><br/><small>{{val|0.255}} × Earth</small><ref name=nssdc/><ref name=sse/> |
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|- |
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| [[Density]] |
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| Center (model): {{val|1.622|e=5|u=kg/m3}}<ref name=nssdc/> |
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|- |
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| Equatorial [[surface gravity]] |
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| {{val|274.0|u=m/s2}}<ref name=nssdc/><br/>{{val|27.94|u=[[g-force|''g'']]}}<br/><small>{{val|27542.29|u=[[cgs|''cgs'']]}}<br/>28 × Earth<small/><ref name=sse/> |
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|- |
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| [[Escape velocity]]<br/><small>(from the surface)</small> |
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| {{val|617.7|u=km/s}}<ref name=sse/><br/><small>55 × Earth</small><ref name=sse/> |
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|- |
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| [[Temperature]] |
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| Center (modeled): ≈ {{val|1.57|e=7|u=K}}<ref name=nssdc/><br>Photosphere (effective): {{val|5778|ul=K}}<ref name=nssdc/><br> [[Corona]]: ≈ {{val|5|e=6|u=K}} |
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|- |
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| [[Luminosity]] (L<sub>sol</sub>) |
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| {{val|3.846|e=26|ul=W}}<ref name=nssdc/><br/><small>≈ {{val|3.75|e=28|u=[[lumen (unit)|lm]]}}</small><br/><small>≈ {{val|98|u=lm/W}} [[Luminous efficacy|efficacy]]</small> |
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|- |
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| Mean [[Radiance|intensity]] (I<sub>sol</sub>) |
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| {{val|2.009|e=7|u=W·m<sup>−2</sup>·sr<sup>−1</sup>}} |
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|- |
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| Age |
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| ≈4.6 billion years<ref name="Bonanno">{{Cite journal |
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|last=Bonanno |first=A. |
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|last2=Schlattl |first2=H. |
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|last3=Paternò |first3=L. |
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|year=2008 |
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|title=The age of the Sun and the relativistic corrections in the EOS |
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|journal=[[Astronomy and Astrophysics]] |
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|volume=390 |issue=3 |pages=1115–1118 |
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|arxiv=astro-ph/0204331 |
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|bibcode=2002A&A...390.1115B |
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|doi=10.1051/0004-6361:20020749 |
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|ref=harv |
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}}</ref><ref>{{Cite web|url=//www.sciencemag.org/content/338/6107/651.full|title=The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk|date=2 November 2012|accessdate=17 March 2014|doi=10.1126/science.1226919 |journal=Science|volume=338 |issue= 6107 |pages=651–655}}{{Registration required}}</ref> |
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|- |
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! bgcolor="#FCC857" colspan="2" align=center |'''[[Rotation]] characteristics''' |
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|- |
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| [[Axial tilt|Obliquity]] |
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| 7.25°<ref name=nssdc/><br/><small>(to the [[ecliptic]])</small><br/>67.23°<br/><small>(to the [[galactic plane]])</small> |
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|- |
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| [[Right ascension]]<br/><small>of North pole<ref name="iau-iag"> |
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{{cite web |
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|last1=Seidelmann |first1=P. K. |
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|author2=''et al.'' |
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|title=Report Of The IAU/IAG Working Group On Cartographic Coordinates And Rotational Elements Of The Planets And Satellites: 2000 |
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|url=http://www.hnsky.org/iau-iag.htm |
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|publisher= |
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|year=2000 |
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|accessdate=2006-03-22 |
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}}</ref></small> |
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| 286.13°<br/><small>{{nowrap|19 h 4 min 30 s}}</small> |
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|- |
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| [[Declination]]<br/><small>of North pole</small> |
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| +63.87°<br/><small>63° 52' North</small> |
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|- |
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| Sidereal [[Solar rotation|rotation period]] <br/><small>(at equator)</small> |
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| 25.05 days<ref name=nssdc/> |
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|- |
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| <small>(at 16° latitude)</small> |
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| 25.38 days<ref name=nssdc/><br/><small>{{nowrap|25 d 9 h 7 min 12 s}}<ref name="iau-iag"/></small> |
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|- |
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| <small>(at poles)</small> |
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| 34.4 days<ref name=nssdc/><!-- derived from T = ( 14.37 - 2.33 sin^2 L - 1.56 sin^4 L ) deg/day, L = 90 deg --> |
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|- |
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| Rotation velocity<br/><small>(at equator)</small> |
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| {{val|7.189|e=3|u=km/h}}<ref name="sse"/><!-- Derived from NASA source: equatorial circumference of 4,379,000 kilometres divided by sidereal rotation period of 609.12 hours; maybe this kind of basic calculation could be done in some generic template code? --> |
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|- |
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! bgcolor="#FCC857" colspan="2" align=center | '''[[photosphere|Photospheric]] composition (by mass)''' |
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|- |
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| [[Hydrogen]] |
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| 73.46%<ref> |
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{{cite web |
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|title=The Sun's Vital Statistics |
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|url=http://solar-center.stanford.edu/vitalstats.html |
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|publisher=[[Stanford Solar Center]] |
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|accessdate=2008-07-29 |
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}} Citing {{cite book |
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|last=Eddy |first=J. |
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|year=1979 |
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|title=A New Sun: The Solar Results From Skylab |
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|url=http://history.nasa.gov/SP-402/contents.htm |
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|page=37 |
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|publisher=[[NASA]] |
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|id=NASA SP-402 |
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}}</ref> |
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|- |
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| [[Helium]] |
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| 24.85% |
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| [[Oxygen]] |
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| 0.77% |
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| [[Carbon]] |
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| 0.29% |
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| [[Iron]] |
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| 0.16% |
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|- |
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| [[Neon]] |
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| 0.12% |
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| [[Nitrogen]] |
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| 0.09% |
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| [[Silicon]] |
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| 0.07% |
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| [[Magnesium]] |
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| 0.05% |
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|- |
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| [[Sulfur]] |
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| 0.04% |
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|- |
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| align="center" colspan="2" | {{navbar|Sun}} |
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|}<noinclude> |
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{{R from more specific name}} |
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Latest revision as of 16:59, 18 January 2023
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