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Baris 1:
{{Infobox
{| class="infobox" style="width: 20em;"
| name = matahari
|+ style="font-size:larger;" | '''Matahari''' [[Image:Sun symbol.svg|25px]]
| bodystyle = width:25em
|-
| title = Matahari [[File:Sun symbol (bold).svg|24px|☉]]
| 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]]
| image = [[File:The Sun in white light.jpg|frameless|275px]]
|-
| caption = Diproyeksikan dalam [[cahaya tampak]] dengan [[filter surya]] pada tahun 2019 dengan [[bintik matahari]] dan [[penggelapan tepi]]
! bgcolor="#FCC857" colspan="2" align=center | '''Data pengamatan'''
| image2 = [[File:The Sun by the Atmospheric Imaging Assembly of NASA's Solar Dynamics Observatory - 20100819.jpg|frameless|275px]]
|-
| caption2 = Gambar [[warna semu|berwarna semu]] yang diambil pada tahun 2010 yang diproyeksikan oleh [[sinar ultraungu]] (panjang gelombang 30,4 nm)
| '''Jarak rata-rata'''<br/><small>dari [[Bumi]]</small>
| headerstyle = background:#FCC857
| {{val|1.496|e=8|u=km}}<br/><small>8&nbsp;menit 19&nbsp;detik ([[kecepatan cahaya]])</small>
| labelstyle = padding:2px
|-
| datastyle = padding:2px
| '''[[Magnitudo tampak|Kecerahan visual]]''' (''V'')
| label1 = Nama
| −26,74<ref name=nssdc>
| data1 = Matahari, Surya,<ref>[https://kbbi.kemdikbud.go.id/entri/surya Surya — KBBI Daring]</ref> Mentari,<ref>[https://kbbi.kemdikbud.go.id/entri/mentari Mentari — KBBI Daring]</ref> Syamsu,<ref>[https://kbbi.kemdikbud.go.id/entri/syamsu Syamsu — KBBI Daring]</ref> Syamsi,<ref>[https://kbbi.kemdikbud.go.id/entri/syamsi Syamsi — KBBI Daring]</ref> Rawi,<ref>[https://kbbi.kemdikbud.go.id/entri/rawi Rawi — KBBI Daring]</ref> Baskara,<ref>[https://kbbi.kemdikbud.go.id/entri/baskara Baskara— KBBI Daring]</ref> ''Sun'', ''Sol'',<ref name=OED>{{OED|Sol}}</ref> ''Helios''<ref name=Lexico>{{Lexico|Helios}}</ref>
{{cite web
| label2 = Kata sifat
|last=Williams |first=D. R.
| data2 = Solar,<ref name=OED2>{{OED|solar}}</ref><ref>[https://kbbi.kemdikbud.go.id/entri/solar%20(2) Solar<sup>2</sup> — KBBI Daring]</ref> Surya
|year=2004
 
|title=Sun Fact Sheet
<!-- section break, rows 1-19-->
|url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html
| header3 = Data pengamatan
|publisher=[[NASA]]
| label4 = Jarak rata-rata<br/><small>dari [[Bumi]]</small>
|accessdate=2010-09-27
| data4 = {{val|1|ul=AU}} ≈ {{val|1.496|e=8|u=km}}<ref name="Pitjeva2009">{{Cite journal |last1=Pitjeva |first1=E. V. |last2=Standish |first2=E. M. |date=2009 |title=Proposals for the masses of the three largest asteroids, the Moon–Earth mass ratio and the Astronomical Unit |journal=[[Celestial Mechanics and Dynamical Astronomy]] |language=en |volume=103 |issue=4 |pages=365–372 |doi=10.1007/s10569-009-9203-8 |issn=1572-9478 |url=https://zenodo.org/record/1000691 |bibcode=2009CeMDA.103..365P|s2cid=121374703 }}</ref><br />8&nbsp;min 19&nbsp;s ([[laju cahaya]])
}}</ref>
| label5 = [[Magnitudo semu|Kecerahan visual]] (''V'')
|-
| data5 = −26,74<ref name=nssdc>{{cite web |last=Williams |first=D.R. |date=1 Juli 2013 |title=Sun Fact Sheet |url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html |publisher=[[NASA Goddard Space Flight Center]] |accessdate=12 Agustus 2013 |archive-url=https://web.archive.org/web/20100715200549/http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html |archive-date=15 Juli 2010 |url-status=dead}}</ref>
| '''[[Magnitudo absolut]]'''
| label6 = [[Magnitudo mutlak]]
| 4,83<ref name=nssdc />
| data6 = 4,83<ref name=nssdc />
|-
| ''' label7 = [[Klasifikasi bintang|Klasifikasi spektrum]]'''
| data7 = G2V<ref>{{cite book |last=Zombeck |first=Martin V. |date=1990 |title=Handbook of Space Astronomy and Astrophysics 2nd edition |publisher=[[Cambridge University Press]] |url=http://ads.harvard.edu/books/hsaa/}}</ref>
| G2V
| label8 = [[Metalisitas|Kelogaman]]
|-
| data8 = ''Z'' = 0,0122<ref>{{cite journal |last1=Asplund |first1=M. |last2=Grevesse |first2=N. |last3=Sauval |first3=A.J. |date=2006 |title=The new solar abundances – Part I: the observations |journal=Communications in Asteroseismology |volume=147 |pages=76–79 |bibcode=2006CoAst.147...76A |doi=10.1553/cia147s76|s2cid=123824232 |url=http://pdfs.semanticscholar.org/05ac/bc83e2e4e19318d3eca489fe60300eb0388b.pdf }}</ref>
| '''[[Metalisitas]]'''
| label9 = [[Diameter sudut]]
| ''Z'' = 0,0122<ref>
| data9 = 31,6–32,7 [[menit busur]]<ref>{{cite web |title=Eclipse 99: Frequently Asked Questions |url=http://education.gsfc.nasa.gov/eclipse/pages/faq.html |publisher=NASA |accessdate=24 Oktober 2010 |url-status=dead |archiveurl=https://web.archive.org/web/20100527142627/http://education.gsfc.nasa.gov/eclipse/pages/faq.html |archivedate=27 Mei 2010 |df=}}</ref>
{{cite journal
| header10 = Ciri-ciri [[orbit]]
|last=Asplund|first=M.
| label11 = Jarak rata-rata<br /><small><span style="white-space:nowrap;">dari pusat [[Bima Sakti]]</small></span>
|coauthors=N. Grevesse and A. J. Sauval
| data11 = ≈ {{val|2.7|e=17|u=km}}<br />{{nowrap|{{val|27200|u=[[tahun cahaya]]}}}}
|year=2006
| label12 = [[Tahun galaksi|Periode galaksi]]
|title=The new solar abundances - Part I: the observations
| data12 = (2,25–2,50){{e|8}} [[Tahun Julian|a]]
|journal=Communications in Asteroseismology
| label13 = [[Kecepatan]]
|volume=147 |pages=76–79
| data13 = ≈ {{val|220|u=km/s}} (orbit mengitari pusat Bima Sakti) <br />≈ {{val|20|u=km/s}} (relatif terhadap kecepatan rata-rata bintang lain dalam kelompok bintang) <br />≈ {{val|370|u=km/s}}<ref>{{cite journal |last=Hinshaw |first=G. |display-authors=etal |year=2009 |title=Five-year Wilkinson Microwave Anisotropy Probe observations: data processing, sky maps, and basic results |journal=[[The Astrophysical Journal Supplement Series]] |volume=180 |issue=2 |pages=225–245 |arxiv=0803.0732 |bibcode=2009ApJS..180..225H |doi=10.1088/0067-0049/180/2/225|s2cid=3629998 }}</ref> (relatif terhadap [[Radiasi latar belakang gelombang mikrokosmis|latar belakang gelombang mikrokosmis]])
|bibcode=2006CoAst.147...76A
 
|doi=10.1553/cia147s76
<!-- section break, rows 20–39 -->
}}</ref>
| header20 = Ciri-ciri fisik
|-
| label21 = [[Jari-jari]] khatulistiwa
| '''[[Ukuran anguler]]'''
| data21 = [[Jari-jari matahari|695.700]]&nbsp;km<ref name=IAU2015resB3>{{cite arxiv |first1=E.E. |last1=Mamajek |first2=A. |last2=Prsa |first3=G. |last3=Torres |first4=al. |last4=et |title=IAU 2015 Resolution B3 on Recommended Nominal Conversion Constants for Selected Solar and Planetary Properties |eprint=1510.07674 |mode=cs2 |class=astro-ph.SR |year=2015}}</ref><br />696.342 km<ref name=arxiv1203_4898>{{citation |first1=Marcelo |last1=Emilio |first2=Jeff R. |last2=Kuhn |first3=Rock I. |last3=Bush |first4=Isabelle F. |last4=Scholl |title=Measuring the Solar Radius from Space during the 2003 and 2006 Mercury Transits |arxiv=1203.4898 |bibcode=2012ApJ...750..135E |doi=10.1088/0004-637X/750/2/135 |volume=750 |issue=2 |journal=The Astrophysical Journal |page=135 |year=2012|s2cid=119255559 }}</ref><br />{{val|109|u=[[Jari-jari Bumi|× Bumi]]}}<ref name=sse/>
| 31,6′ – 32,7′<ref>
| label22 = [[Keliling]] khatulistiwa
{{cite web
| data22 = {{val|4.379|e=6|u=km}}<ref name=sse/><br />109 × Bumi<ref name=sse>{{cite web |title=Solar System Exploration: Planets: Sun: Facts & Figures |url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=Facts&System=Metric |archiveurl=https://web.archive.org/web/20080102034758/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=Facts&System=Metric |archivedate=2 Januari 2008 |publisher=NASA}}</ref>
|title=Eclipse 99: Frequently Asked Questions
| label23 = [[Kepepatan]]
|url=http://education.gsfc.nasa.gov/eclipse/pages/faq.html
| data23 = {{val|9|e=-6}}
|publisher=[[NASA]]
| label24 = [[Luas permukaan]]
|accessdate=2010-10-24
| data24 = {{val|6.09|e=12|u=km2}}<ref name=sse/><br />{{nowrap|{{val|12000}}}} × Bumi<ref name=sse/>
}}</ref>
| label25 = [[Volume]]
|-
| data25 = {{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 />{{nowrap|{{val|1300000}}}} × Bumi
| '''Kata sifat'''
| label26 = [[Massa]]
| Surya
| data26 = {{val|1.9891||e=30|u=kg}}<ref name=nssdc/><br />{{nowrap|{{val|333000|u=[[Massa bumi|× Bumi]]}}}}<ref name=nssdc/><!-- NASA Sun Fact Sheet states 333,000, a figure coherent with data already present in en.wiki -->
|-
| label27 = [[Kepadatan]] rata-rata
! bgcolor="#FCC857" colspan="2" align=center | '''Ciri-ciri [[orbit]]'''
| data27 = {{val|1.408|e=3|u=kg/m3}}<ref name=nssdc/><ref name=sse/><ref>
|-
| '''Jarak rata-rata'''<br/><small>dari inti [[Bima Sakti]]</small>
| ~{{val|2.5|e=17|u=km}}<br/><small>{{val|26000|u=[[tahun cahaya]]}}</small>
|-
| '''Periode [[galaksi]]'''
| (2,25–2,50){{e|8}} [[tahun Julian (astronomi)|a]]
|-
| '''[[Kecepatan]]'''
| ~{{val|220|u=km/detik}} <small>(orbit mengitari pusat galaksi)</small> <br />~{{val|20|u=km/detik}} <small>(relatif terhadap kecepatan rata-rata bintang lain dalam grup bintang)</small> <br />~{{val|370|u=km/detik}}<ref>
{{cite journal
|last=Hinshaw |first=G.
|coauthors=''et al.''
|year=2009
|title=Five-year Wilkinson Microwave Anisotropy Probe observations: data processing, sky maps, and basic results
|journal=The [[Astrophysical Journal]] Supplement Series
|volume=180 |pages=225–245
|doi=10.1088/0067-0049/180/2/225
|bibcode=2009ApJS..180..225H
|issue=2
}}</ref> <small>(relatif terhadap [[radiasi latar gelombang mikro kosmik#anisotropi dipol CMBR|latar gelombang mikro kosmik]])</small>
|-
! bgcolor="#FCC857" colspan="2" align=center | '''Ciri-ciri fisik'''
|-
| '''Diameter rata-rata'''
| {{val|1.392684|e=6|u=km}}<ref name=arxiv1203_4898>{{citation |first1=Marcelo |last1=Emilio |first2=Jeff R. |last2=Kuhn |first3=Rock I. |last3=Bush |first4=Isabelle F. |last4=Scholl |title=Measuring the Solar Radius from Space during the 2003 and 2006 Mercury Transits |work=arXiv |url=http://arxiv.org/abs/1203.4898 |date=March 5, 2012 |accessdate=March 28, 2012}}</ref>
|-
| '''[[Radius]] khatulistiwa'''
| {{val|6.96342|e=5|u=km}}<ref name=arxiv1203_4898 /> <br/><small>109 × Bumi<small/><ref name=sse/>
|-
| '''[[Keliling]] khatulistiwa'''
| {{val|4.379|e=6|u=km}}<ref name=sse/><br/><small>109 × Bumi<small/><ref name=sse>
{{cite web
|title=Solar System Exploration: Planets: Sun: Facts & Figures
|url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=Facts&System=Metric
|archiveurl=http://web.archive.org/web/20080102034758/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun&Display=Facts&System=Metric
|archivedate=2008-01-02
|publisher=[[NASA]]
}}</ref>
|-
| '''[[Pemipihan]]'''
| {{val|9|e=-6}}
|-
| '''[[Luas permukaan]]'''
| {{val|6.0877|e=12|u=km2}}<ref name=sse/><br/><small>{{val|11990}} × Bumi</small><ref name=sse/>
|-
| '''[[Volum]]'''
| {{val|1.412|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) --><br/><small>{{val|1300000}} × Bumi</small>
|-
| '''[[Massa]]'''
| <!-- 1.988&nbsp;435 Someone please cite this before implementing it. -->{{val|1.9891|e=30|u=kg}}<ref name=nssdc/><br/><small>{{val|333000}} × Bumi</small><ref name=nssdc/><!-- NASA Sun Fact Sheet states 333,000, a figure coherent with data already present in en.wiki -->
|-
| '''[[Kepadatan|Kepadatan rata-rata]]'''
| {{val|1.408|e=3|u=kg/m3}}<ref name=nssdc/><ref name=sse/><ref>
{{cite web
|last=Ko |first=M.
Baris 112 ⟶ 60:
|editor=Elert, G.
|work=The Physics Factbook
}}</ref><br />{{val|1.408|u=g/cm3}}<ref name=nssdc/><ref name=sse/><ref>{{cite web |last=Ko |first=M. |date=1999 |title=Density of the Sun |url=http://hypertextbook.com/facts/1999/MayKo.shtml |editor=Elert, G. |website=The Physics Factbook}}</ref><br />{{val|0.255}} × Bumi<ref name=nssdc/><ref name=sse/>
}}</ref>
| label28 = [[Kepadatan]]
|-
| data28 = '''pusat <small>(permodelan)</small>'''<br />{{val|1.622|e=5|u=kg/m3}}<ref name=nssdc/><br />{{val|162.2|u=g/cm3}}<ref name=nssdc/><br />{{val|12.4}} × Bumi<br />'''fotosfer'''<br />{{val|2|e=-4|u=kg/m3}}<br />'''kromosfer'''<br />{{val|5|e=-6|u=kg/m3}}<br />'''korona <small>(rata-rata)</small>'''<br />{{val|1|e=-12|u=kg/m3}}<ref>
| '''[[Kepadatan]]'''
| Pusat (model): {{val|1.622|e=5|u=kg/m3}}<ref name=nssdc/><br/>Fotosfer bawah: {{val|2|e=-4|u=kg/m3}}<br/>Kromosfer bawah: {{val|5|e=-6|u=kg/m3}}<br/>Korona ({{dabbr|rt|rata-rata}}): {{val|1|e=-12|u=kg/m3}}<ref>
{{cite web
|last= |first=
|date=30 AugustAgustus 2007
|title=Principles of Spectroscopy
|url=http://www.astro.lsa.umich.edu/undergrad/Labs/spectro/short_spectro.html
|publisher=[[University ofUniversitas Michigan]], Astronomy Department
}}</ref>
| label29 = [[Gravitasi permukaan]] khatulistiwa
|-
| data29 = {{val|274|u=m/s2}}<ref name=nssdc/><br />28 × Bumi<ref name=sse/>
| '''[[Gravitasi permukaan]] khatulistiwa'''
| label30 = [[Faktor momen inersia]]
| {{val|274.0|u=m/s2}}<ref name=nssdc/><br/>{{val|27.94|u=[[gaya G|''g'']]}}<br/><small>{{val|27542.29|u=[[cgs|''cgs'']]}}<br/>28 × Bumi<small/><ref name=sse/>
| data30 = {{val|0.070}}<ref name=nssdc /> (perkiraan)
|-
| ''' label31 = [[Kecepatan lepas]]'''<br /><small>(dari permukaan)</small>
| data31 = {{val|617.7|u=km/detiks}}<ref name=sse/><br /><small>55 × Bumi</small><ref name=sse/>
| label32 = Suhu
|-
| data32 = '''pusat <small>(permodelan)</small>'''<br />{{val|1.57|e=7|u=K}}<ref name=nssdc/><br />'''[[fotosfer]] <small>(efektif)</small>'''<br />{{nowrap|{{val|5772|ul=K}}}}<ref name=nssdc/><br />'''[[korona]]'''<br />≈ {{val|5|e=6|u=K}}
| '''[[Suhu]]'''
| label33 = [[Luminositas]] (L<sub>sol</sub>)
| Pusat (model): ~{{val|1.57|e=7|u=K}}<ref name=nssdc/><br>Fotosfer (efektif): {{val|5778|ul=K}}<ref name=nssdc/><br> [[Korona]]: ~{{val|5|e=6|u=K}}
| data33 = {{val|3.828|e=26|ul=W}}<ref name=nssdc/><br />≈ {{val|3.75|e=28|u=[[Lumen (satuan)|lm]]}}<br />≈ {{val|98|u=lm/W}} [[Efikasi cahaya|efikasi]]
|-
| label34 = [[Indeks warna|Warna]] (B-V)
| '''[[Luminositas]]''' (L<sub>sol</sub>)
| data34 = 0,63
| {{val|3.846|e=26|ul=W}}<ref name=nssdc/><br/><small>~{{val|3.75|e=28|u=[[lumen (satuan)|lm]]}}</small><br/><small>~{{val|98|u=lm/W}} [[daya penerangan|daya]]</small>
| label35 = [[Radians]] rata-rata&nbsp;(I<sub>sol</sub>)
|-
| data35 = {{val|2.009|e=7|u=W·m<sup>−2</sup>·sr<sup>−1</sup>}}
| '''[[Radians|Intensitas]] rata-rata'''&nbsp;(I<sub>sol</sub>)
| label36 = Umur
| {{val|2.009|e=7|u=W·m<sup>−2</sup>·sr<sup>−1</sup>}}
| data36 = ≈ 4,6 miliar tahun<ref name="Bonanno">{{Cite journal |last1=Bonanno |first1=A. |last2=Schlattl |first2=H. |last3=Paternò |first3=L. |year=2002 |title=The age of the Sun and the relativistic corrections in the EOS |journal=[[Astronomy and Astrophysics]] |volume=390 |issue=3 |pages=1115–1118 |arxiv=astro-ph/0204331 |bibcode=2002A&A...390.1115B |doi=10.1051/0004-6361:20020749 |ref=harv}}</ref><ref>{{Cite journal |title=The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk |date=2 November 2012 |doi=10.1126/science.1226919 |journal=Science |volume=338 |issue=6107 |pages=651–655 |bibcode=2012Sci...338..651C |pmid=23118187 |last1=Connelly |first1=JN |last2=Bizzarro |first2=M |last3=Krot |first3=AN |last4=Nordlund |first4=Å |last5=Wielandt |first5=D |last6=Ivanova |first6=MA|s2cid=21965292 }}{{Registration required}}</ref>
|-
 
| '''Usia'''
<!-- section break, rows 40–49 -->
| 4,57 miliar tahun<ref name="Bonanno">{{Cite journal
| header40 = Ciri-ciri [[rotasi]]
|last=Bonanno |first=A. |last2=Schlattl |first2=H. |last3=Paternò |first3=L.
| label41 = [[Kemiringan sumbu]]
|title=The age of the Sun and the relativistic corrections in the EOS
| data41 = 7,25°<ref name=nssdc/><br /><small>(terhadap [[ekliptika]])</small><br />67,23°<br /><small>(terhadap [[bidang galaksi]])</small>
|journal=[[Astronomy and Astrophysics]]
| label42 = [[Asensio rekta]]<br /><small>pada kutub utara</small><ref name="iau-iag">{{cite web |last1=Seidelmann |first1=P.K. |display-authors=etal |title=Report Of The IAU/IAG Working Group On Cartographic Coordinates And Rotational Elements Of The Planets And Satellites: 2000 |url=http://www.hnsky.org/iau-iag.htm |date=2000 |accessdate=22 Maret 2006}}</ref>
|volume=390
| data42 = 286,13°<br />{{nowrap|19 jam 4 menit 30 detik}}
|issue=3 |pages=1115–1118
| label43 = [[Deklinasi]]<br /><small>pada kutub utara</small>
|year= 2008
| data43 = +63,87°<br />63° 52' LU
|doi=10.1051/0004-6361:20020749
| label44 = [[Rotasi matahari|Periode rotasi]] sideris
|arxiv=astro-ph/0204331
| data44 = '''terhadap khatulistiwa'''<br />25,05 hari<ref name=nssdc/><br />'''terhadap lintang 16°'''<br />25,38 hari<ref name=nssdc/><br />{{nowrap|25 hari 9 jam 7 menit 12 detik}}<ref name="iau-iag"/><br />'''terhadap kutub'''<br />34,4 hari<ref name=nssdc/><!-- derived from T = ( 14.37 − 2.33 sin^2 L − 1.56 sin^4 L ) °/day, L = 90° -->
|ref=harv |bibcode=2002A&A...390.1115B
| label47 = Kecepatan rotasi<br /><small>(terhadap khatulistiwa)</small>
}}</ref>
| data47 = {{val|7.189|e=3|u=km/h}}<ref name="sse"/><!-- Derived from NASA source: equatorial circumference of 4,379,000 kilometers divided by sidereal rotation period of 609.12 hours; maybe this kind of basic calculation could be done in some generic template code? -->
|-
 
! bgcolor="#FCC857" colspan="2" align=center |'''Ciri-ciri [[rotasi]]'''
<!-- section break, rows 50–69 -->
|-
| header50 = Komposisi [[fotosfer]] (menurut massa)
| '''[[Kemiringan sumbu|Kemiringan]]'''
| label51 = [[Hidrogen]]
| 7,25°<ref name=nssdc/><br/><small>(terhadap [[ekliptika]])</small><br/>67,23°<br/><small>(terhadap [[bidang galaksi]])</small>
| data51 = 73,46%<ref>{{cite web |title=The Sun's Vital Statistics |url=http://solar-center.stanford.edu/vitalstats.html |publisher=Stanford Solar Center |accessdate=29 Juli 2008}} Citing {{cite book |last=Eddy |first=J. |date=1979 |title=A New Sun: The Solar Results From Skylab |url=https://history.nasa.gov/SP-402/contents.htm |page=37 |publisher=NASA |id=NASA SP-402}}</ref>
|-
| label52 = [[Helium]]
| '''[[Asensio rekta]]'''<br/><small>dari kutub utara<ref name="iau-iag">
| data52 = 24,85%
{{cite web
| label53 = [[Oksigen]]
|last1=Seidelmann |first1=P. K.
| data53 = 0,77%
|coauthors=''et al.''
| label54 = [[Karbon]]
|title=Report Of The IAU/IAG Working Group On Cartographic Coordinates And Rotational Elements Of The Planets And Satellites: 2000
| data54 = 0,29%
|url=http://www.hnsky.org/iau-iag.htm
| label55 = [[Besi]]
|publisher=
| data55 = 0,16%
|year=2000
| label56 = [[Neon]]
|accessdate=2006-03-22
| data56 = 0,12%
}}</ref></small>
| label57 = [[Nitrogen]]
| 286,13°<br/><small>{{nowrap|19 jam 4 menit 30 detik}}</small>
| data57 = 0,09%
|-
| label58 = [[Silikon]]
| '''[[Deklinasi]]'''<br/><small>dari kutub utara</small>
| data58 = 0,07%
| +63,87°<br/><small>63° 52' Utara</small>
| label59 = [[Magnesium]]
|-
| data59 = 0,05%
| '''[[rotasi matahari|Rotasi]] sidereal'''<br/><small>(di khatulistiwa)</small>
| label60 = [[Belerang]]
| 25,05 hari<ref name=nssdc/>
| data60 = 0,04%
|-
}}<noinclude>
| <small>(di lintang 16°)</small>
| 25,38 hari<ref name=nssdc/><br/><small>{{nowrap|25 hari 9 jam 7 menit 12 detik}}<ref name="iau-iag"/></small>
|-
| <small>(di kutub)</small>
| 34,4 hari<ref name=nssdc/><!-- derived from T = ( 14.37 - 2.33 sin^2 L - 1.56 sin^4 L ) deg/day, L = 90 deg -->
|-
| '''Kecepatan rotasi'''<br/><small>(di khatulistiwa)</small>
| {{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? -->
|-
! bgcolor="#FCC857" colspan="2" align=center | '''Komposisi [[fotosfer]] (menurut massa)'''
|-
| [[Hidrogen]]
| 73.46%<ref>
{{cite web
|title=The Sun's Vital Statistics
|url=http://solar-center.stanford.edu/vitalstats.html
|publisher=[[Stanford Solar Center]]
|accessdate=2008-07-29
}}, citing {{cite book
|last=Eddy |first=J.
|title=A New Sun: The Solar Results From Skylab
|url=http://history.nasa.gov/SP-402/contents.htm
|publisher=[[NASA]]
|year=1979
|page=37
|id=NASA SP-402
}}</ref>
|-
| [[Helium]]
| 24,85%
|-
| [[Oksigen]]
| 0,77%
|-
| [[Karbon]]
| 0,29%
|-
| [[Besi]]
| 0,16%
|-
| [[Neon]]
| 0,12%
|-
| [[Nitrogen]]
| 0,09%
|-
| [[Silikon]]
| 0,07%
|-
| [[Magnesium]]
| 0,05%
|-
| [[Belerang]]
| 0,04%
|-
| align="center" colspan="2" | {{navbar|Solar System Infobox/Sun}}
|}<noinclude>
 
{{pp-template}}
{{Daftar referensi templat}}
 
[[CategoryKategori:Templat kotakinfo astronomi|{{PAGENAME}}]]
 
</noinclude>
Diperoleh dari "https://wiki-indonesia.club/wiki/Templat:Matahari"