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Sun characteristics

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The Sun
Observation data
Mean distance
from Earth
1.496×108 km
8 min 19 s at light speed
Visual brightness (V) −26.74[1]
Absolute magnitude 4.83[1]
Spectral classification G2V
Metallicity Z = 0.0122[2]
Angular size 31.6′ – 32.7′[3]
Adjectives Solar
Orbital characteristics
Mean distance
from Milky Way core
~2.5×1017 km
26000 light-years
Galactic period (2.25–2.50)×108 a
Velocity ~220 km/s (orbit around the center of the Galaxy)
~20 km/s (relative to average velocity of other stars in stellar neighborhood)
~370 km/s[4] (relative to the cosmic microwave background)
Physical characteristics
Mean diameter 1.392684×106 km[5]
Equatorial radius 6.96342×105 km[5]
109 × Earth[6]
Equatorial circumference 4.379×106 km[6]
109 × Earth[6]
Flattening 9×10−6
Surface area 6.0877×1012 km2[6]
11990 × Earth[6]
Volume 1.412×1018 km3[6]
1300000 × Earth
Mass 1.9891×1030 kg[1]
333000 × Earth[1]
Average density 1.408×103 kg/m3[1][6][7]
Density Center (model): 1.622×105 kg/m3[1]
Lower photosphere: 2×10−4 kg/m3
Lower chromosphere: 5×10−6 kg/m3
Corona (Template:Dabbr): 1×10−12 kg/m3[8]
Equatorial surface gravity 274.0 m/s2[1]
27.94 g
28 × Earth[6]
Escape velocity
(from the surface)
617.7 km/s[6]
55 × Earth[6]
Temperature Center (modeled): ~1.57×107 K[1]
Photosphere (effective): 5778 K[1]
Corona: ~5×106 K
Luminosity (Lsol) 3.846×1026 W[1]
~3.75×1028 lm
~98 lm/W efficacy
Mean intensity (Isol) 2.009×107 W·m−2·sr−1
Age 4.57 billion years[9]
Rotation characteristics
Obliquity 7.25°[1]
(to the ecliptic)
67.23°
(to the galactic plane)
Right ascension
of North pole[10]
286.13°
19 h 4 min 30 s
Declination
of North pole
+63.87°
63° 52' North
Sidereal rotation period
(at equator)
25.05 days[1]
(at 16° latitude) 25.38 days[1]
25 d 9 h 7 min 12 s[10]
(at poles) 34.4 days[1]
Rotation velocity
(at equator)
7.189×103 km/h[6]
Photospheric composition (by mass)
Hydrogen 73.46%[11]
Helium 24.85%
Oxygen 0.77%
Carbon 0.29%
Iron 0.16%
Neon 0.12%
Nitrogen 0.09%
Silicon 0.07%
Magnesium 0.05%
Sulfur 0.04%

  1. ^ a b c d e f g h i j k l m n Williams, D. R. (2004). "Sun Fact Sheet". NASA. Retrieved 2010-09-27.
  2. ^ Asplund, M. (2006). "The new solar abundances - Part I: the observations". Communications in Asteroseismology. 147: 76–79. Bibcode:2006CoAst.147...76A. doi:10.1553/cia147s76. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  3. ^ "Eclipse 99: Frequently Asked Questions". NASA. Retrieved 2010-10-24.
  4. ^ Hinshaw, G. (2009). "Five-year Wilkinson Microwave Anisotropy Probe observations: data processing, sky maps, and basic results". The Astrophysical Journal Supplement Series. 180 (2): 225–245. Bibcode:2009ApJS..180..225H. doi:10.1088/0067-0049/180/2/225. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  5. ^ a b Emilio, Marcelo; Kuhn, Jeff R.; Bush, Rock I.; Scholl, Isabelle F. (March 5, 2012), "Measuring the Solar Radius from Space during the 2003 and 2006 Mercury Transits", arXiv, retrieved March 28, 2012
  6. ^ a b c d e f g h i j k "Solar System Exploration: Planets: Sun: Facts & Figures". NASA. Archived from the original on 2008-01-02.
  7. ^ Ko, M. (1999). Elert, G. (ed.). "Density of the Sun". The Physics Factbook.
  8. ^ "Principles of Spectroscopy". University of Michigan, Astronomy Department. 30 August 2007.
  9. ^ Bonanno, A.; Schlattl, H.; Paternò, L. (2008). "The age of the Sun and the relativistic corrections in the EOS". Astronomy and Astrophysics. 390 (3): 1115–1118. arXiv:astro-ph/0204331. Bibcode:2002A&A...390.1115B. doi:10.1051/0004-6361:20020749. {{cite journal}}: Invalid |ref=harv (help)
  10. ^ a b Seidelmann, P. K. (2000). "Report Of The IAU/IAG Working Group On Cartographic Coordinates And Rotational Elements Of The Planets And Satellites: 2000". Retrieved 2006-03-22. {{cite web}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  11. ^ "The Sun's Vital Statistics". Stanford Solar Center. Retrieved 2008-07-29., citing Eddy, J. (1979). A New Sun: The Solar Results From Skylab. NASA. p. 37. NASA SP-402.