✔ 最佳答案
Of course. It is because the sun is the star at the center of the Solar System. The Earth and other matter (including other planets, asteroids, meteoroids, comets and dust) orbit the Sun, which by itself accounts for about 99.8% of the solar system's mass. Energy from the Sun, in the form of sunlight, supports almost all life on Earth via photosynthesis, and drives the Earth's climate and weather.
The Sun
圖片參考:
http://upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Sun920607.jpg/270px-Sun920607.jpg
Observation data
Mean distance
from Earth
1.496×1011 m
8.31 min at light speed
Visual brightness (V)
−26.74m [54]
Absolute magnitude
4.83m [54]
Spectral classification
G2V
Angular size
31.6' - 32.7' [55]
Adjectives
solar
Orbital characteristics
Mean distance
from Milky Way core
~2.5×1020 m
26,000 light-years
Galactic period
2.25–2.50×108 a
Velocity
2.17×105 m/s
(orbit around the center of the Galaxy)
2×104 m/s
(relative to average velocity of other stars in stellar neighborhood)
Physical characteristics
Mean diameter
1.392×109 m [54]
109 Earths
Equatorial radius
6.955×108 m [56]
Equatorial circumference
4.379×109 m [56]
Flattening
9×10−6
Surface area
6.088×1018 m² [56]
11,900 Earths
Volume
1.4122×1027 m³ [56]
1,300,000 Earths
Mass
1.9891 ×1030 kg[54]
332,946 Earths
Average density
1.409 ×103 kg/m³ [56]
Equatorial surface gravity
274.0 m/s2 [54]
27.94 g
Escape velocity
(from the surface)
617.7 km/s [56]
55 Earths
Temperature
of surface (effective)
5,778 K [54]
Temperature
of corona
~5,000,000 K
Temperature
of core
~15,710,000 K [54]
Luminosity (Lsol)
3.846×1026 W [54]
~3.75×1028 lm
~98 lm/W efficacy
Mean Intensity (Isol)
2.009×107 W m-2 sr-1
Rotation characteristics
Obliquity
7.25° [54]
(to the ecliptic)
67.23°
(to the galactic plane)
Right ascension
of North pole[57]
286.13°
19 h 4 min 30 s
Declination
of North pole
+63.87°
63°52' North
Sidereal Rotation period
(at 16° latitude)
25.38 days [54]
25 d 9 h 7 min 13 s[57]
(at equator)
25.05 days [54]
(at poles)
34.3 days [54]
Rotation velocity
(at equator)
7.284 ×103 km/h
Photospheric composition (by mass)
Hydrogen
73.46 %
Helium
24.85 %
Oxygen
0.77 %
Carbon
0.29 %
Iron
0.16 %
Sulfur
0.12 %
Neon
0.12 %
Nitrogen
0.09 %
Silicon
0.07 %
Magnesium
0.05 %