Sun
The sun is fairly an orinary star of
spectral type G2V and with a madnitude of 4.8.However ,is proximity to the
earth makes it of most immediate interest to us also most accessible for
styudy.The vital statistics of the sun are follows;
Age=4.5*10 9 year
Mass=1.99*10 30 kg
Radius=696000 km
Mean density=1.4*10 3 kg/m 3
Mean distance
from earth=150*10 6 km
Surface gravity=274 m/s
Escapevelocity at surface=618 km/s
Luminosity=3.86*10 26 W
Equtorial rotation period=26 days
Mass loss rate=10 9 kg/s
Effective black body temperature=5785 k
Inclination of sun’s equator to plane of
earth’s orbit=7 0
Composition;
Approximately 90% H, 10% He,0.1%
other elemente like C, N, O…..etc
COMPARISON OF SUN
WITH EARTH:
Inoeder to put some of these figures into perspective,we may note that
the sun’s mass is 330000 times that of earth, and its radius is 109 times
larger.The mean density of earth is only about 4 times that of the sun,the
atmospheric density at surfece of earth is 1 kg/m 3 .which makesthe
earths sea level atmospheric pressure five times the suns surface pressure.One
astronomical unit (AU) is only 215 times of the radius of the sun and it takes
sunlight 8 min to reach the earth.the suns emmitted radiation amounts to 1kW/m 2 at the surface of earth.the surface gravityis
27 times greater at the sun,and the suns rotation produces an equatorial
velocity of 2 Km/s.
The sun is a massive ball of gas held
together ans compressed under its own gravitational attraction.It consists
primarly of H and He.Theses gases ar% of the mass of the sun and are present
roughly the sameproportion s on the earh.
R

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