Motion in Straight Line
Distance of the Earth from the Sun, re = 1.5 × 108 km
= 1.5 × 1011 m
Time period of the Earth = Te
Time period of Saturn, Ts = 29. 5 Te
Distance of Saturn from the Sun = rs
From Kepler’s third law of planetary motion,
T = (4π2r3 / GM)1/2
For Saturn and Sun,
rs3 / re3 = Ts2 / Te2
rs = re(Ts / Te)2/3
= 1.5 × 1011 (29.5 Te / Te)2/3
= 1.5 × 1011 (29.5)2/3
= 14.32 × 1011 m
Hence, the distance between Saturn and the Sun is 1.43 × 1012 m.
Sponsor Area
State which of the following are examples of one, two or three dimensional motion:
(a) A kite flying in the sky.
(b) The earth revolving around the sun.
(c) A train moving along the equator of the earth in clockwise direction.
(d) Accelerated motion of a particle in a straight line.
Sponsor Area
Sponsor Area