abhishek its easy use keplers 3 law
T^2 IS PROPORTIONAL TO a^3
LET T1 & T2 BE THE TIME OF REVO FOR EARTH
& SATURN . AND A1 &A2 BE RADIUS OF THEIR ORBIT
THEN
[T2/T1]^2 =[A2/A1]^3 PUT IN THE VALUES AND CALCULATE
29.5^2 = [A2/1.5]^3
A2=14.3 YOU HAVE DISPLACED THE DECIMAL POINT
you can always use kepplers law coz its for planetary motion and not to b considered only for earth or its sattltes....so in any motion whose path is elliptical we can use kepplers law
T^2 IS PROPORTIONAL TO a^3
LET T1 & T2 BE THE TIME OF REVO FOR EARTH
& SATURN . AND A1 &A2 BE RADIUS OF THEIR ORBIT
THEN
[T2/T1]^2 =[A2/A1]^3 PUT IN THE VALUES AND CALCULATE
29.5^2 = [A2/1.5]^3
A2=14.3 YOU HAVE DISPLACED THE DECIMAL POINT