By using Kepler’s law
T2∝r3
By substituting the time period and the value of radius we get
(T1T2)2=(r1r2)3
(365T2)2=(2r1r1)3
T2=3652√2
The time period will be129days
If the distance between the earth and the sun were reduces to half its present value, Then the number of days in one year would have been
If the distance between the Earth and the Sun were half its present value, the approximate number of days in a year on the Earth would have been: