According to Kepler’s law
T² ∝ r³
(T₁ / T₂)² = (r₁ / r₂)³
(365 / T₂)² = (2r₁ / r₁)³
(365 / T₂)² = 8
365 / T₂) = 2√2
T₂ = 365 / (2√2)
T₂ = 129 days
There will be 129 days in an year.
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 number of days in a year would have been