Answer:
8 years
Step-by-step explanation:
We can solve the problem by using Kepler's third law, which states that the cube of the radius of the orbit of a planet is proportional to the square of its orbital period. We can rewrite this law as follows:

where
is the distance of the Earth from the Sun
is the Earth's orbital period
is the distance of the planet from the Sun
is its orbital period
By re-arranging the equation and substituting the numbers, we can find T2:
