Answer:
Kepler's third law of planetary motion
Explanation:
Kepler's third law of motion gives the relationship between a planet’s distance from the sun and the amount of time it takes the planet to orbit the sun. Its formula is given by :
[tex]T^2=\dfrac{4\pi ^2}{GM}a^3[/tex]
Where
T is the time taken by the planet to orbit the sun
M is the mass of sun
G is the universal gravitational constant
a is the distance of planet form the sun
