Kepler's third law states that the square of the period of a planet's orbit (T) is directly proportional to the cube of the semi-major axis of its orbit (r). Mathematically, this is often expressed as:
\[ \frac{T_1^2}{T_2^2} = \frac{r_1^3}{r_2^3} \]
This means that the correct response is:
The square of the ratio of the periods equals the cube of the ratio of the radii.