Final answer:
Kepler's third law states that the orbital period squared is directly proportional to the cube of the semi-major axis of the orbit. This relationship can be represented by the equation P^2 = k * a^3, where P is the orbital period and a is the semi-major axis of the orbit.
Step-by-step explanation:
Kepler's third law states that the square of a planet's orbital period is directly proportional to the cube of the semi-major axis of its orbit. In equation form, this can be written as:
P^2 = k * a^3
Where P is the orbital period and a is the semi-major axis of the orbit. The constant k represents a proportionality constant that is the same for all planets orbiting the Sun.
When plotted on a graph, this relationship between P^2 and a^3 will result in a straight line with a positive slope.