The orbital radius and period of a planet are directly related. This means that as the orbital radius increases, the period also increases. This relationship is known as Kepler's third law of planetary motion.
The larger the orbital radius, the longer it takes for a planet to complete one orbit around its star. This is because the further a planet is from its star, the weaker the gravitational pull, and therefore, it takes longer for the planet to complete its orbit.
The formula for calculating the orbital period of a planet is T = 2π√(a^3/GM), where T is the period, a is the orbital radius, G is the gravitational constant, and M is the mass of the central star.
No, the orbital radius is the distance between the planet and the center of its star. The distance from the planet to its star may vary depending on the shape of the planet's orbit.
The orbital period of a planet does not directly affect its temperature. However, the distance from the planet to its star, which is determined by the orbital radius and period, can impact the planet's temperature. A longer period and larger orbital radius may result in a colder planet, while a shorter period and smaller orbital radius may result in a warmer planet.