GIVE A BRIEF DESCRIPTION OF KEPLER'S LAW'S.
Kepler’s first law:
Kepler’s first law, the law of orbits, states that the orbit of a planet is an ellipse with the sun at one of the foci. An ellipse is a closed, curved shape that is defined by two points called foci representing an elongated circle.The closest point on a planet’s orbit from the sun is called perihelion and the farthest point from the sun is called the aphelion.
Kepler’s second law:
Kepler’s second law of planetary motion, also known as the law of areas, states that the line joining the planet to the sun sweeps out equal areas in equal intervals of time as the planet travels in its orbit.
Kepler’s third law:
Kepler’s third law, the law of periods, defines the relationship between the orbital period of a planet and the average radius of its orbit. The orbital period of a planet, denoted by T, is the time taken by the planet to make a complete revolution around the sun along its orbit.
The average radius of the orbit of a planet is also the mean distance of the planet from the sun. The law of periods states that the square of the orbital period, T, of a planet is proportional to the cube of its mean distance, R, from the sun.