Kepler's laws of planetary motion consist of three fundamental principles that describe the orbits of planets around the Sun. The first law, the Law of Ellipses, states that planets move in elliptical orbits with the Sun at one focus. The second law, the Law of Equal Areas, asserts that a line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time, meaning planets move faster when closer to the Sun. The third law, the Law of Harmonies, establishes a relationship between the period of a planet's orbit and its average distance from the Sun, stating that the square of the orbital period is proportional to the cube of the semi-major axis of its orbit.
Known for his eponymous laws of planetary motion.
Mindboggling? They are "Laws of Planetary Motion". So I guess the answer is "motion".
Kepler's law that describes how fast planets travel at different points in their orbits is called the Law of Equal Areas. This law states that a planet will travel faster when it is closer to the Sun and slower when it is farther away, so that the area it sweeps out in a given time is the same regardless of its distance from the Sun.
Isaac Newton
April 27, 4977 B.C. That was when he once calculated that the universe began. Or, you may mean when he published his Laws of Planetary Motion. He published his first 2 laws in 1609 and his 3rd law around 1619.
newton first law of motion newton second law of motion newton third law of motion newton gravitation law of motion
Distance from the body and the mass of the body. See Keplers laws of planetary motion for more info.
# Linear # Reciprocating # Oscillating # Rotary
Isaac Newton, he discovered: -Newton's First Law of motion. -Newton's Second Law of motion. -Newton's Third Law of motion.
In Kepler's laws of planetary motion, m1 and m2 represent the masses of two objects (usually the Sun and a planet) that are orbiting around each other. Kepler's laws describe the relationship between the orbit of a planet and the mass of the objects involved.
Kepler's Third Law, also known as the Harmonic Law, states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
The three laws of motion are: The Law of Inertia The Law of Acceleration and The Law of Interaction.