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According to Kepler's Third Law of Planetary Motion, the square of a planet's orbital period (T) is directly proportional to the cube of the semi-major axis (a) of its orbit. This can be expressed mathematically as ( T^2 \propto a^3 ). Essentially, this means that planets that are farther from the Sun take longer to orbit than those that are closer, with the relationship providing a precise way to compare their orbital periods and distances.

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According to the three laws of planetary motion planetary orbits are in the shape of an?

According to Kepler's laws of planetary motion, planetary orbits are in the shape of an ellipse with the Sun at one of the foci.


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Mindboggling? They are "Laws of Planetary Motion". So I guess the answer is "motion".


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According to Kepler's laws of planetary motion, its distance from the sun.


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Rotation and revolution. Gravity and Inertia. See Kepler's Law of Planetary motion.


How many laws of planetary motion did Johannes Kepler discover?

3 laws' of planetary motion


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Keplar figured out the laws of planetary motion using Tycho Brahe's data.


What is the similarities do the movements of the planets share?

They all obey Kepler's 3 laws of planetary motion.


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Yes, the distance of a planet from the sun affects its period of revolution. According to Kepler's third law of planetary motion, planets that are closer to the sun have shorter revolution periods compared to planets that are farther away.


How is Keppler related to Solar System?

Well, seeing as he was a Mathematician and Astronomer, he is closely related to the Solar System. During the Scientific Revolution of the 17th century Johannes Kepler discovered and documented the laws of planetary motion. His studies also laid the groundwork for Isaac Newton's theory of universal gravitation.


Who discovered the planetary motion?

Johannes Kepler


What did Kepler formulate?

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What planetary motion determines length of year?

The length of a year is determined by the Earth's orbital motion around the Sun. Specifically, it takes approximately 365.25 days for the Earth to complete one full revolution around the Sun, which defines the length of a year. This orbital period is influenced by gravitational forces and the elliptical shape of Earth's orbit, as described by Kepler's laws of planetary motion.