explain laws of Keplereperler
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here are the laws of Kepler
#1. the orbit of a planet is an ellipse with the sun at one of its foci
#2. the line joining the planet and the sun sweeps equal area in equal interval of time.
#3. the cube of the mean distance of a planet from the sun is proportional to the square of its orbital period T. Or, r³/T²= constant
#1. the orbit of a planet is an ellipse with the sun at one of its foci
#2. the line joining the planet and the sun sweeps equal area in equal interval of time.
#3. the cube of the mean distance of a planet from the sun is proportional to the square of its orbital period T. Or, r³/T²= constant
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- Kepler's first law : The orbit of a planet is an ellipse with sun at one of the foci.
- Kepler's second law : The line joining the planet and the sun sweeps equal areas in equal interval of time.
- Kepler's third law : The square of the period of revolution of the planet around the sun is directly proportional the cube of the mean distance of planet from the Sun.
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