In short, the three laws of planetary motion can be given as follows: (1) Planets move in ellipses with the sun at one focus; (2) The radius vector describes equal areas in equal times; and (3) The squares of the periodic times are to each other as the cubes of the mean distances.
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Explanation:
three laws
In short, the three laws of planetary motion can be given as follows: (1) Planets move in ellipses with the sun at one focus; (2) The radius vector describes equal areas in equal times; and (3) The squares of the periodic times are to each other as the cubes of the mean distances.
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