Define all capler's law of planetary motion in a detailed way.
Anonymous:
its Kepler's laws
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mainly thats not capler it is kepler...
1st law --
The orbit of the planet towards sun is in oval or elliptical in shape.
2nd law --
if a planet covers a distance of A to B in particular time (i. e-24hours) and a same distance and time in other position of C to D, then the both areas formed as a cone are equal. (join sun to A and to B and same as C to D in a elipt).
3rd law --
The cube of the average or (mean) distance from the sun to the planet is proportional to the square of its orbital period. (d^2/T^2).{here" T" denotes proportionality constant.}
1st law --
The orbit of the planet towards sun is in oval or elliptical in shape.
2nd law --
if a planet covers a distance of A to B in particular time (i. e-24hours) and a same distance and time in other position of C to D, then the both areas formed as a cone are equal. (join sun to A and to B and same as C to D in a elipt).
3rd law --
The cube of the average or (mean) distance from the sun to the planet is proportional to the square of its orbital period. (d^2/T^2).{here" T" denotes proportionality constant.}
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