Question

state the capiler's law of planetery motion in detail.​

Answer 1

Answer:

Kepler's three laws of planetary motion can be stated as follows: (1) All planets move about the Sun in elliptical orbits, having the Sun as one of the foci. ... (3) The squares of the sidereal periods (of revolution) of the planets are directly proportional to the cubes of their mean distances from the Sun.

Answer 2

it tells us that the square of the time taken by a body revolving around another is directly proportional to the cube of the distance covered by that body around another one (in this case, the sun). The equation goes like this:

t2 α r3

in order to remove proportionality, we multiply the R.H.S. by a constant, K so that we get:

t2 = Kr3