How does kepler law help newton to arrive at the inverse square law of gravity?
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For a uniform circular orbit of radius r, the acceleration is
a = ω2r, ω = 2π/T________(A)
where T is the orbital period. Comparing eq. (A) with Kepler's third law
T2 ∝ r3______________(B)
we conclude that the gravitational acceleration
a ∝ r−2________________(C)
is proportional to the inverse square distance r
a = ω2r, ω = 2π/T________(A)
where T is the orbital period. Comparing eq. (A) with Kepler's third law
T2 ∝ r3______________(B)
we conclude that the gravitational acceleration
a ∝ r−2________________(C)
is proportional to the inverse square distance r
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Kepler law help Newton to arrive at the inverse square law of gravity
Explanation:
Johannes Kepler studied about the planets motion and their positions and. ... Kepler's Third law: The Square of its period of revolution around the Sun is directly proportional to the cube of the mean distance of a planet from the Sun. Have a look on attachment
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