state Newton law of gravitation by using keplar's third law
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Kepler's Third Law can be written as
P2 = kr3
or P2 = (4π2/GM).r3 (1)
now, we know that the time period, P = 2πr/v, so (1) becomes
(2πr/v)2 = (4π2/GM).r3
or 4π2 (r/v)2 = (4π2/GM).r3
or (r/v)2 = (1/GM).r3 = r3/GM (2)
we know that,
centripetal acceleration a = v2/r [from ma = mv2/r]
thus, equation (2) becomes
r/a = r3/GM
or 1/a = r2/GM
or a = GM/r2 (3)
and we also know that F = ma, thus using equation (3) we would get
F = ma = m(GM/r2)
thus, we have derived the Newton's Law of Gravitation, which is
F = GMm/r2
from Kepler's Third Law
P2 = kr3
or P2 = (4π2/GM).r3 (1)
now, we know that the time period, P = 2πr/v, so (1) becomes
(2πr/v)2 = (4π2/GM).r3
or 4π2 (r/v)2 = (4π2/GM).r3
or (r/v)2 = (1/GM).r3 = r3/GM (2)
we know that,
centripetal acceleration a = v2/r [from ma = mv2/r]
thus, equation (2) becomes
r/a = r3/GM
or 1/a = r2/GM
or a = GM/r2 (3)
and we also know that F = ma, thus using equation (3) we would get
F = ma = m(GM/r2)
thus, we have derived the Newton's Law of Gravitation, which is
F = GMm/r2
from Kepler's Third Law
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