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Question
The difference in the acceleration due to gravity at the pole and equator is ______.
(g = acceleration due to gravity, R = radius of the earth; θ = latitude, ω = angular velocity, cos0° = 1, cos90° = 0)
Options
`(Romega^2)/g^2`
Rω2 cos2θ
Rω2
ωcos2θ
MCQ
Fill in the Blanks
Solution
The difference in the acceleration due to gravity at the pole and equator is Rω2.
Explanation:
The value of acceleration due to gravity due to the rotation of the Earth,
g' = g - ω2Rcos2λ
At poles, λ = 90°
∴ `g_p = g - omega^2Rcos^2 90^circ = g`
At equator, λ = 0°
∴ `g_e = g - omega^2Rcos^2 0^circ = g - omega^2R`
∴ `g_p - g_e = g - g + Romega^2 = Romega^2`
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