Question
Question: Due to rotation of the earth the direction of vertical at a place is not along the radius of the ear...
Due to rotation of the earth the direction of vertical at a place is not along the radius of the earth and actually makes a small angle ϕ with the true vertical (i.e. with radius). At hat latitude Θ is this angle ϕ maximum?

0
30
45
60
45^\circ
Solution
The effective acceleration due to gravity (geff) at a latitude Θ is the vector sum of the true gravitational acceleration (g0, directed towards the Earth's center) and the centrifugal acceleration (ac, directed outwards from the axis of rotation).
The true vertical is along the direction of g0. The apparent vertical is along the direction of geff. The angle ϕ is between these two directions.
Let's resolve geff into components along the true vertical and true horizontal.
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True Gravitational Acceleration (g0): Acts radially inwards, magnitude g0.
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Centrifugal Acceleration (ac): Magnitude ac=ω2RcosΘ, where R is Earth's radius and ω is its angular velocity. This force acts outwards from the axis of rotation.
- The component of ac along the true horizontal (tangent to the surface, towards the equator) is geff,H=acsinΘ=ω2RcosΘsinΘ.
- The component of ac along the true vertical (radially outwards) is accosΘ=ω2Rcos2Θ. This component acts opposite to g0.
The effective components of acceleration are:
- Horizontal component: geff,H=ω2RsinΘcosΘ.
- Vertical component: geff,V=g0−ω2Rcos2Θ.
The angle ϕ between the apparent vertical and the true vertical is given by:
tanϕ=geff,Vgeff,H=g0−ω2Rcos2Θω2RsinΘcosΘTo find the latitude Θ where ϕ (and thus tanϕ) is maximum, we differentiate this expression with respect to Θ and set it to zero.
Let K=g0ω2R. Since g0≫ω2R, K is a small quantity.
tanϕ=1−Kcos2ΘKsinΘcosΘ=1−Kcos2Θ2Ksin(2Θ)Differentiating and setting the derivative to zero (ignoring the denominator which is never zero):
dΘd(2Ksin(2Θ))(1−Kcos2Θ)−2Ksin(2Θ)dΘd(1−Kcos2Θ)=0 Kcos(2Θ)(1−Kcos2Θ)−2Ksin(2Θ)(−K⋅2cosΘ(−sinΘ))=0 Kcos(2Θ)(1−Kcos2Θ)−K2sin(2Θ)sinΘcosΘ=0Divide by K (since K=0):
cos(2Θ)(1−Kcos2Θ)−Ksin(2Θ)sinΘcosΘ=0Substitute sin(2Θ)=2sinΘcosΘ:
cos(2Θ)(1−Kcos2Θ)−K(2sinΘcosΘ)sinΘcosΘ=0 cos(2Θ)(1−Kcos2Θ)−2Ksin2Θcos2Θ=0Substitute cos(2Θ)=2cos2Θ−1 and sin2Θ=1−cos2Θ:
(2cos2Θ−1)(1−Kcos2Θ)−2K(1−cos2Θ)cos2Θ=0Let c2=cos2Θ.
(2c2−1)(1−Kc2)−2K(1−c2)c2=0 2c2−2Kc4−1+Kc2−2Kc2+2Kc4=0 (2+K−2K)c2−1=0 (2−K)c2−1=0 c2=2−K1Since K=g0ω2R is very small (K≈0.00345), we can approximate 2−K≈2.
cos2Θ≈21 cosΘ=21This implies Θ=45∘.
The angle ϕ is maximum at a latitude of 45∘.