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Question: The earth, radius \(6400 \mathrm{km}\)makes one revolution about its own axis in 24 hours. The centr...

The earth, radius 6400km6400 \mathrm{km}makes one revolution about its own axis in 24 hours. The centripetal acceleration of a point on its equator is nearly.
A. 340cmsec2340\dfrac{\text{cm}}{\text{se}{{\text{c}}^{2}}}
B. 3.4cmsec23.4\dfrac{cm}{se{{c}^{2}}}
C. 34cmsec234\dfrac{\text{cm}}{\text{se}{{\text{c}}^{2}}}
D. 0.34cmsec20.34\dfrac{\text{cm}}{\text{se}{{\text{c}}^{2}}}

Explanation

Solution

We know that a centripetal force is a force that makes a body follow a curved path. The direction is always orthogonal to the motion of the body and towards the fixed point of the instantaneous centre or curvature of the path. It is a force which is necessary to keep an object moving in a curved path and that is directed inward toward the centre of rotation of a string on the end of which a stone is whirled about exerts centripetal force on the force. Based on this concept we have to answer this question.

Complete step by step answer:
The time period of earth's rotation or the time that the earth takes to rotate around its own axis is,
T=24h=86400sT=24\text{h}=86400\text{s}
We know that the angular velocity ω=2π/T\omega=2 \pi / \mathrm{T}
Radius of the earth is represented as r=6400km=640000m\mathrm{r}=6400 \mathrm{km}=640000 \mathrm{m}
Now, we can equate the centripetal acceleration as ω2r=(2π)T2r=0.034m/s2\omega 2\text{r}=\dfrac{(2\pi )}{\text{T}}2\text{r}=0.034\text{m}/{{\text{s}}^{2}}.
Therefore, the total centripetal acceleration of a point on Earth’s equator is 3.4cmsec23.4\dfrac{cm}{se{{c}^{2}}}.

Hence, the correct answer is Option B.

Note: We know that time period is defined as the time that is taken for one complete cycle of vibration to pass a given point. As the frequency of a wave increases, the time period of the wave decreases. Frequency and time period are in a reciprocal relationship that can be expressed mathematically as T = 1 / f.
The rotation period is calculated using the formula rotation period = rotation speed divided by the planet’s circumference, where the circumference is the pi times the diameter.