Question:

Assume the earth's orbit around the sun as circular and the distance between their centers as 'D' mass of the earth is 'M' and its radius is 'R' If earth has an angular velocity $'\omega_0'$ with respect to its center and $'\omega'$ with respect to the center of the sun, the total kinetic energy of the earth is:

Updated On: Jul 6, 2022
  • $\frac{MR^2\omega^2_0}{5}\left[1+\left(\frac{\omega}{\omega_0}\right)+\frac{5}{2}\left(\frac{D\omega}{R\omega_0}\right)^2\right]$
  • $\frac{MR^2\omega^2_0}{5}\left[1+\frac{5}{2}\left(\frac{D\omega}{R\omega_0}\right)^2\right]$
  • $\frac{2}{5}MR^2\omega^2_0\left[1+\frac{5}{2}\left(\frac{D\omega}{R\omega_0}\right)^2\right]$
  • $\frac{2}{5}MR^2\omega^2_0\left[1+\left(\frac{\omega}{\omega_0}\right)+\frac{5}{2}\left(\frac{D\omega}{R\omega_0}\right)^2\right]$
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The Correct Option is A

Solution and Explanation

Total kinetic energy = $\frac{1}{2} \, I \, \omega^2_0 + \frac{1}{2} m \nu^2 + \frac{1}{2} I \, \omega^2$ $\frac{1}{2} \left[ \frac{2}{5} MR^2\right] \omega_0^2 + \frac{1}{2}MD^2\omega^2 + \frac{1}{2} \left[ \frac{2}{5} MR^2 \right] \omega^2$ = $\frac{MR^2 \omega^2_0}{5} \left[ 1 + \frac{\omega^2}{\omega_0^2} + \frac{5}{2} \frac{D^2 \omega^2}{R^2 \omega^2_0} \right]$ (or) $\frac{MR^2 \omega^2_0}{5} \left[ 1 + \frac{5}{2} \left( \frac{D^2 \omega^2}{R^2 \omega^2_0}\right) \right]$
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Concepts Used:

Gravitational Potential Energy

The work which a body needs to do, against the force of gravity, in order to bring that body into a particular space is called Gravitational potential energy. The stored is the result of the gravitational attraction of the Earth for the object. The GPE of the massive ball of a demolition machine depends on two variables - the mass of the ball and the height to which it is raised. There is a direct relation between GPE and the mass of an object. More massive objects have greater GPE. Also, there is a direct relation between GPE and the height of an object. The higher that an object is elevated, the greater the GPE. The relationship is expressed in the following manner:

PEgrav = mass x g x height

PEgrav = m x g x h

Where,

m is the mass of the object,

h is the height of the object

g is the gravitational field strength (9.8 N/kg on Earth) - sometimes referred to as the acceleration of gravity.