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A ball A of mass m falls on the surface ...

A ball A of mass m falls on the surface of the earth from infinity. Another ball B of mass 2m falls on the earth from the height equal to six times the radius of the earth. Then ratio of velocities of A and B on reaching the earth is `sqrt(x//y)` where x and y are coprimes. Find x+y .

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To solve the problem, we need to find the velocities of two balls A and B just before they reach the surface of the Earth and then determine the ratio of these velocities. ### Step 1: Calculate the velocity of ball A Ball A of mass \( m \) falls from infinity. We can use the conservation of mechanical energy to find its velocity just before it hits the Earth. - **Initial Energy (at infinity)**: - Potential Energy (PE) = 0 (since it is at infinity) - Kinetic Energy (KE) = 0 (since it starts from rest) - **Final Energy (just before hitting the Earth)**: - Potential Energy (PE) = \( -\frac{GMm}{R} \) (where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( R \) is the radius of the Earth) - Kinetic Energy (KE) = \( \frac{1}{2} mv_A^2 \) Using conservation of energy: \[ \text{Initial Energy} = \text{Final Energy} \] \[ 0 = -\frac{GMm}{R} + \frac{1}{2} mv_A^2 \] Rearranging gives: \[ \frac{1}{2} mv_A^2 = \frac{GMm}{R} \] Dividing by \( m \) and multiplying by 2: \[ v_A^2 = \frac{2GM}{R} \] Thus, \[ v_A = \sqrt{\frac{2GM}{R}} \] ### Step 2: Calculate the velocity of ball B Ball B of mass \( 2m \) falls from a height of \( 6R \) (which is 6 times the radius of the Earth). - **Initial Energy (at height \( 6R \))**: - Potential Energy (PE) = \( -\frac{GM(2m)}{7R} \) (the distance from the center of the Earth is \( 7R \)) - Kinetic Energy (KE) = 0 (since it starts from rest) - **Final Energy (just before hitting the Earth)**: - Potential Energy (PE) = \( -\frac{GM(2m)}{R} \) - Kinetic Energy (KE) = \( \frac{1}{2} (2m) v_B^2 \) Using conservation of energy: \[ \text{Initial Energy} = \text{Final Energy} \] \[ -\frac{GM(2m)}{7R} = -\frac{GM(2m)}{R} + \frac{1}{2} (2m) v_B^2 \] Rearranging gives: \[ -\frac{GM(2m)}{7R} + \frac{GM(2m)}{R} = mv_B^2 \] Finding a common denominator: \[ \frac{-2GM}{7R} + \frac{14GM}{7R} = mv_B^2 \] This simplifies to: \[ \frac{12GM}{7R} = mv_B^2 \] Dividing by \( m \): \[ v_B^2 = \frac{12GM}{7R} \] Thus, \[ v_B = \sqrt{\frac{12GM}{7R}} \] ### Step 3: Calculate the ratio of velocities Now we can find the ratio of the velocities \( \frac{v_A}{v_B} \): \[ \frac{v_A}{v_B} = \frac{\sqrt{\frac{2GM}{R}}}{\sqrt{\frac{12GM}{7R}}} \] This simplifies to: \[ \frac{v_A}{v_B} = \sqrt{\frac{2GM}{R} \cdot \frac{7R}{12GM}} = \sqrt{\frac{14}{12}} = \sqrt{\frac{7}{6}} \] ### Step 4: Identify \( x \) and \( y \) Here, \( x = 7 \) and \( y = 6 \). Since 7 and 6 are coprime, we can find \( x + y \): \[ x + y = 7 + 6 = 13 \] ### Final Answer Thus, the final answer is \( 13 \).

To solve the problem, we need to find the velocities of two balls A and B just before they reach the surface of the Earth and then determine the ratio of these velocities. ### Step 1: Calculate the velocity of ball A Ball A of mass \( m \) falls from infinity. We can use the conservation of mechanical energy to find its velocity just before it hits the Earth. - **Initial Energy (at infinity)**: - Potential Energy (PE) = 0 (since it is at infinity) - Kinetic Energy (KE) = 0 (since it starts from rest) ...
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