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The terminal velocity of a sphere moving...

The terminal velocity of a sphere moving through a viscous medium is :

A

directly proportional to the radius of the sphere

B

inversely proportional to the radius of the sphere

C

directly propotional to the square of the radius of sphere

D

inversely propotional to the square of the radius of sphere

Text Solution

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The correct Answer is:
To find the relationship between the terminal velocity of a sphere moving through a viscous medium and its radius, we can derive the formula for terminal velocity and analyze the dependencies. ### Step-by-Step Solution: 1. **Understanding Terminal Velocity**: Terminal velocity is the constant speed that a freely falling object eventually reaches when the resistance of the medium prevents further acceleration. For a sphere falling through a viscous fluid, the forces acting on it are gravity and drag force. 2. **Forces Acting on the Sphere**: - **Weight of the Sphere (W)**: The weight can be expressed as \( W = V \cdot \rho \cdot g \), where \( V \) is the volume of the sphere, \( \rho \) is the density of the fluid, and \( g \) is the acceleration due to gravity. - **Drag Force (F_d)**: The drag force acting on the sphere can be expressed using Stokes' law as \( F_d = 6 \pi \eta r v \), where \( \eta \) is the viscosity of the fluid, \( r \) is the radius of the sphere, and \( v \) is the velocity of the sphere. 3. **Setting Up the Equation**: At terminal velocity, the drag force equals the weight of the sphere: \[ V \cdot \rho \cdot g = 6 \pi \eta r v_t \] where \( v_t \) is the terminal velocity. 4. **Volume of the Sphere**: The volume \( V \) of the sphere is given by: \[ V = \frac{4}{3} \pi r^3 \] Substituting this into the weight equation gives: \[ \frac{4}{3} \pi r^3 \cdot \rho \cdot g = 6 \pi \eta r v_t \] 5. **Simplifying the Equation**: Canceling \( \pi \) from both sides and rearranging gives: \[ \frac{4}{3} r^3 \cdot \rho \cdot g = 6 \eta r v_t \] Dividing both sides by \( r \) (assuming \( r \neq 0 \)): \[ \frac{4}{3} r^2 \cdot \rho \cdot g = 6 \eta v_t \] 6. **Solving for Terminal Velocity**: Rearranging for \( v_t \): \[ v_t = \frac{4}{18} \cdot \frac{r^2 \cdot \rho \cdot g}{\eta} \] Simplifying further: \[ v_t = \frac{2}{9} \cdot \frac{r^2 \cdot \rho \cdot g}{\eta} \] 7. **Analyzing the Proportionality**: From the final equation, we can see that: \[ v_t \propto r^2 \] This indicates that the terminal velocity is directly proportional to the square of the radius of the sphere. ### Conclusion: Thus, the terminal velocity of a sphere moving through a viscous medium is directly proportional to the square of the radius of the sphere.
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