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NEET PHYSICSMedium

A small sphere of radius rr falls from rest in a viscous liquid. As a result, heat is produced due to the viscous force. The rate of production of heat when the sphere attains its terminal velocity is proportional to:

A

r3r^3

B

r2r^2

C

r5r^5

D

r4r^4

Step-by-Step Solution

  1. Terminal Velocity (vtv_t): When a sphere of radius rr falls through a viscous fluid, it attains a constant terminal velocity given by the formula vt=2r2(ρσ)g9ηv_t = \frac{2r^2(\rho - \sigma)g}{9\eta} . This implies that vtr2v_t \propto r^2.
  2. Viscous Force (FF): According to Stokes' Law, the viscous drag force acting on the sphere moving with terminal velocity is F=6πηrvtF = 6\pi \eta r v_t . Substituting the proportionality for vtv_t, we get Fr(r2)r3F \propto r(r^2) \propto r^3.
  3. Rate of Heat Production (Power): The rate of heat production is equal to the power (PP) dissipated by the viscous force, which is the product of the force and velocity: P=F×vtP = F \times v_t.
  4. Calculation: Substituting the proportionalities: P(r3)×(r2)P \propto (r^3) \times (r^2) Pr5P \propto r^5 Thus, the rate of heat production is proportional to the fifth power of the radius.
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