Q.Define terminal velocity and derive a relation for it.
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Start your 14-day free trial to unlock the full solution →Terminal velocity is reached when weight = upthrust + viscous drag; for a sphere it works out to v_t = 2 r^2 g (rho - sigma) / (9 eta).
Definition: When a small solid body (e.g. a sphere) falls through a viscous fluid, it initially accelerates under gravity, but as its speed increases, the opposing viscous drag force (given by Stokes' law) also increases. Eventually the net force on the body becomes zero, and it continues to fall with a constant maximum velocity -- this constant velocity is called the terminal velocity.
Derivation:
Consider a small sphere of radius r and density rho falling through a fluid of density sigma and coefficient of viscosity eta. Three forces act on the sphere as it falls:
- Weight (downward): W = (4/3) pi r^3 rho g
- Upthrust / buoyant force (upward, by Archimedes' principle): U = (4/3) pi r^3 sigma g
- Viscous drag force (upward, opposing motion, by Stokes' law): F = 6 pi eta r v
At terminal velocity v_t, the net force is zero, so the downward weight equals the sum of the upward forces:
W = U + F
(4/3) pi r^3 rho g = (4/3) pi r^3 sigma g + 6 pi eta r v_t
Rearranging:
(4/3) pi r^3 g (rho - sigma) = 6 pi eta r v_t
Solving for v_t:
v_t = [ (4/3) pi r^3 g (rho - sigma) ] / (6 pi eta r)
v_t = [ 4 r^2 g (rho - sigma) ] / (18 eta) …
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