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Zorluk: Çok zorFluids at Rest, Archimedes' Principle and Viscosity

A spherical particle of radius 3.0×103 m3.0 \times 10^{-3}\text{ m} and density 8.0×103 kg/m38.0 \times 10^3\text{ kg/m}^3 is released from rest and falls vertically through a tall column of a viscous liquid of density 2.0×103 kg/m32.0 \times 10^3\text{ kg/m}^3. If the coefficient of viscosity of the fluid is 0.40 Pas0.40\text{ Pa}\cdot\text{s} and the acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2, calculate the magnitude of its terminal velocity in m/s\text{m/s}.

Cevap: 0.3 m/s

Cevap

The magnitude of the terminal velocity of the falling sphere is 0.3 m/s0.3\text{ m/s}.
When a body falls at terminal velocity through a viscous medium, its weight is balanced by the sum of buoyancy upthrust and Stokes' viscous drag force. Applying vt=2r2(ρsρf)g9ηv_t = \frac{2 r^2 (\rho_s - \rho_f) g}{9 \eta} with sphere radius r=0.003 mr = 0.003\text{ m}, sphere density ρs=8000 kg/m3\rho_s = 8000\text{ kg/m}^3, fluid density ρf=2000 kg/m3\rho_f = 2000\text{ kg/m}^3, viscosity η=0.40 Pas\eta = 0.40\text{ Pa}\cdot\text{s}, and g=10 m/s2g = 10\text{ m/s}^2 yields vt=0.3 m/sv_t = 0.3\text{ m/s}.

Adım Adım Çözüm

1
Formulate the dynamic equilibrium condition at terminal velocity.
At terminal velocity, the net acceleration is zero, leading to the force balance equation W=U+FvW = U + F_v, where WW is the gravitational weight of the sphere, UU is the buoyant upthrust, and FvF_v is the retarding viscous force.
Terminal velocity occurs when the downward force of gravity is precisely balanced by the sum of upward resistive and buoyancy forces.
2
Substitute algebraic expressions for weight, upthrust, and Stokes' viscous drag.
W=43πr3ρsgW = \frac{4}{3}\pi r^3 \rho_s g, U=43πr3ρfgU = \frac{4}{3}\pi r^3 \rho_f g, and Fv=6πηrvtF_v = 6\pi \eta r v_t.
Archimedes' principle defines the upthrust force equal to the weight of displaced liquid, while Stokes' law governs viscous resistance on spherical bodies.
3
Solve the equilibrium equation for terminal velocity vtv_t.
vt=2r2(ρsρf)g9ηv_t = \frac{2 r^2 (\rho_s - \rho_f) g}{9 \eta}.
Equating 43πr3(ρsρf)g=6πηrvt\frac{4}{3}\pi r^3 (\rho_s - \rho_f) g = 6\pi \eta r v_t and simplifying cancels common factors of π\pi and rr.
4
Substitute the specified numerical parameters into the derived expression.
vt=2×(3.0×103)2×(80002000)×109×0.40=2×9.0×106×6000×103.6=1.083.6=0.3 m/sv_t = \frac{2 \times (3.0 \times 10^{-3})^2 \times (8000 - 2000) \times 10}{9 \times 0.40} = \frac{2 \times 9.0 \times 10^{-6} \times 6000 \times 10}{3.6} = \frac{1.08}{3.6} = 0.3\text{ m/s}.
Direct calculation yields the exact value of terminal velocity.

Anahtar Kavram

Terminal Velocity, Stokes' Law, and Archimedes' Principle
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