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Derive the expression for terminal velocity for a sphere falling through a viscous fluid.

Physics

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Answer

vt=2r2(ρ−σ)g9ηv_t = \frac{2 r^2 (\rho - \sigma) g}{9 \eta}

Step-by-step solution

4 steps

Definition of Terminal Velocity:
Terminal velocity is the constant maximum velocity attained by an object falling through a fluid when the net force acting on it becomes zero. This occurs when the sum of the upward forces (buoyant force and viscous drag force) equals the downward force (gravitational force).

Expression for Terminal Velocity:
Consider a spherical object of radius rr and density ρ\rho falling through a viscous liquid of density σ\sigma and coefficient of viscosity η\eta.

  1. Identify the forces acting on the sphere.

    • Gravitational force (FgF_g) acting downwards: Fg=mg=(volume of sphere)×(density of sphere)×gF_g = mg = (\text{volume of sphere}) \times (\text{density of sphere}) \times g Fg=43πr3ρgF_g = \frac{4}{3}\pi r^3 \rho g
    • Buoyant force (FbF_b) acting upwards (by Archimedes' principle): Fb=(volume of sphere)×(density of liquid)×gF_b = (\text{volume of sphere}) \times (\text{density of liquid}) \times g Fb=43πr3σgF_b = \frac{4}{3}\pi r^3 \sigma g
    • Viscous drag force (FvF_v) acting upwards (by Stokes' Law): Fv=6πηrvF_v = 6\pi \eta r v where vv is the instantaneous velocity of the sphere.
  2. Apply Newton's second law.

    The net force on the sphere is Fnet=Fg−Fb−FvF_{net} = F_g - F_b - F_v.

    ma=43πr3ρg−43πr3σg−6πηrvma = \frac{4}{3}\pi r^3 \rho g - \frac{4}{3}\pi r^3 \sigma g - 6\pi \eta r v mdvdt=43πr3(ρ−σ)g−6πηrvm \frac{dv}{dt} = \frac{4}{3}\pi r^3 (\rho - \sigma) g - 6\pi \eta r v
  3. Determine terminal velocity.

    When the sphere reaches terminal velocity (vtv_t), its acceleration becomes zero (a=0a = 0). At this point, the net force is zero, meaning the upward forces balance the downward force.

    Fg=Fb+FvF_g = F_b + F_v 43πr3ρg=43πr3σg+6πηrvt\frac{4}{3}\pi r^3 \rho g = \frac{4}{3}\pi r^3 \sigma g + 6\pi \eta r v_t
  4. Solve for vtv_t.

    Rearrange the equation to isolate vtv_t:

    6πηrvt=43πr3ρg−43πr3σg6\pi \eta r v_t = \frac{4}{3}\pi r^3 \rho g - \frac{4}{3}\pi r^3 \sigma g 6πηrvt=43πr3(ρ−σ)g6\pi \eta r v_t = \frac{4}{3}\pi r^3 (\rho - \sigma) g

    Divide both sides by 6πηr6\pi \eta r:

    vt=4πr3(ρ−σ)g3×6πηrv_t = \frac{4\pi r^3 (\rho - \sigma) g}{3 \times 6\pi \eta r} vt=4πr3(ρ−σ)g18πηrv_t = \frac{4\pi r^3 (\rho - \sigma) g}{18\pi \eta r}

    Simplify the expression:

    vt=2r2(ρ−σ)g9η\boxed{v_t = \frac{2 r^2 (\rho - \sigma) g}{9 \eta}}

    Graphical Variation of Velocity with Time:
    When an object is dropped in a viscous fluid, its velocity initially increases from zero. As the velocity increases, the viscous drag force also increases, which reduces the net accelerating force. Consequently, the acceleration decreases over time. Eventually, the sum of the upward buoyant force and viscous drag force equals the downward gravitational force. At this point, the net force becomes zero, acceleration becomes zero, and the object attains a constant maximum velocity called the terminal velocity (vtv_t).

    The graph of velocity (vv) versus time (tt) shows an exponential increase in velocity from zero, which then levels off to a constant value (terminal velocity) as time progresses.

    Velocity
      ^
      |      /
      |     /
      |    /
      |   /
      |  /
      | /
      |/_________________ Terminal Velocity (v_t)
      |
      +----------------------> Time
      0
    
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