Correct Answer - Option 2 : 4 ∶ 1
Concept:
Terminal velocity:
- If a spherical body of radius r is dropped in a viscous fluid, it is first accelerated, and then its acceleration becomes zero and it attains a constant velocity called terminal velocity.
- The terminal velocity is given as,
\(⇒ v=\frac{2r^2(ρ-σ)}{9η}\)
Where v = terminal velocity, r = radius, ρ = density of the body, σ = density of liquid, g = gravitational acceleration, and η = viscosity
Calculation:
- We know that the terminal velocity is given as,
\(⇒ v=\frac{2r^2(ρ-σ)}{9η}\)
If all quantities other than r is constant, then,
⇒ v ∝ r2
or
r2 ∝ v
⇒ r
2 = k v -- (1)
Here, k is constant.
So, if for radius r1 the terminal velocity is v1, and for radius r2 the terminal velocity is v2 then we can say
\(\frac{(r_1)^2}{(r_2)^2} = \frac{v_1}{v_2}\) -- (2)
Given, the ratio of radii is 2: 1
\(\frac{(r_1)}{(r_2)} = \frac{2}{1}\) -- (3)
Putting (3) in (2)
\(\frac{(2)^2}{(1)^2} = \frac{v_1}{v_2}\)
\(\implies \frac{4}{1} = \frac{v_1}{v_2}\)
So, the ratio of velocities is 4 : 1.
The correct option is 4 : 1.