Step 1: Use the lens formula.
$\displaystyle \frac{1}{v} + \frac{1}{u} = \frac{1}{f}$, where $u<0$ for a real object.
Differentiating w.r.t. time $t$:
$\displaystyle -\frac{1}{u^2}\frac{du}{dt} - \frac{1}{v^2}\frac{dv}{dt} = 0.$
Step 2: Relate object and image velocities.
Let object velocity $V_o = -\dfrac{du}{dt}$ (positive towards the lens),
and image velocity $V_i = \dfrac{dv}{dt}$.
Then from the differentiated lens equation:
$\displaystyle \frac{V_o}{u^2} = \frac{V_i}{v^2}.$
Thus
$\displaystyle V_i = V_o \left(\frac{v}{u}\right)^2.$
Step 3: Behaviour between $2f$ and $f$.
When $f<u<2f$, the image lies beyond $2f$ on the other side and $|v| > |u|$.
So
$\displaystyle \left(\frac{v}{u}\right)^2 > 1 \;\Rightarrow\; V_i > V_o.$
Step 4: Direction.
As the object approaches the lens, the image moves away from the lens (positive $V_i$).
Step 5: Conclusion.
The image moves faster than the object and in the opposite direction:
$V_i > V_o$, moving away from the lens ⇒ option (C).
The strain-stress plot for materials A, B, C and D is shown in the figure. Which material has the largest Young's modulus? 

At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)