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).
A slanted object AB is placed on one side of convex lens as shown in the diagram. The image is formed on the opposite side. Angle made by the image with principal axis is: 

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.)