Step 1: For the first lens (\(L_1\)), the object is placed at \(4f\) from \(L_1\). Using the lens formula: \[ \frac{1}{f} = \frac{1}{v_1} - \frac{1}{u_1} \] where \(u_1 = -4f\) (object distance for \(L_1\)) and \(v_1\) is the image distance from \(L_1\), we solve for \(v_1\): \[ \frac{1}{f} = \frac{1}{v_1} + \frac{1}{4f} \] \[ \frac{1}{v_1} = \frac{1}{f} - \frac{1}{4f} = \frac{3}{4f} \] So, \[ v_1 = \frac{4f}{3} \] The image formed by \(L_1\) is located \(\frac{4f}{3}\) to the right of \(L_1\).
Step 2: This image acts as the object for the second lens (\(L_2\)). The distance between the two lenses is \(\frac{f}{2}\), so the object for \(L_2\) is at a distance: \[ u_2 = \frac{4f}{3} - \frac{f}{2} = \frac{8f}{6} - \frac{3f}{6} = \frac{5f}{6} \] Now, using the lens formula for \(L_2\): \[ \frac{1}{f} = \frac{1}{v_2} - \frac{1}{u_2} \] where \(u_2 = \frac{5f}{6}\) and \(v_2\) is the image distance for \(L_2\), we solve for \(v_2\): \[ \frac{1}{f} = \frac{1}{v_2} - \frac{6}{5f} \] \[ \frac{1}{v_2} = \frac{1}{f} + \frac{6}{5f} = \frac{11}{5f} \] So, \[ v_2 = \frac{5f}{11} \] Therefore, the final image is at a distance of \(\frac{5f}{11}\) to the right of \(L_2\).