Step 1: The object is \(4f\) away from the first lens (\(L_1\)). Applying the lens formula: \[ \frac{1}{f} = \frac{1}{v_1} - \frac{1}{u_1} \] where \(u_1 = -4f\) and \(v_1\) is the image distance from \(L_1\), we find \(v_1\): \[ \frac{1}{f} = \frac{1}{v_1} + \frac{1}{4f} \] \[ \frac{1}{v_1} = \frac{1}{f} - \frac{1}{4f} = \frac{3}{4f} \] Thus, \[ v_1 = \frac{4f}{3} \] The image from \(L_1\) is \(\frac{4f}{3}\) to the right of \(L_1\).
Step 2: This image is the object for the second lens (\(L_2\)). The lenses are \(\frac{f}{2}\) apart, so the object distance for \(L_2\) is: \[ u_2 = \frac{4f}{3} - \frac{f}{2} = \frac{8f}{6} - \frac{3f}{6} = \frac{5f}{6} \] Applying 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 \(v_2\): \[ \frac{1}{f} = \frac{1}{v_2} - \frac{6}{5f} \] \[ \frac{1}{v_2} = \frac{1}{f} + \frac{6}{5f} = \frac{11}{5f} \] Therefore, \[ v_2 = \frac{5f}{11} \] The final image is \(\frac{5f}{11}\) to the right of \(L_2\).