Analyzing the Setup
Imagine a parallel beam of light traveling from the left and striking the first convex lens, L1.
We know from the fundamental principles of optics that a convex lens converges parallel rays to its focal point.
Therefore, the first lens will focus these rays at a point F1, which is located at a distance f1 from the optical center of L1. Since L1 is at the origin (0,0), the coordinates of this intermediate focal point F1 are simply (f1,0).
The Virtual Object
Before these converging rays can actually meet at F1, they are intercepted by the second lens, L2.
This is where the concept of a virtual object comes into play. The point F1 acts as a virtual object for L2.
We are given that L2 is placed at a horizontal distance d from L1. Therefore, the distance of this virtual object from L2 is (f1−d).
According to our sign convention, since the incident light travels to the right and the virtual object is also to the right of L2, the object distance u is positive.
Calculating the x-coordinate
Now, we apply the thin lens formula for the second lens to find the final image distance v.
Substituting our value for u, we get:
Rearranging to solve for v:
v1=f21+f1−d1=f2(f1−d)f1−d+f2
Inverting this expression gives us the image distance from L2:
To find the absolute x-coordinate from the origin O, we must add the position of L2 (which is d) to the image distance v.
x=d+v=d+f1+f2−df2(f1−d)
Taking the common denominator and simplifying:
x=f1+f2−dd(f1+f2−d)+f2(f1−d)=f1+f2−df1f2+d(f1−d)
The Masterstroke
The y-coordinate
This is the part where many students make a mistake. We must carefully consider the reference frames.
The second lens L2 is shifted vertically by a distance Δ. This means its principal axis is the line y=Δ.
Our virtual object F1 lies on the x-axis, which is y=0. Therefore, relative to the principal axis of L2, the object is located at a depth of Δ.
This gives us our object height, yobj=−Δ.
To find the final image height, we need the transverse magnification m of the second lens.
m=uv=f1−df1+f2−df2(f1−d)=f1+f2−df2
The image height relative to the principal axis of L2 is simply the magnification times the object height.
Finally, to find the absolute y-coordinate from the origin, we must add this relative image height to the height of L2's principal axis.
Substituting our expression for m:
y=Δ(1−f1+f2−df2)=Δ(f1+f2−df1+f2−d−f2)
And there we have it! The complete coordinates of the final focal point.