Use the lens equation with clean distances to solve for where the image forms.

optics The clean numbers are chosen so the reciprocal arithmetic lands exactly on a whole-number image distance.

Example

Use the lens equation with clean distances to solve for where the image forms. Exact arithmetic here means exact results for the stated model inputs; measured inputs still carry uncertainty and significant-figure limits.

highlighted = computed this step

Start with focal length and object distance

Use focal length 10 metres and object distance 15 metres. The image distance is the unknown.

f=10 mu=15 mf = 10\ \text{m}\qquad u = 15\ \text{m}
Solving image distanceChecked rays meet at the solved image point.FFlensobjectimage

A nearby object makes a farther image

With the focal length fixed, compare three object placements. Outside the focus, moving closer pushes the real image farther away; inside the focus, the sign changes and the image becomes virtual.

fuvm10 m20 m20 m110 m15 m30 m210 m5 m10 m2\begin{array}{c|c|c|c}f&u&v&m\\10\ \text{m}&20\ \text{m}&20\ \text{m}&-1\\10\ \text{m}&15\ \text{m}&30\ \text{m}&-2\\10\ \text{m}&5\ \text{m}&-10\ \text{m}&2\\\end{array}
Solving image distanceThe table compares distances while this ray case is checked.FFlensobjectimage

Subtract the reciprocals

The focal reciprocal minus the object reciprocal gives the image reciprocal.

1v=110 m115 m=130 1/m\frac{1}{v} = \frac{1}{10\ \text{m}} - \frac{1}{15\ \text{m}} = \tfrac{1}{30}\ 1/\text{m}

Invert the reciprocal

The reciprocal is one over 30 metres, so the image distance is 30 metres on the far side of the lens.

v=30 mv = 30\ \text{m}
Solving image distanceChecked rays meet at the solved image point.FFlensobjectimage