3.2.3 Thin Lenses – Virtual Image Formation by a Converging Lens
Learning Objective
Draw and use ray diagrams to predict the position, nature and size of a virtual image formed by a converging (convex) lens, and verify the result with the thin‑lens formula.
Key Concepts
- Converging (convex) lens: thicker at the centre than at the edges; parallel incident rays are brought to a focus on the opposite side of the lens.
- Diverging (concave) lens: thinner at the centre; parallel incident rays diverge as if they originated from a focal point on the same side as the object. Consequently a diverging lens always produces a virtual, upright, reduced image on the object side.
- Principal axis: straight line passing through the optical centre and both focal points.
- Optical centre (O): geometric centre of the lens; a ray that passes through O continues undeviated.
- Focal points (F1, F2): points on the principal axis where rays that are initially parallel to the axis appear to converge (F2) or diverge from (F1).
- Virtual image: formed when the refracted rays diverge; the image cannot be projected on a screen and is located on the same side of the lens as the object.
Sign‑Convention (Cambridge IGCSE)
| Quantity | Symbol | Sign |
| Focal length | f | + for converging, – for diverging |
| Object distance | u | + (measured from the lens to the object on the incoming‑light side) |
| Image distance | v | + for real images (opposite side), – for virtual images (same side as the object) |
| Height (object, image) | h, h′ | + if measured upwards from the principal axis |
Lens‑Maker’s Equation & Optical Power (optional)
The focal length of a thin lens is related to its radii of curvature (R1, R2) and refractive index n by
\[
\frac{1}{f}= (n-1)\left(\frac{1}{R_{1}}-\frac{1}{R_{2}}\right)
\]
The optical power \(P\) is
\[
P = \frac{1}{f}\qquad\text{(dioptres, D)}
\]
Ray‑Diagram Construction
1. Virtual Image (object placed **between** the lens and its focal point, \(0
- Draw a horizontal line – the principal axis.
- Mark the optical centre O of the lens on the axis.
- Mark the two focal points: F1 on the object side and F2 on the image side, each a distance \(|f|\) from O.
- Place the upright object (arrow) between O and F1 so that \(0
- From the top of the object draw the three principal rays:
- Parallel ray: travels parallel to the principal axis, strikes the lens and **appears to diverge from F1** after refraction. (Extend the refracted ray backwards; it meets the other ray at the virtual image.)
- Focal ray: aimed toward the focal point on the image side (F2); after refraction it emerges **parallel to the principal axis**.
- Central ray: passes straight through the optical centre O without deviation.
- Extend the refracted rays **backwards** (i.e. behind the lens on the object side) until they intersect. The intersection point is the virtual image.
- Label the image:
- Upright (same orientation as the object).
- Magnified if the object is close to the lens; the magnification decreases as the object approaches the focal point.
- Located on the same side of the lens as the object, between the lens and F1.
2. Real Image (object placed **beyond** the focal point, \(u>f\)) – quick reference
- Object is to the right of F1 (i.e. \(u>f\)).
- Ray behaviour:
- Parallel ray: after refraction passes through the **near** focal point F1.
- Focal ray: aimed toward F1 before the lens; after refraction it emerges parallel to the principal axis.
- Central ray: passes undeviated through O.
- The refracted rays actually meet on the opposite side of the lens – this point is a real, inverted image.
Worked Example (Virtual Image)
Given a converging lens with \(f = +10\;\text{cm}\) and an object placed \(u = 6\;\text{cm}\) from the lens (i.e. \(u < f\)), find the image distance \(v\) and the magnification \(m\).
| Quantity | Symbol | Value | Sign (IGCSE) |
| Focal length | f | +10 cm | Positive (converging) |
| Object distance | u | +6 cm | Positive (object side) |
| Image distance | v | ? | Negative for a virtual image |
Thin‑lens equation (IGCSE sign convention)
\[
\frac{1}{f}= \frac{1}{v}+ \frac{1}{u}
\qquad\Longrightarrow\qquad
\frac{1}{v}= \frac{1}{f}-\frac{1}{u}
\]
Substituting the numbers
\[
\frac{1}{v}= \frac{1}{10}-\frac{1}{6}= \frac{3-5}{30}= -\frac{2}{30}= -\frac{1}{15}
\]
\[
v = -15\;\text{cm}
\]
Thus the virtual image forms **15 cm in front of the lens** (same side as the object).
Magnification (IGCSE formula)
\[
m = -\frac{v}{u}= -\frac{-15}{6}= +2.5
\]
- A **positive** magnification indicates an upright image.
- \(|m| = 2.5\) shows the image is 2.5 times taller than the object (magnified).
Everyday Applications of Virtual Images
- Magnifying glass: a convex lens held close to an object creates a large, upright virtual image that the eye can focus on.
- Microscope eyepiece: the eyepiece forms a virtual image of the real image produced by the objective, providing the final magnification.
- Reading glasses: a weak convex lens produces a virtual image at the near point of the eye, reducing the accommodation effort for presbyopic readers.
Practical Activity (AO3 – Skills)
- Secure a thin converging lens on a sheet of paper and draw a straight principal axis.
- Mark the optical centre O and the focal points F1 and F2 (measure the focal length using a distant light source).
- Place an upright object (e.g. a pencil) at three different positions between O and F1 (e.g. 2 cm, 4 cm, 6 cm).
- Using a ray‑tracing kit or a laser pointer, draw the three principal rays for each object position.
- Extend the refracted rays backwards to locate the virtual image; measure its distance from the lens.
- Calculate the theoretical image distance and magnification with the thin‑lens equation; compare with your measurements.
- Record all data in a table, comment on any discrepancies, and discuss possible sources of error (lens thickness, parallax, non‑thin‑lens effects, etc.).
Common Mistakes to Avoid
- Confusing the near focal point F1 with the far focal point F2.
- Drawing the parallel ray through the wrong focal point – for a virtual‑image case it must **appear** to diverge from F1 after refraction.
- Forgetting to extend the refracted rays **backwards** when locating a virtual image.
- Applying the sign convention incorrectly: remember that \(u\) is always positive, \(v\) is negative for virtual images, and \(f\) is positive for converging lenses.
- Using the magnitude of \(v\) directly in the magnification formula; the sign of \(v\) determines the sign of \(m\) and therefore the image orientation.
- Interpreting a negative magnification as “upright”. In the IGCSE convention, **positive** magnification → upright; **negative** → inverted.
Summary Checklist
- Identify lens type and assign the correct sign to the focal length.
- Confirm the object is placed between the lens and its focal point (\(0
- Draw the three principal rays accurately, remembering the correct behaviour of the parallel ray for a virtual image.
- Extend the refracted rays backwards to locate the virtual image.
- Use the thin‑lens equation with the IGCSE sign convention to verify the image distance.
- Calculate magnification with \(m = -v/u\); a **positive** value confirms an upright image.
- Relate the result to a real‑world example (e.g., magnifying glass) and, if possible, test it experimentally.