Combination of Thin Lenses

When two or more thin lenses are placed in contact with each other, they behave as a single equivalent lens. This is the fundamental idea behind combination of thin lenses. Rather than tracing rays through each lens separately — which quickly becomes tedious — physicists developed simple rules to find the combined focal length and optical power of the system in one step. This principle underlies almost every optical instrument you will ever encounter, from spectacles and microscopes to telephoto camera lenses. The key insight is that optical power is additive. The power P of a lens is defined as the reciprocal of its focal length: P = 1/f (in metres). When two thin lenses with powers P₁ and P₂ are placed in contact, the total power is simply P_total = P₁ + P₂. Equivalently, the reciprocal of the combined focal length equals the sum of the reciprocals of the individual focal lengths. This additive property makes designing multi-lens systems far more straightforward. Sign convention matters enormously here. Using the standard convention, converging (convex) lenses have positive focal lengths and positive powers, while diverging (concave) lenses have negative values. A combination can therefore be converging, diverging, or even act like a plane glass sheet (infinite focal length, zero power) depending on the individual lenses chosen. Understanding these combinations is essential for designing corrective lenses and scientific instruments.

Key takeaways
  • Why Powers Add: A Refraction Argument
  • Power: The Practical Unit
  • Extending to Three or More Lenses
  • Effective Focal Length and Image Formation

Why Powers Add: A Refraction Argument

Consider a ray passing through the first lens of focal length f₁. The lens bends (refracts) the ray by an amount proportional to 1/f₁. The second lens then bends it further by an amount proportional to 1/f₂. Because the lenses are in contact (zero separation), these angular deflections simply add together. The total deflection corresponds to a single lens of focal length f_eq, where 1/f_eq = 1/f₁ + 1/f₂. This is not an approximation for thin lenses in contact — it is exact within the thin-lens model.

Power: The Practical Unit

Optical power P = 1/f, measured in dioptres (D), where 1 D = 1 m⁻¹. A converging lens of focal length +0.5 m has power +2 D. A diverging lens of focal length −0.25 m has power −4 D. Combined, their total power is +2 + (−4) = −2 D, giving an equivalent focal length of f_eq = 1/(−2) = −0.5 m — a diverging combination. Optometrists use dioptres every day when prescribing spectacles; a typical short-sighted person might have a prescription of −2.5 D.

Extending to Three or More Lenses

The rule extends naturally: for n thin lenses in contact, 1/f_eq = 1/f₁ + 1/f₂ + ... + 1/fₙ, or equivalently P_total = P₁ + P₂ + ... + Pₙ. This is only valid when the lenses are truly in contact (negligible separation). If there is a significant gap d between two lenses, the correct formula becomes 1/f_eq = 1/f₁ + 1/f₂ − d/(f₁f₂). For the combination-in-contact case, d = 0, which recovers the simple sum.

Effective Focal Length and Image Formation

Once you have f_eq, you treat the combination exactly like a single thin lens. The thin-lens equation 1/v − 1/u = 1/f_eq applies directly (using the real-is-positive or Cartesian sign convention consistently). The combined lens produces the same image position and magnification that the full multi-lens system would produce, provided the lenses are truly in close contact and both are thin relative to the object and image distances.

The Key Equation

1feq=1f1+1f2⟺Ptotal=P1+P2\frac{1}{f_{\text{eq}}} = \frac{1}{f_1} + \frac{1}{f_2} \quad \Longleftrightarrow \quad P_{\text{total}} = P_1 + P_2
  • f_{\text{eq}} — Equivalent focal length (metres (m)): The focal length of the single lens that produces the same effect as the combination.
  • f_1,\, f_2 — Individual focal lengths (metres (m)): Focal lengths of the first and second lens; positive for converging, negative for diverging.
  • P_{\text{total}} — Total optical power (dioptres (D = m⁻¹)): The combined refracting power of the lens system.
  • P_1,\, P_2 — Individual powers (dioptres (D)): Powers of each lens: P = 1/f. Positive for converging, negative for diverging lenses.

Worked Example

Problem. A converging lens of focal length +20 cm is placed in contact with a diverging lens of focal length −30 cm. Find (a) the equivalent focal length and (b) the total power of the combination. Is the combination converging or diverging?

feq=+60 cm,Ptotal=+1.67 D (converging)f_{\text{eq}} = +60\text{ cm},\quad P_{\text{total}} = +1.67\text{ D (converging)}

Answer. Equivalent focal length = +60 cm; Total power = +1.67 D; the combination is converging.

Figure
Diagram
Combination of Two Thin Lenses in ContactaxisL₁ (converging)f₁ = +20 cmL₂ (diverging)f₂ = −30 cmEquivalent lensf_eq = +60 cmIncident rayF_eqP_total = P₁ + P₂= +5.00 + (−3.33)= +1.67 D
Origins · 1 minAugustin-Jean Fresnel and how this was discovered
AF
Augustin-Jean Fresnel
1788–1827 · French

Fresnel made foundational contributions to the wave theory of light and lens optics. He developed the mathematical framework for understanding how lenses refract and combine light, and invented the Fresnel lens — a multi-element optical device that effectively combines many thin refracting zones to produce a powerful, lightweight lens. His work on the addition of optical elements directly informs how we analyse combinations of thin lenses today. Fresnel's lighthouse lenses were so revolutionary that they could project a beam visible over 50 km out to sea, replacing much heavier and less efficient mirror systems — all using the principle of dividing a thick lens into thin annular sections whose powers add together.

  • Thin Lens Formula — The thin-lens equation (1/v − 1/u = 1/f) is applied directly once the equivalent focal length of a combination has been found.
  • Power of a Lens — Optical power P = 1/f in dioptres is the central quantity that makes lens combination calculations additive and simple.
  • Refraction at Curved Surfaces — Understanding how a single curved surface refracts light provides the physical basis for why individual lens powers add when lenses are combined.
  • Optical Instruments — Microscopes, telescopes, and cameras all exploit lens combinations; knowing equivalent focal length is essential to analyse their magnification and design.