Quick Recap — Ray Optics in Action

Work with a strict sign convention (distances measured from the pole/optical centre; real-is-positive for mirrors on the object side).

  • Mirror: 1v+1u=1f\dfrac{1}{v}+\dfrac{1}{u}=\dfrac{1}{f}, m=vum=-\dfrac{v}{u}. Lens: 1v1u=1f\dfrac{1}{v}-\dfrac{1}{u}=\dfrac{1}{f}, m=vum=\dfrac{v}{u}.
  • Lens-maker: 1f=(n1)(1R11R2)\dfrac{1}{f}=(n-1)\left(\dfrac{1}{R_1}-\dfrac{1}{R_2}\right); in a medium replace (n1)(n-1) by (nlensnmed1)\left(\dfrac{n_{lens}}{n_{med}}-1\right) — the sign can flip.
  • Two lenses a distance dd apart: P=P1+P2dP1P2P=P_1+P_2-d\,P_1P_2. Displacement method: f=D2x24Df=\dfrac{D^2-x^2}{4D}.
  • Refraction at a spherical surface: n2vn1u=n2n1R\dfrac{n_2}{v}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R}. Apparent shift through a slab =t(11n)=t\left(1-\dfrac{1}{n}\right).

Worked mini-example. Object 20 cm before a concave mirror, f=15f=15 cm: 1v=1f1u=115+120=160\dfrac{1}{v}=\dfrac{1}{f}-\dfrac{1}{u}=-\dfrac{1}{15}+\dfrac{1}{20}=-\dfrac{1}{60}, so v=60v=-60 cm (real) and m=vu=3m=-\dfrac{v}{u}=-3 — a real, inverted image magnified three times.