Focal length

The signed distance from a mirror or lens to its focal point. It is positive for a converging optic and negative for a diverging one, and it is the quantity f in the thin lens and mirror equation.

1si+1so=1f\frac{1}{s_i} + \frac{1}{s_o} = \frac{1}{f}

Printed on the AP Physics 2 sheet, and it serves mirrors and lenses alike. The sign of ff is what tells the equation which optic you have.

OpticSign of ff
Concave mirror, convergingpositive
Convex mirror, divergingnegative
Converging lens, convexpositive
Diverging lens, concavenegative

One pattern generates the table: ff is positive when real light actually converges at the focal point, and negative when the rays only appear to come from it. A concave mirror can start a fire, a convex one cannot.

Focal point and focal length are not the same thing. The focal point is a place, where rays parallel to the principal axis meet or appear to meet. The focal length is a signed distance to it. A lens has a focal point on each side; for the thin symmetric lenses this course uses, both sit f|f| from the centre, so one number describes the lens.

For a spherical mirror the CED says the focal point may be approximated as the point halfway between the surface and the centre of curvature, so f=R/2|f| = R/2 for rays close to the axis. That relation is not on the equation sheet, so halve the radius yourself. No equivalent exists for lenses: no lensmaker's equation appears anywhere in AP Physics 2, so a lens focal length is given or measured. A flat mirror has infinite ff, and 1/f=01/f = 0.

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