Focal Length of a Spherical Mirror

f=R2f = \frac{R}{2}

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Rays arriving parallel to the axis of a spherical mirror reflect through a point halfway to the center of curvature — a small-angle result that makes mirror design beautifully simple. Grind a telescope mirror to a 4 m radius of curvature and you get a 2 m focal length. The rule underlies everything from shaving mirrors to the giant primaries of observatories (which are then tweaked into paraboloids to remove the residual spherical aberration).

Focal Length of a Spherical Mirror
f=R2f = \frac{R}{2}
Where
  • ff= Focal length
  • RR= Radius of curvature
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