loading...
Accommodation required against object vergence (red = now) and the amplitude left at this age
Starting.
running...
The science
Vergence. Light from an object at distance d reaches the eye with vergence −1/d (dioptres, metres). The eye adds its power P and the light converges to an image at distance v inside the vitreous (refractive index n = 1.336): n/v = P − 1/d. The image is sharp when v equals the axial length L, so the power needed is Preq = n/L + 1/d. A relaxed normal eye has P = 60 D, so L = n/P = 22.3 mm.
Accommodation. The ciliary muscle contracts, the zonule fibres slacken and the elastic lens rounds up and thickens, adding A dioptres: P = 60 + S + A, with S the spectacle power. The eye uses A = Preq − 60 − S limited to 0 … Amax, with the Hofstetter mean Amax = 18.5 − 0.30 · age. The near point is about 1/(Amax + 0.25 D).
Preq = n/L + 1/d A = clamp(Preq − 60 − S, 0, Amax) b = Dp L |ΔP| / n
Blur. If the power is wrong by ΔP the rays from the two pupil edges meet in front of or behind the retina, and a point becomes a disc of diameter b = Dp L |ΔP| / n. The eye accepts ±0.25 D (depth of focus) before things look blurred. The red bar on the retina and the letters in the inset use this blur.
Eye length and glasses. A long eye (myopia) focuses in front of the retina and needs a concave lens S = n/L − 60, about −2.7 D per extra millimetre. A short eye (hyperopia) focuses behind the retina and is hidden by accommodation; presbyopia is the loss of Amax, treated with a plus lens.
Honest simplifications. A reduced eye: all refraction at one principal plane in one medium, thin spectacle lens at the cornea (the drawn spectacle position is pictorial), no spherical aberration, astigmatism, chromatic effects or Stiles-Crawford effect. The globe and lens are drawn schematically (lens thickness 3.6 mm + 0.045 mm per dioptre); the object is placed on a compressed logarithmic scale. Hofstetter amplitude and the 0.25 D depth of focus are typical values, individuals vary by about 2 D.