Lenses
Posted in Physics, OpticsCurvature of wavefronts
Light from most sources - like the sun - radiates outwards as a series of wavefronts. These wave fronts are curved and as they travel further from their source their curvature decreases. Light from a far away source such as the sun or stars are assumed to have no curvature as the difference between this and the actual wave length is negligible.
Lenses
The purpose a lens is to either increase or decrease the curvature of the waves entering them.
Converging lenses add more curvature to the entering wavefronts focusing them at a point if they are entering parallel. The distance of this point from the lens is referred to as the focal length of the lens. At this point a 'real image' of the light entering the lens is formed.
Diverging lenses remove curvature from the wavefronts causing them to diverge.
The power of the lens
The power of the lens describes how much curvature a lens adds or removes from the wavefronts entering and is measured in dioptres (D). The power of a lens is given by the formula:
Where f is the focal length of the lens
The lens equation
The lens equation relates the focal length of a lens and the curvature of the wave fronts entering and leaving:
Where is the image distance, the distance between the lens and the point where the in-focus image is formed,
is the object distance, the distance between the object the image is of and the lens and
is the focal length of the lens.
Note: the object distance is always negative.
Magnification
The change in size of an object image by a lens is called magnification and is given by the equation: