lens formula derivation

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The derivation of the Gaussian form proceeds from triangle geometry. Again, take the convex lens formula, 1/f = (n-1) (1/R1 -1/R2) where n is the refractive index and R1 and R2 are radii of the two faces of the lens. For a biconvex lens, assuming that R1 = R2, and n= 1.5 roughly for glass,then substituting these values in the above formula, we get the value of f as infinity, which is really absurd. The object lies close to principal axis. ; The lens has a small aperture. For a thin lens, the lens power P is the sum of the surface powers. ; The incident rays make small angles with the lens surface or the principal axis. Consider a convex lens with O be the optical centre, and F be the principal focus with focal length f. Now, let AB be the object kept perpendicular to the principal axis and at a distance beyond the focal length. Lens Formula Derivation. The thin lens equation is also sometimes expressed in the Newtonian form. The lens equation tells us everything we need to know about the image of an object that is a known distance from the plane of a thin lens of known focal length. Here, x 1 and x 2 are the distances to the object and image respectively from the focal points. The same derivation used for the thin lens equation can be used to show that for a thick lens provide the effective focal length given by is used, and the distances s o and s i are measured from the principle points located at 1 s i + 1 s o = 1 1 f f = (n l! n m)! Assumptions made: The lens is thin. 1 R 1! 2. Convex Lens. For thicker lenses, Gullstrand's equation can be used to get the equivalent power. 1 R 2 + (n l! The Newtonian Lens Equation We have been using the “Gaussian Lens Formula” An alternate lens formula is known as the Newtonian Lens Formula which can be easily verified by substituting p = f + x 1 and q = f + x 2 into the Gaussian Lens Formula. Numerical Methods In Lens (A) Lens Formula Definition: The equation relating the object distance (u), the image distance (v) and the focal length (f) of the lens is called the lens formula. The sign conventions for the given quantities in the lens equation and magnification equations are as follows: f is + if the lens is a double convex lens (converging lens) f is - if the lens is a double concave lens (diverging lens) d i is + if the image is a real image and located on the opposite side of the lens. While we have derived it for the case of an object that is a distance greater than the focal length, from a converging lens, it works for all the combinations of lens and object distance for which the thin lens approximation is good.

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