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shows such a telescope. Note that in the reflecting telescope the light never passes The largest reflecting telescopes in the world are at the Keck Observatory on Mauna Kea, Hawaii. The site includes two telescopes with diameters of 10 m, each containing Summary 1165 The lateral magnification M of the image due to a mirror or lens is defined as the ratio of the image height h! to the object height h and is equal to the negative of the (36.1, 36.2) In the paraxial ray approximation, the object distance p and image distance q for a spherical mirror of radius R are related by the mirror equation: (36.4, 36.6) where f " R/2 is the focal length of the mirror. An image can be formed by refraction from a spherical surface of radius R . The object and image distances for refraction from such a surface are related by (36.8) where the light is incident in the medium for which the index of refraction is n 1 and is refracted in the medium for which the index of refraction is n 2 . The inverse of the focal length f of a thin lens surrounded by air is given by the lens makers’ equation: (36.15) Converging lenses have positive focal lengths, and diverging lenses have negative For a thin lens, and in the paraxial ray approximation, the object and image distances are related by the thin lens equation: (36.16) The ratio of the focal length of a camera lens to the diameter of the lens is called the f-number of the lens: (36.18) The intensity of light incident on the film in the camera varies according to: (36.19) I , 1 (
f/D) 2 , 1 (
f -number) 2 f -number ! f D 1 & 1 q " 1 1 f " (n $ 1) $ 1 R 1 $ 1 R 2 % n 1 p & n 2 q " n 2 $ n 1 R 1 & 1 q " 2 R " 1 M " h! h " $ q p S U M M A R Y Take a practice test for this chapter by clicking on |