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Concept Version 10
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The Thin Lens Equation and Magnification

The thin lens equation relates the object distance do, image distance di, and focal length f.

Learning Objective

  • Formulate five basic rules of ray tracing


Key Points

    • Ray tracing can be used to construct an image from the light rays originating from an object that pass through a lens. The image is located at the point where the rays cross. By choosing several points from an object the entire image can be constructed .
    • We define do to be the object distance, the distance of an object from the center of a lens. Image distance di is defined to be the distance of the image from the center of a lens. The height of the object and height of the image are given the symbols ho and hi, respectively.
    • The thin lens equation quickly provides the relation between di, do, and the focal length f. It can be derived from a geometric analysis of ray tracing for thin lenses and is given by $\frac{1}{d_o}+\frac{1}{d_i}=\frac{1}{f}$ .
    • The magnification m of an image is the ratio between the image and object height (hi/ho). The magnification is related to do, di, ho, and hi by the following relation: $\frac{h_i}{h_o}=-\frac{d_i}{d_o}=m$ .

Terms

  • thin lens equation

    Relates object distance do, image distance di, and focal length f: $\frac{1}{d_o}+\frac{1}{d_i}=\frac{1}{f}$

  • image distance

    The distance of the image from the center of the lens.

  • magnification

    The apparent enlargement of an object in an image.


Full Text

The Thin Lens Equation and Magnification

Image Formation by Thin Lenses

How does a lens form an image of an object? We can use the technique of ray tracing to illustrate how lenses form images. We can also develop equations to describe the images quantitatively. Recall the five basic rules of ray tracing:

  1. A ray entering a converging lens parallel to its axis passes through the focal point F of the lens on the other side.
  2. A ray entering a diverging lens parallel to its axis seems to come from the focal point F.
  3. A ray passing through the center of either a converging or a diverging lens does not change direction.
  4. A ray entering a converging lens through its focal point exits parallel to its axis.
  5. A ray that enters a diverging lens by heading toward the focal point on the opposite side exits parallel to the axis.

Consider an object some distance away from a converging lens, as shown in . To find the location and size of the image formed, we trace the paths of selected light rays originating from one point on the object (in this case the top of the person's head). The figure shows three rays from the top of the object that can be traced using the five ray tracing rules. Rays leave this point going in many directions, but we concentrate on only a few with paths that are easy to trace. The first ray is one that enters the lens parallel to its axis and passes through the focal point on the other side (rule 1). The second ray passes through the center of the lens without changing direction (rule 3). The third ray passes through the nearer focal point on its way into the lens and leaves the lens parallel to its axis (rule 4). The three rays cross at the same point on the other side of the lens. The image of the top of the person's head is located at this point. All rays that come from the same point on the top of the person's head are refracted in such a way as to cross at the point shown. Rays from another point on the object, such as her belt buckle, will also cross at another common point, forming a complete image, as shown. Although three rays are traced in , only two are necessary to locate the image. It is best to trace rays for which there are simple ray tracing rules. Before applying ray tracing to other situations, let us consider the example shown in in more detail.

Image Formation with a Thin Lens

Ray tracing is used to locate the image formed by a lens. Rays originating from the same point on the object are traced—the three chosen rays each follow one of the rules for ray tracing, so that their paths are easy to determine. The image is located at the point where the rays cross. In this case, a real image—one that can be projected on a screen—is formed.

Several important distances appear in . We define do as the object distance—the distance of an object from the center of a lens. Image distance diis defined as the distance of the image from the center of a lens. The height of the object and height of the image are given the symbols ho and hi, respectively. Images that appear upright relative to the object have heights that are positive and those that are inverted have negative heights. Using the rules of ray tracing and making a scale drawing with paper and pencil, like that in , we can accurately describe the location and size of an image. But the real benefit of ray tracing is in visualizing how images are formed in a variety of situations. To obtain numerical information, we use a pair of equations that can be derived from a geometric analysis of ray tracing for thin lenses. The thin lens equation is:

$\frac{1}{d_o}+\frac{1}{d_i}=\frac{1}{f}$

We define the ratio of image height to object height (hi/ho) as the magnification m. The magnification is related to do, di, ho, and hi by the following relation:

$\frac{h_i}{h_o}=-\frac{d_i}{d_o}=m$

In many cases both of these equations are referred to together as the thin lens equations. The thin lens equations are broadly applicable to all situations involving thin lenses (and "thin" mirrors).

Thin Lens Equations for a Convex Lens

Shows how to use the thin lens equation to calculate the image distance, image height and image orientation for convex lenses when the object distance is greater the the focal length (f).

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