IB PHYSICS HL2 OPTICS LAB: LENSES AND MIRRORS Purpose In this lab we will observe the images formed by lenses and mirrors and use the thin lens equation to calculate their focal lengths. We will also set up a slide projector, an overhead projector, and make some general observations about how these instruments form images. Background Thin, spherical lenses and mirrors can both be used to form images. This is because they have the ability to bring light rays from distant objects to a focus (see diagrams below). Light rays from an object an infinite distance away will be parallel. When parallel rays pass through a lens, they will be refracted to a single point on the other side of the lens. This point is called the focal point, and the distance between the center of the lens and the focal point is called the focal length f of the lens. Focal point Object at infinity Converging lens Parallel rays striking a mirror will be reflected to a point: the focal point of the mirror. The distance from the mirror to the focal point is the focal length of the mirror. It is found that for rays not too far from the mirror’s optical axis (axis of symmetry) the focal length is one-half its radius of curvature: f = R/2. Focal point Object at infinity Converging mirror Light rays from nearby objects will not be parallel. They will be refracted or reflected in such a way as to form an image near the focal point. Where the image forms depends on the focal length of the lens or mirror and on how far away the object is. To calculate the image location, we can use the thin lens equation. The Thin Lens Equation Both lenses and mirrors obey the thin lens equation: 1 = 1 + 1 f di do (1) where f is the focal length; do is the object distance: the distance from the object emitting the light to the center of the lens or mirror; di is the image distance: the distance from the lens or mirror to the image formed. For converging lenses and mirrors, f is a positive number. Converging lenses and mirrors cause light rays to converge to a point, as in the two diagrams above. For diverging lenses or mirrors, f is considered negative. Diverging lenses and mirrors cause light rays to diverge. The focal point is the point from which the rays appear to diverge. See diagrams below. Focal point Diverging Lens Focal point Diverging Mirror The image distance, di, can be positive or negative depending on where the image forms. Consider first a converging lens (refer to the first diagram above). When the object is located outside its focal length, the converging lens will form an image beyond the focal point on the other side of the lens. This is called a real image, since it occupies a real position in space. (For instance, the image can be observed on a screen placed at the image distance.) In this case the image distance is considered positive. In the limiting case where the object is located at infinity (or far enough away to be considered at infinity), the image forms at the focal point. That is, f = di (object at infinity) as is evident from the thin lens equation, with do very large. As the object moves closer to the lens, the image moves farther away on the other side, as is also evident from the thin lens equation. When the object moves inside the focal length of the lens, the image will form on the same side of the lens as the object. The image distance is considered a negative number, and the image is called a virtual image. A virtual image is one that can be seen only by looking through the lens. It cannot be projected on a screen and its position cannot be directly measured. Instead, we must measure the image distance by an indirect method (see the method of parallax, below). Converging mirrors also form real and virtual images. The image will be real and di is a positive number when the object is located outside the focal length of the mirror. The image will form on the same side of the mirror as the object, outside its focal point. An object at infinity will form a real image at the focal point. When the object moves inside the focal distance of the mirror, the image becomes virtual – we have to look into the mirror to see it – and it appears to form on the other side of the mirror from the object. In this case, the image distance di is considered to be a negative number. Diverging lenses and mirrors form virtual images only - the images they form cannot be projected on a screen. For a diverging lens the image forms on the same side of the lens as the object. For a diverging mirror, the image forms on the opposite side of the mirror from the object. For both, the image distance i is taken to be a negative number, as is the focal length f. Magnification The magnification of an image can be calculated in two ways: (2) m = -hi/ho or (3) m = d i /d o where m is the magnification, ho is the height of the object and hi is the height of the image, and di and do are the image and object distances, respectively. In Part A, you will investigate the images formed by lenses and mirrors. For each of the images you find, record the positions of the object, lens, and screen in your lab notebook. Later, you will calculate the object distances, image distances, and focal lengths for each image. Also record the heights of the object and of the image (omit for object at infinity) and describe the image as real or virtual, enlarged or reduced, upright or inverted. In Part B, you will set up three simple optical instruments: a microscope, an overhead projector, and a slide projector. For reference: Thin Lens equation 1 = 1 + 1 f di do Magnification m = hi/ho= di/do Equipment Optics bench Object lamp Screen Converging (convex) lens Converging (concave) mirror Table lamp Object for optical bench Light source at “infinity” f = focal length di = image distance do = object distance M = magnification hi = height of image ho = height of object di = dist. from lens to image do = dist. from lens to object Part A. Investigate image formation by a convex lens and a concave mirror. Convex Lens 1 1. Object at infinity. Place the longer focal length lens on the optics bench and point it out the window or door and find an image of a distant object. In this case, the focal length is the same as the image distance. Determine and record this. 2. Nearby objects. Place the object lamp at one end and the screen at the other end of the optics bench. Put the lens in between. First, get a qualitative overview of the object/image relationship. Observe and describe how the image and its position change for different object distances. Then measure the positions and the heights of the object and image for object placed at approximately 3f, 2.5f, 2f, 1.5f and .5f, where f is the focal length as determined above. For the last object position (object inside focal length) a qualitative description is sufficient, since no real image exists. Convex Lens 2 -Repeat the procedure above for the convex lens of shorter focal length. Concave Mirror 1. Object at infinity. Place the mirror on the optics bench and point it out the window or door and find an image of a distant object. In this case, the focal length is the same as the image distance. Determine and record this. 2. Nearby objects. Place the object lamp at one end of the bench and the mirror at the other end. First, get a qualitative overview of the object/image relationship. Observe and describe how the image and its position change for different object distances. Then measure the positions and the heights of the object and image for object placed at approximately 3f, 2.5f, 2f, 1.5f and .5f. For the last object position (object inside focal length) a qualitative description is sufficient, since no real image exists. Part B. Optical Instruments For each of the following, describe the image (real or virtual/upright or inverted), estimate the image magnification, and record the length of the instrument (the distance between the lenses). Overhead Projector Examine this device for a few minutes. How does this device make use of lenses and mirrors to produce the desired effect (For example, why isn’t the teacher’s writing reversed left to right)? Describe in words and include a diagram. Note the number of lenses, number of mirrors, and the location of each. Slide Projector How does this instrument work? Why is it sometimes confusing when placing slides into a projector? What “case” (choose from #1-6) for a converging lens is this instrument? *This is a discussion only…you will not actually experiment with this! Compound Microscope How many lenses are used in a compound microscope? What type of image (real or virtual?) does each lens form? Why is it sometimes confusing to adjust a slide in a microscope? Analysis: A. Lenses and Mirrors. Calculate the focal lengths and magnifications for each image, for each lens or mirror. Take an average for the focal lengths and compare to the value obtained for the lens or mirror with the sun (“infinite distance” away). Compare the magnifications as determined by measurement (M=hi/ho) to that given by theory (M=-di/do). Discuss the sources of error for ach of these measurements. B. Optical Instruments. Include your answers to the questions posed above for each optical instrument and your diagrams for the light rays in each type of optical instrument. The diagrams should show the light rays from the time they leave the object until they form the image. C. For each of the following, draw ray diagrams to scale in your lab book: *Use rulers and compasses for these! (1) convex lens with object outside the focal point (do >f) (2) convex lens with object inside the focal point (do < f) (3) concave lens with object outside the focal point (do >f) (4) concave mirror with object outside the focal point (do > f)