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Lenses Physics 202 Professor Lee Carkner Lecture 23
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Refraction Lenses can be used for the same purposes Lenses have focal lengths and real and virtual images, but their properties also depend on the index of refraction It has two sides we have to account for
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Lenses We will consider only thin lenses, i.e. thickness much smaller than i, p or f If the two surfaces are the same, the lens is symmetric
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Lenses and Mirrors Mirrors produce virtual images on the opposite side from the object Mirrors produce real images on the same side as the object If a mirror curves towards the object, f and r are positive (real focus) Real is positive, virtual is negative
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Converging and Diverging
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Converging Lens A lens consisting of two convex lenses back to back is called a converging lens The focal point is on the opposite side from the incoming rays Converging lenses produce images larger than the object m = -i/p
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Diverging Lens A lens consisting of two concave lenses back to back is called a diverging lens f is virtual and negative Diverging lenses produce images smaller than the object
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Converging and Diverging
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Lens Equations A thin lens follows the same equation as a mirror, namely: 1/f = 1/p + 1/i 1/f = (n-1) (1/r 1 -1/r 2 ) Where r 1 and r 2 are the radii of curvature of each side of the lens (r 1 is the side nearest the object) For symmetric lenses r 1 and r 2 have opposite sign
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Three Types of Images
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Converging Lenses and Images Objects in front of the focal point (nearer to the lens) produce virtual images on the same side as the object Objects behind the focal point (further from the lens) produce real images on the opposite side of the lens
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Diverging Lenses and Images No matter where the object is, a diverging lens produces an upright, virtual image on the same side as the object Virtual images form on the same side as the object, real images form on the opposite side
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Three Types of Images
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1)
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2)
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Two Lenses To find the final image we find the image produced by the first lens and use that as the object for the second lens For a two lens system the magnification is: M = m 1 m 2 In reality the lenses are not thin and may be arranged in a complex fashion
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Dual Lenses
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Near Point How can you make an object look bigger Increases angular size The largest clear (unlensed) image of an object is obtained when it is at the near point (about 25 cm) A converging lens will increase the angular diameter of an object
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Magnifying Lens You can use a magnifying lens to overcome the limitation of your eye’s near point The magnification is: m = 25 cm /f This is the size of the object seen through the lens compared to its size at the near point
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Magnifying Glass
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Compound Microscope A simple compound microscope consists of an objective and eyepiece The eyepiece acts as a magnifying glass The magnification of the objective is m = -i/p p is very close to the focal length of the objective, f ob M = (-s/f ob )(25 cm/f ey ) where s is the distance between the focal point of the lenses (the tube length) and f is the focal length
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Microscope
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Refracting Telescope In a telescope the two lenses are placed so that the two inner focal points are in the same place The eyepiece then magnifies the real image m = -f ob /f ey
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Refracting Telescope
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Giant 40 inch Refractor at Yerkes Observatory, Williams Bay Wisconsin
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Newtonian Telescope
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Telescopes The magnification of the telescope can be altered by changing eyepieces Magnification is not the most important property of a telescope The true purpose of the objective lens is to gather more light than your eye can and focus it so that it can be viewed The objective becomes so large it is hard to build and support
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