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In the science of optics, the magnification of an object like a lens is the ratio of the height of the image you can see to the height of the actual object being magnified. For instance, a lens that makes a small object appear very big has a high magnification, while a lens that makes an object appear small has a low magnification. An object's magnification is generally given by the equation M = (hi/ho) = -(di/do), where M = magnification, hi = image height, ho = object height, and di and do = image and object distance.

Method 1
Method 1 of 2:

Finding the Magnification of a Single Lens

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Note: A converging lens is wider in the middle than it is at the edges (like a magnifying glass.) A diverging lens is wider at the edges than it is in the middle (like a bowl).[1] Finding magnification is the same for both, with one important exception. Click here to go straight to the diverging lens exception.

  1. [2] Like with many other physics problems, a good way to approach magnification problems is to first write the equation you need to find your answer. From here, you can work backwards to find any pieces of the equation that you need.[3]
    • For example, let's say that a 6 centimeter tall action figure is placed half a meter away from a converging lens with a focal length of 20 centimeters. If we want to find the magnification, image size, and image distance, we can start by writing our equation like this:
      M = (hi/ho) = -(di/do)
    • Right now, we know ho (the height of the action figure) and do (the distance of the action figure from the lens.) We also know the focal length of the lens, which isn't in this equation. We need to find hi, di, and M.
  2. If you know the distance of the object you're magnifying from the lens and the focal length of the lens, finding the distance of the image is easy with the lens equation. The lens equation is 1/f = 1/do + 1/di, where f = the focal length of the lens.[4]
    • In our example problem, we can use the lens equation to find di. Plug in your values for f and do and solve:
      1/f = 1/do + 1/di
      1/20 = 1/50 + 1/di
      5/100 - 2/100 = 1/di
      3/100 = 1/di
      100/3 = di = 33.3 centimeters
    • A lens's focal length is the distance from the center of the lens to the point where the rays of light converge in a focal point. If you've ever focused light through a magnifying glass to burn ants, you've seen this. In academic problems, this is often given to you. In real life, you can sometimes find this information labeled on the lens itself.
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  3. Once you know do and di, you can find the height of the magnified image and the magnification of the lens. Notice the two equals signs in the magnification equation (M = (hi/ho) = -(di/do)) — this means that all of the terms are equal to each other, so we can find M and hi in whatever order we want.[5]
    • For our example problem, we can find hi like this:
      (hi/ho) = -(di/do)
      (hi/6) = -(33.3/50)
      hi = -(33.3/50) × 6
      hi = -3.996 cm
    • Note that a negative height indicates that the image we see will be inverted (upside down).
  4. You can solve for your final variable using either -(di/do) or (hi/ho).[6]
    • In our example, we would finally find M like this:
      M = (hi/ho)
      M = (-3.996/6) = -0.666
    • We also get the same answer if we use our d values:
      M = -(di/do)
      M = -(33.3/50) = -0.666
    • Note that magnification does not have a unit label.
  5. Once you have a magnification value, you can predict several things about the image you would view through the lens. These are:
    • Its size. The bigger the absolute value of the M value, the bigger the object will seem under magnification. M values between 1 and 0 indicate that the object will look smaller.
    • Its orientation. Negative values indicate that the image of the object will be inverted.
    • In our example, our M value of -0.666 means that, under the conditions given, the image of the action figure will appear upside down and two-thirds its normal size.
  6. Even though diverging lenses look very different than converging lenses, you can find their magnification values using the same formulas as above. The one important exception here is that divergent lenses will have negative focal lengths. In a problem like the one above, this will affect the answer you get for di, so be sure to pay close attention.[7]
    • Let's re-do the example problem above, only this time, we'll say we're using a diverging lens with a focal length of -20 centimeters. All of the other starting values are the same.
    • First, we'll find di with the lens equation:
      1/f = 1/do + 1/di
      1/-20 = 1/50 + 1/di
      -5/100 - 2/100 = 1/di
      -7/100 = 1/di
      -100/7 = di = -14.29 centimeters
    • Now we'll find hi and M with our new di value.
      (hi/ho) = -(di/do)
      (hi/6) = -(-14.29/50)
      hi = -(-14.29/50) × 6
      hi = 1.71 centimeters
      M = (hi/ho)
      M = (1.71/6) = 0.285
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Method 2
Method 2 of 2:

Finding the Magnification of Multiple Lenses in Sequence

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Easy Two-Lens Method

  1. When you're dealing with a device that is made up of two lenses lined up with each other (like a telescope or one part of a pair of binoculars), all you need to know is the focal length of both lenses to find the overall magnification of the final image. This is done with the simple equation M = fo/fe.[8]
    • In the equation, fo refers to the focal length of the objective lens and fe to the focal length of the eyepiece lens. The objective lens is the large lens at the end of the device, while the eyepiece lens is, as its name suggests, the small lens you put your eye next to.
  2. Once you have the focal lengths for both of your lenses, solving is easy — just find the ratio by dividing the objective's focal length by the eyepiece's. The answer you get will be the magnification of the device.[9]
    • For example, let's say that we have a small telescope. If the focal length of the objective lens is 10 centimeters and the focal length of the eyepiece lens is 5 centimeters, the magnification is simply 10/5 = 2.
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Detailed Method

  1. If you have two lenses lined up in front of an object, it's possible to determine the magnification of the final image if you know the distances of the lenses and objects in relation to each other, the size of the object, and the focal lengths of both lenses. Everything else can be derived.
    • For example, let's say that we have the same setup as in our example problem in Method 1: a six-inch action figure 50 centimeters away from a converging lens with a focal length of 20 centimeters. Now, let's put a second converging lens with a focal length of 5 centimeters 50 centimeters behind the first lens (100 centimeters away from the action figure.) In the next few steps, we'll use this information to find the magnification of the final image.
  2. The first part of any multi-lens problem is the same as if you were dealing with just the first lens. Starting with the lens closest to the object, use the lens equation to find the distance of the image, then use the magnification equation to find its height and magnification. Click here for a recap of single-lens problems.
    • From our work in Method 1 above, we know that the first lens produces an image -3.996 centimeters high, 33.3 centimeters behind the lens, and with a magnification of -0.666.
  3. Now, finding the magnification, height, and so on for the second lens is easy — just use the same techniques that you used for the first lens, only this time, use its image in place of the object. Keep in mind that the image will usually be a different distance from the second lens as the object was from the first one.[10]
    • In our example, since the image is 33.3 centimeters behind the first lens, it is 50-33.3 = 16.7 centimeters in front of the second one. Let's use this and the new lens's focal length to find the second lens's image.
      1/f = 1/do + 1/di
      1/5 = 1/16.7 + 1/di
      0.2 - 0.0599 = 1/di
      0.14 = 1/di
      di = 7.14 centimeters
    • Now, we can find hi and M for the second lens:
      (hi/ho) = -(di/do)
      (hi/-3.996) = -(7.14/16.7)
      hi = -(0.427) × -3.996
      hi = 1.71 centimeters
      M = (hi/ho)
      M = (1.71/-3.996) = -0.428
  4. This basic approach is the same whether you have three, four, five, or a hundred lenses lined up in front of an object. For each lens, treat the image of the previous lens as its object and use the lens equation and magnification equation to find your answers.
    • Keep in mind that subsequent lenses can continue to invert your image. For instance, the magnification value we got above (-0.428) indicates that the image we see will be about 4/10 the size of the image from the first lens, but right side up, since the image from the first lens was upside down.
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Community Q&A

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  • Question
    What does it mean when a magnifying glass is 100mm - 5x?
    Donagan
    Donagan
    Top Answerer
    Its diameter is 100 mm, and it makes objects appear to be five times their actual size.
  • Question
    How does percent magnification convert to x times magnification?
    Donagan
    Donagan
    Top Answerer
    100% magnification equals 2x magnification. 200% = 3x. 300% = 4x, and so forth.
  • Question
    Should I look at the sign on the value of magnification to know if the image is larger than the object?
    Community Answer
    Community Answer
    No, the sign is related to whether the image is (-) or isn't (+) inverted in relation to the object. You know that the image is larger if the value is bigger than one M > 1.
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Tips

  • Binoculars are typically specified as a number times a number. For example, binoculars can be specified as 8x25 or 8x40. When such a specification is made, the first number is the magnification of the binoculars. It does not matter that the examples given have different second numbers, the binoculars both have a magnification of 8. The second number refers to the clarity of the image presented by the binoculars.
  • Note that for a single lens magnifying tool, the magnification would be a negative number if the distance to the object was greater than the focal length of the lens. That does not mean that the object would be reduced in apparent size. In such a case, the magnification would occur, but the image would be seen upside down by the observer.
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About This Article

Grace Imson, MA
Reviewed by:
Math Teacher
This article was reviewed by Grace Imson, MA. Grace Imson is a math teacher with over 40 years of teaching experience. Grace is currently a math instructor at the City College of San Francisco and was previously in the Math Department at Saint Louis University. She has taught math at the elementary, middle, high school, and college levels. She has an MA in Education, specializing in Administration and Supervision from Saint Louis University. This article has been viewed 377,885 times.
80 votes - 59%
Co-authors: 13
Updated: October 16, 2024
Views: 377,885
Categories: Physics
Article SummaryX

To calculate magnification, use the following formula: magnification = the height of the image ÷ by the height of the object. Plug your data into the formula and solve. If your answer is greater than 1, that means the image is magnified. If your answer is between 0 and 1, the image is smaller than the object. Finally, if your answer is negative, that means the image is upside down. Keep reading to learn how to calculate magnification when you're looking through multiple lenses!

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