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An object of height \(h\) is placed at a distance \(d_{0}\) on the left side of a converging lens of focal length \(f\left(f

Short Answer

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Question: An object is placed in front of a converging lens, and an image is formed 3 times the focal length, f, to the right of the lens. a) Calculate the distance the object needs to be placed on the left side of the lens, dâ‚€. b) Calculate the magnification, M, of the image. Answer: a) The object must be placed at a distance of \(\frac{3f}{2}\) on the left side of the lens. b) The magnification of the image is -2, meaning the image is flipped and twice the size of the object.

Step by step solution

01

Solving for \(d_0\) with the lens equation

We have the lens equation: \(\frac{1}{f} = \frac{1}{d_0} + \frac{1}{d}\). Given that \(d = 3f\), we can substitute this into the lens equation and solve for \(d_0\): \(\frac{1}{f} = \frac{1}{d_0} + \frac{1}{3f}\) Now, we'll solve for \(d_0\): \(\frac{1}{d_0} =\frac{1}{f} - \frac{1}{3f} = \frac{3-1}{3f} = \frac{2}{3f}\) Therefore, \(d_0 = \frac{3f}{2}\) So the object must be placed at a distance \(\frac{3f}{2}\) on the left side of the lens for the image to form at a distance \(3f\) on the right side of the lens.
02

Calculating the magnification

Now that we have found \(d_0 = \frac{3f}{2}\), we can use the formula for magnification, \(M = \frac{-d}{d_0}\): \(M = \frac{-3f}{\frac{3f}{2}}\) Multiplying by \(\frac{2}{1}\) to clear the fraction: \(M = \frac{-2(3f)}{1(3f)}\) Canceling the common factor of \(3f\) in the numerator and denominator: \(M = -2\) The magnification is -2, indicating that the image is flipped (which is denoted by the negative sign) and is twice the size of the object.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Lens Equation
The lens equation is a fundamental formula used in optics, helping us understand how converging lenses, like the one in this exercise, form images. It is represented by the equation \( \frac{1}{f} = \frac{1}{d_0} + \frac{1}{d} \), where:
  • \( f \) is the focal length of the lens,
  • \( d_0 \) is the distance from the lens to the object, and
  • \( d \) is the distance from the lens to the image.
Knowing how to rearrange and use this equation can help solve many problems related to lenses. For instance, if the desired image distance \( d \) and the lens's focal length \( f \) are known, you can rearrange the equation to find the object distance \( d_0 \). In our case, we needed the image to form at \( 3f \). Substituting this into the lens equation allowed us to solve for \( d_0 \), leading to \( d_0 = \frac{3f}{2} \). This indicates how far the object should be placed from the lens to achieve the required image distance.
Magnification
Magnification tells us how much larger or smaller the image is compared to the object. It also gives us information about the orientation of the image. In optics, magnification \( M \) can be calculated using the formula: \( M = \frac{-d}{d_0} \), where:
  • \( d \) is the image distance,
  • \( d_0 \) is the object distance, and
  • The negative sign indicates that a negative magnification means the image is inverted.
In our exercise, with \( d = 3f \) and \( d_0 = \frac{3f}{2} \), plugging these into the magnification formula gives \( M = -2 \). This result tells us two things:
  • The image is flipped upside down as the magnification is negative, and
  • It is twice the size of the original object.
Image Formation
Image formation through lenses is a key concept in understanding how lenses function in various applications, from eyeglasses to cameras. A converging lens, as used in our problem, bends light rays inward, converging them at a point to form an image.
Images formed by lenses can be either real or virtual. A real image is formed when the light actually converges at the image location and can be projected onto a screen. Conversely, a virtual image forms when the light rays do not actually meet but only appear to converge.
In the given exercise, the image formed at a distance \( 3f \) on the right side of the lens is real and inverted, which is confirmed by the negative magnification value. Understanding how the arrangement of the object, lens, and placement affects the type and orientation of the image is crucial for effectively utilizing lenses in practical scenarios.

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Most popular questions from this chapter

You are experimenting with a magnifying glass (consisting of a single converging lens) at a table. You discover that by holding the magnifying glass \(92.0 \mathrm{~mm}\) above your desk, you can form a real image of a light that is directly overhead. If the distance between the light and the table is \(2.35 \mathrm{~m},\) what is the focal length of the lens?

You have found in the lab an old microscope, which has lost its eyepiece. It still has its objective lens, and markings indicate that its focal length is \(7.00 \mathrm{~mm}\). You can put in a new eyepiece, which goes in \(20.0 \mathrm{~cm}\) from the objective. You need a magnification of about 200. Assume you want the comfortable viewing distance for the final image to be \(25.0 \mathrm{~cm}\). You find in a drawer eyepieces marked \(2.00-, 4.00-,\) and \(8.00-\mathrm{cm}\) focal length. Which is your best choice?

When a diver with \(20 / 20\) vision removes her mask underwater, her vision becomes blurry. Why is this the case? Does the diver become nearsighted (eye lens focuses in front of retina) or farsighted (eye lens focuses behind retina)? As the index of refraction of the medium approaches that of the lens, where does the object get imaged? Typically, the index of refraction for water is 1.33 , while the index of refraction for the lens in a human eye is \(1.40 .\)

Mirrors for astronomical instruments are invariably first-surface mirrors: The reflective coating is applied on the surface exposed to the incoming light. Household mirrors, on the other hand, are second-surface mirrors: The coating is applied to the back of the glass or plastic material of the mirror. (You can tell the difference by bringing the tip of an object close to the surface of the mirror. Object and image will nearly touch with a first-surface mirror; a gap will remain between them with a second-surface mirror.) Explain the reasons for these design differences.

A refracting telescope has the objective lens of focal length \(10.0 \mathrm{~m}\). Assume it is used with an eyepiece of focal length \(2.00 \mathrm{~cm}\). What is the magnification of this telescope?

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