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An object is placed 18.0 \(\mathrm{cm}\) from a screen. (a) At what two points between object and screen may a converging lens with a 3.00 -cm focal length be placed to obtain an image on the screen? (b) What is the magnification of the image for each position of the lens?

Short Answer

Expert verified
Place the lens at 3 cm or 15 cm from the object. Magnifications are -5 and -1/5, respectively.

Step by step solution

01

Identify the Given Information

We have an object, a screen, and a lens described by its focal length. The distance between the object and the screen is given as 18.0 cm, and the focal length of the lens is 3.00 cm.
02

Understand Lens Equation

The lens-maker's formula is: \[ \frac{1}{f} = \frac{1}{d_o} + \frac{1}{d_i} \] where \( f \) is the focal length, \( d_o \) is the object distance from the lens, and \( d_i \) is the image distance from the lens. To form an image on the screen, \( d_o + d_i = 18.0 \text{ cm} \). We need to solve for both \( d_o \) and \( d_i \).
03

Express Image Distance in Terms of Object Distance

Using \( d_o + d_i = 18 \), we can express \( d_i \) as \( 18 - d_o \). Substitute \( d_i = 18 - d_o \) into the lens equation to get: \[ \frac{1}{3} = \frac{1}{d_o} + \frac{1}{18 - d_o} \].
04

Solve for Object Distance

Multiply through by \( d_o(18 - d_o) \) to clear the fractions: \[ d_o (18 - d_o) = 3(18) \]. Simplify to form a quadratic equation: \[ 3d_o^2 - 18d_o + 54 = 0 \].
05

Simplify and Solve the Quadratic Equation

Divide by 3 to simplify: \[ d_o^2 - 6d_o + 18 = 0 \]. Use the quadratic formula \( d_o = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a} \) with \( a = 1 \), \( b = -6 \), and \( c = 9 \): \[ d_o = \frac{6 \pm \sqrt{36 - 36}}{2} \]. Simplifying gives \( d_o = 3 \text{ cm} \) or \( d_o = 15 \text{ cm} \).
06

Calculate Image Distance for Each Lens Position

For \( d_o = 3 \text{ cm} \), \( d_i = 18 - 3 = 15 \text{ cm} \). For \( d_o = 15 \text{ cm} \), \( d_i = 18 - 15 = 3 \text{ cm} \). In both cases, the symmetric placement gives either distance as the other.
07

Calculating Magnification for Each Position

Magnification \( m \) is given by \( m = - \frac{d_i}{d_o} \). For \( d_o = 3 \text{ cm} \), \( m = -\frac{15}{3} = -5 \). For \( d_o = 15 \text{ cm} \), \( m = -\frac{3}{15} = -\frac{1}{5} \).
08

Interpretation of Results

The lens can be placed at \( 3 \text{ cm} \) or \( 15 \text{ cm} \) from the object. At these positions, the magnifications will be \(-5\) and \(-\frac{1}{5}\) respectively.

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Key Concepts

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

Lens Equation
The heart of understanding how a lens forms an image lies in the lens equation. The lens equation relates the object distance, image distance, and focal length of the lens. It is given by:\[\frac{1}{f} = \frac{1}{d_o} + \frac{1}{d_i}\]where:
  • \( f \) is the focal length of the lens. It indicates how strongly the lens converges or diverges light.
  • \( d_o \) is the object distance, i.e., how far the object is from the lens.
  • \( d_i \) is the image distance, measuring how far the image forms from the lens.
This equation helps us determine where an image will form for a given object and lens setup. In our exercise, we were tasked with finding the points at which a converging lens must be placed to cast the image on a screen. This forms the system of equations that can be used to solve for unknown distances.
Object Distance
The object distance is an essential element in understanding lens behavior. It represents how far the object is from the lens. In our exercise, the lens was placed at two distinct distances from the object to form a clear image on a screen. We denote this distance as \( d_o \).
To find the positions where the lens can create an image, we used the sum of object and image distances, affirming:\[d_o + d_i = 18 \text{ cm}\]Substituting in the lens equation allows us to express \( d_i \) as a function of \( d_o \):\[d_i = 18 - d_o\]This transformation is critical in setting up a solvable equation to find out where exactly to place the lens to achieve focused images.
Image Distance
The image distance tells us how far the formed image is from the lens. Using the relationship between object and image distances, this value becomes understandable. In our case, we defined it as the difference between the total distance and the object distance:\[d_i = 18 - d_o\]This expression was substituted into the lens equation to form a quadratic equation:\[\frac{1}{3} = \frac{1}{d_o} + \frac{1}{18 - d_o}\]On solving, it was revealed that the lens could be positioned where:
  • \( d_o = 3 \text{ cm} \)
  • \( d_o = 15 \text{ cm} \)
Each position of the lens aligns uniquely with a corresponding image distance, showing the symmetric nature of the setup.
Magnification Calculation
Magnification provides insight into how the size of the image changes compared to the object. It is calculated using the formula:\[m = -\frac{d_i}{d_o}\]This reveals the size relation of the image to the object, with the negative sign indicating image inversion by the lens.
In our setup:
  • For \( d_o = 3 \text{ cm} \), magnification \( m = -\frac{15}{3} = -5 \). This means the image is five times larger than the object and inverted.
  • For \( d_o = 15 \text{ cm} \), magnification \( m = -\frac{3}{15} = -\frac{1}{5} \). Thus, the image is one-fifth the size of the object, again inverted.
Understanding magnification aids in predicting not only where an image will form, but also how it compares in size and orientation to the original object.

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Most popular questions from this chapter

A camera lens has a focal length of 180.0 \(\mathrm{mm}\) and an aperture diameter of 16.36 \(\mathrm{mm}\) (a) What is the \(f\) -number of the lens? (b) If the correct exposure of a certain scene is \(\frac{1}{30} \mathrm{s}\) at \(f / 11\) , what is the correct exposure at \(f / 2.8 ?\)

Saturn is viewed through the Lick Observatory refracting telescope (objective focal length 18 \(\mathrm{m} )\) . If the diameter of the image of Satum produced by the objective is \(1.7 \mathrm{mm},\) what angle does Saturn subtend from when viewed from earth?

Pinhole Camera. A pinhole camera is just a rectangular box with a tiny hole in one face. The film is on the face opposite this hole, and that is where the image is formed. The camera forms an image without a lens, (a) Make a clear ray diagram to show how a pinhole camera can form an image on the film without using a lens. (Hint: Put an object outside the hole, and then draw rays passing through the hole to the opposite side of the box.) (b) A certain pinhole camera is a box that is 25 \(\mathrm{cm}\) square and 20.0 \(\mathrm{cm}\) deep, with the hole in the middle of one of the \(25 \mathrm{cm} \times 25 \mathrm{cm}\) faces. If this camera is used to photograph a fierce chicken that is 18 \(\mathrm{cm}\) high and 1.5 \(\mathrm{m}\) in front of the camera, how large is the image of this bird on the film? What is the magnification of this camera?

A transparent rod 50.0 \(\mathrm{cm}\) long and with a refractive index of 1.60 is cut flat at the right end and rounded to a hemispherical surface with a 15.0 -cm radius at the left end. An object is placed on the axis of the rod 120 \(\mathrm{cm}\) to the left of the vertex of the hemispherical end. (a) What is the position of the final image? (b) What is its magnification?

A solid glass hemisphere of radius 12.0 \(\mathrm{cm}\) and index of refraction \(n=1.50\) is placed with its flat face downward on a table. A parallel beam of light with a circular cross section 3.80 \(\mathrm{mm}\) in diameter travels straight down and enters the hemisphere at the center of its curved surface. (a) What is the diameter of the circle of light formed on the table? (b) How does your result depend on the radius of the hemisphere?

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