69 through 79 76, 78 75, 77 More lenses. Object ostands on the central axis of a thin symmetric lens. For this situation, each problem in Table 34-8 refers to (a) the lens type, converging C or diverging D , (b) the focal distance f , (c) the object distance p, (d) the image distance i, and (e) the lateral magnification m. (All distances are in centimeters.) It also refers to whether (f) the image is real Ror virtual V, (g) inverted I or non-inverted (NI) from O, and (h) on the same side of the lens as Oor on the opposite side. Fill in the missing information, including the value of m when only an inequality is given, where only a sign is missing, answer with the sign.

Short Answer

Expert verified
  1. The lens type is converging.
  2. The focal distance is +10cm.
  3. The object distance is +20 cm.
  4. The image distance is +20cm.
  5. The lateral magnification is -1.0.
  6. The image is real (R).
  7. The image is inverted (I).

8. The image is on the opposite side of the lens as the object

Step by step solution

01

The given data

  1. The lens is a converging type of lens.
  2. The object distance, p=+20cm
  3. The focal length of the lens, f=10cm
  4. The lens is converging.
02

Understanding the concept of properties of the lens

An object, when placed in front of a lens, produces an image. It could be real or virtual, magnified or diminished, inverted or not inverted. The type of image is decided by the type of lens used, the focal length of the lens, and the distance of the object from the lens.

Formulae:

The lens formula, 1f=1p+1i (i)

The magnification formula of the lens, m=-ip (ii)

03

a) Calculation of the lens type

From the given data in table, the lens is converging.

04

b) Calculation of the focal distance

From the data in table, the focal distance is +10cm .

05

c) Calculation of the object distance

The object distance is +20 cm as given in the problem.

06

d) Calculation of the image distance

Using the given data in equation (i), the image distance can be given as follows:

1i=110-120=120i=+20cm

Hence, the image distance is +20cmand positive.

07

e) Calculation of the lateral magnification

Now, using the given object distance and the above image distance, we can get the lateral magnification of the lens as follows:

m=-2020=-1.0cm

Hence, the lateral magnification is -1.0cm.

08

f) Calculation of the type of image

The image is real because the image distance is positive.

Hence, the image is real (R).

09

g) Calculation if the image is inverted or not

The image is inverted as the lens is converging.

Hence, the image is inverted (I).

10

h) Calculation of the position of the object

The image is on the opposite of the lens as O since the image distance is positive.

Hence, the image is on the opposite side of object.

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Most popular questions from this chapter

In Fig. 34-52, an object is placed in front of a converging lens at a distance equal to twice the focal length f1of the lens. On the other side of the lens is a concave mirror of focal lengthf2separated from the lens by a distance 2(f1+f2). Light from the object passes rightward through the lens, reflects from the mirror, passes leftward through the lens, and forms a final image of the object. What are (a) the distance between the lens and that final image and (b) the overall lateral magnification M of the object? Is the image (c) real or virtual (if it is virtual, it requires someone looking through the lens toward the mirror), (d) to the left or right of the lens, and (e) inverted or non-inverted relative to the object?

An object is placed against the center of a thin lens and then moved away from it along the central axis as the image distance is measured. Figure 34-41 gives i versus object distance p out to ps=60cm. What is the image distancewhen p=100cm?

Two plane mirrors are placed parallel to each other and 40cmapart. An object is placed 10cmfrom one mirror. Determine the (a) smallest, (b) second smallest, (c) third smallest (occurs twice), and (d) fourth smallest distance between the object and image of the object.


Isaac Newton, having convinced himself (erroneously as it turned out) that chromatic aberration is an inherent property of refracting telescopes, invented the reflecting telescope, shown schematically in Fig. 34-59. He presented his second model of this telescope, with a magnifying power of 38, to the Royal Society (of London), which still has it. In Fig. 34-59, incident light falls, closely parallel to the telescope axis, on the objective mirror. After reflection from the small mirror (the figure is not to scale), the rays form a real, inverted image in the focal plane (the plane perpendicular to the line of sight, at focal point F). This image is then viewed through an eyepiece. (a) Show that the angular magnification for the device is given by Eq. 34-15:

mθ=fob/fey

fob

the focal length of the objective is a mirror and

feyis that of the eyepiece.

(b) The 200 in. mirror in the reflecting telescope at Mt. Palomar in California has a focal length of 16.8 m. Estimate the size of the image formed by this mirror when the object is a meter stick 2.0 km away. Assume parallel incident rays. (c) The mirror of a different reflecting astronomical telescope has an effective radius of curvature of 10 m (“effective” because such mirrors are ground to a parabolic rather than a spherical shape, to eliminate spherical aberration defects). To give an angular magnification of 200, what must be the focal length of the eyepiece?

Two thin lenses of focal lengths f1andf2 are in contact and share the same central axis. Show that, in image formation, they are equivalent to a single thin lens for which the focal length is f=f1f2(f1+f2).

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