In Fig. 34-51, a box is somewhere at the left, on the central axis of the thin converging lens. The image Imof the box produced by the plane mirror is 4.00cm “inside” the mirror. The lens–mirror separation is 10.0cm, and the focal length of the lens is 2.00cm. (a) What is the distance between the box and the lens? Light reflected by the mirror travels back through the lens, which produces a final image of the box. (b) What is the distance between the lens and that final image?

Short Answer

Expert verified
  1. The distance between box and lens is 3cm.
  2. The distance between the lens and final image is 2.33cm.

Step by step solution

01

The given data

  • Lens-mirror separation,10cm
  • Distance ofImproduced by the plane mirror,4cm
  • Focal length, f=2cm
02

Understanding the concept of lens-mirror set

Consider a thin converging lens in which the thickest part is very small in width relative to the object distance, the image distance, and the focal length. In this case, the object for the mirror that results in that box image is equally in front of the mirror about 4 cm. This object is the first image formed by the system produced by the first transmission through the lens, i.e., 10 - 4 = 6cm, and focal length is f = 2 cm. For the second transmission through the lens, to find the distance between the lens and the final image, we can use distance and focal length from the first one.

Formulae:

The lens formula,

1f=1p+1i ...(i)

Here f is the focal length, i is the image distance, p is the object distance, m is the magnification.

03

a) Calculation of the distance between box and lens

The object for the mirror that results in that box image is equally in front of the mirror. Thus, for the first transmission the image distance is found to be:

i1=10cm-4cm=6cm

And the focal length to be: f=2cm.

Now, using the above values in equation (i), the object distance (box) from the lens as follows:

localid="1663025945731" 12cm=1p+16cm1p=12cm-16cm=3-16cm=13cmp=3cm

Hence, the distance between box and the lens is 3cm.

04

b) Calculation of the distance between the lens and the final image

The box image serves as an object for the light returning through the lens f=2cm.

At this point, the object distance is found to be:

role="math" localid="1663025875085" p=10cm+4cm=14cm.

Thus, using the above values in equation (i), the distance between the lens and the final image can be calculated as follows:

role="math" localid="1663025833390" 12cm=114cm+1i1i=12cm-114cm=7-114cm=614cmi=2.33cm

Hence, the distance between the image and the lens is 2.33cm.

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Most popular questions from this chapter

58 through 67 61 59 Lenses with given radii. An object Ostands in front of a thin lens, on the central axis. For this situation, each problem in Table 34-7 gives object distance p, index of refraction n of the lens, radius r1of the nearer lens surface, and radius r2of the farther lens surface. (All distances are in centimeters.) Find (a) the image distance and (b) the lateral magnification m of the object, including signs. Also, determine whether the image is (c) real (R)or virtual (V), (d) inverted (I)from the object Oor non-inverted (NI), and (e) on the same side of the lens as object Oor on the opposite side

An object is 20cmto the left of a thin diverging lens that has a 30cmfocal length. (a) What is the image distance i? (b) Draw a ray diagram showing the image position.


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 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.

An object is placed against the center of a concave mirror and then moved along the central axis until it is 5.0 m from the mirror. During the motion, the distance |i|between the mirror and the image it produces is measured. The procedure is then repeated with a convex mirror and a plane mirror. Figure 34-28 gives the results versus object distance p. Which curve corresponds to which mirror? (Curve 1 has two segments.)

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