Figure 34-47a shows the basic structure of the human eye. Light refracts into the eye through the cornea and is then further redirected by a lens whose shape (and thus ability to focus the light) is controlled by muscles. We can treat the cornea and eye lens as a single effective thin lens (Fig. 34-47b). A “normal” eye can focus parallel light rays from a distant object O to a point on the retina at the back of the eye, where the processing of the visual information begins. As an object is brought close to the eye, however, the muscles must change the shape of the lens so that rays form an inverted real image on the retina (Fig. 34-47c). (a) Suppose that for the parallel rays of Figs. 34-47a and b, the focal length fof the effective thin lens of the eye is 2.50 cm. For an object at distance p = 40 cm, what focal length f of the effective lens is required for the object to be seen clearly? (b) Must the eye muscles increase or decrease the radii of curvature of the eye lens to give focal length f?

Short Answer

Expert verified
  1. The focal lengthf of the effective lens required for the object to be seen clearly is 2.35 cm.
  2. For the focal lengthf, the radii of the curvature must be decreased.

Step by step solution

01

Step 1: Given data

  • f=2.5cm.
  • p=40cm.
02

Determining the concept

Using the given lens formula for the eye, find its new focal length. After that, using the lens maker's equation, find the decrease in the radii of the curvature of the eye lens to give focal length f.

The formulas are as follows:

1f=(1p+1i)1f=(n-1)(1r1-1r2)

Here p is the pole, f is the focal length, and i is the image distance.

03

Determining the focal length f’ of the effective lens required for the object to be seen clearly.

(a)

This problem is regarding the human eye. Model the cornea and eye lens as a single effective thin lens, with the image formed at the retina.

The lens formula is given by,

1i=1f-1p

For a relaxed eye, its lens focuses far-away objects on the retina so that the image distance i is behind the lens, and the object distance isp=, then,

1i=1f-11i=1fi=f

Here f is the focal length of the relaxed effective lens.

So thati=f=2.50cm.

Now p is the new object distance and f is the new focal length, then,

According to the lens formula,

1p+1i=1f'

Butlocalid="1663029348279" i=f.

Hence,

1p+1f=1f'f'=1p+1f-1f'=pfp+f

Substituting the values,

localid="1663029034365" f'=40.0×2.5040.0+2.50f'=100.042.5f'=2.35cm

Therefore, the focal lengthf of the effective lens required for the object to be seen clearly is 2.35 cm.

04

Determining the eye muscles increase or decrease the radii of curvature of the eye lens to give a focal length f’

The lens maker's equation is,

1f=n-11r1-1r2

Where, r1and r2are the radii of the curvature of the two surfaces of the lens, and n is the refractive index of the material from which the lens is formed.

But r1and r2have the same magnitude. r1 is positive and r2is negative.

role="math" localid="1663029226148" 1f=n-11r1-1r1f=n-1-11r1-1r1-1

Hence, the focal length decreases the radii of the curvature also decrease.

Using the lens formula, the focal length of an effective lens of the eye required to see the object clearly can be found.

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Most popular questions from this chapter

In Fig. 34-26, stick figure Ostands in front of a spherical mirrorthat is mounted within the boxed region;the central axis through themirror is shown. The four stick figures I1to I4suggest general locationsand orientations for the images that might be produced by themirror. (The figures are onlysketched in; neither their heightsnor their distances from the mirror are drawn to scale.) (a) Whichof the stick figures could not possibly represent images? Of thepossible images, (b) which would be due to a concave mirror, (c)which would be due to a convex mirror, (d) which would be virtual,and (e) which would involve negative magnification?


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?

(a) A luminous point is moving at speedV0toward a spherical mirror with a radius of curvaturer, along the central axis of the mirror. Show that the image of this point is moving at the speed

vI=-(r2p-r)2v0

Where,p is the distance of the luminous point from the mirror at any given time. Now assume the mirror is concave, withr=15cm.and letV0=5cm/s. FindV1when (b)p=30cm(far outside the focal point), (c) p=8.0cm(just outside the focal point), and (d)p=10mm(very near the mirror).

80 through 87 80, 87 SSM WWW 83 Two-lens systems. In Fig. 34-45, stick figure O (the object) stands on the common central axis of two thin, symmetric lenses, which are mounted in the boxed regions. Lens 1 is mounted within the boxed region closer to O, which is at object distance p1. Lens 2 is mounted within the farther boxed region, at distance d. Each problem in Table 34-9 refers to a different combination of lenses and different values for distances, which are given in centimeters. The type of lens is indicated by C for converging and D for diverging; the number after C or D is the distance between a lens and either of its focal points (the proper sign of the focal distance is not indicated). Find (a) the image distance i2 for the image produced by lens 2 (the final image produced by the system) and (b) the overall lateral magnification M for the system, including signs. Also, determine whether the final image is (c) real (R) or virtual (V), (d) inverted (I) from object O or non-inverted (NI), and (e) on the same side of lens 2 as object O or on the opposite side.

80 through 87 80, 87 SSM WWW 83 Two-lens systems. In Fig. 34-45, stick figure (the object) stands on the common central axis of two thin, symmetric lenses, which are mounted in the boxed regions. Lens 1 is mounted within the boxed region closer to O, which is at object distance p1. Lens 2 is mounted within the farther boxed region, at distance d. Each problem in Table 34-9 refers to a different combination of lenses and different values for distances, which are given in centimeters. The type of lens is indicated by C for converging and D for diverging; the number after C or D is the distance between a lens and either of its focal points (the proper sign of the focal distance is not indicated). Find (a) the image distance localid="1663045000066" i2for the image produced by lens 2 (the final image produced by the system) and (b) the overall lateral magnification Mfor the system, including signs. Also, determine whether the final image is (c) real(R)or virtual localid="1663045476655" (V), (d) inverted (I)from object O or non-inverted (NI), and (e) on the same side of lens 2 as object O or on the opposite side.

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