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The equation 1p+1i=2rfor spherical mirrors is an approximation that is valid if the image is formed by rays that make only small angles with the central axis. In reality, many of the angles are large, which smears the image a little. You can determine how much. Refer to Fig. 34-22 and consider a ray that leaves a point source (the object) on the central axis and that makes an angle a with that axis. First, find the point of intersection of the ray with the mirror. If the coordinates of this intersection point are x and y and the origin is placed at the center of curvature, then y=(x+p-r)tan a and x2+ y2= r2where pis the object distance and r is the mirror鈥檚 radius of curvature. Next, use tan=yxto find the angle b at the point of intersection, and then use+y=2tofind the value of g. Finally, use the relationtany=y(x+i-r)to find the distance iof the image. (a) Suppose r=12cmand r=12cm. For each of the following values of a, find the position of the image 鈥 that is, the position of the point where the reflected ray crosses the central axis:(0.500,0.100,0.0100rad). Compare the results with those obtained with theequation1p+1i=2r.(b) Repeat the calculations for p=4.00cm.

Short Answer

Expert verified
  1. The position of the image for the given values of (0.500rad,0.100rad,0.0100rad)whenr=12andp=20is7.799cm,8.544cm,8.571cm.
  2. The position of the image for the given values of(0.500rad,0.100rad,0.0100rad)whenr=12andp=4cmis-13.56cm,-12.05cm,-12cm.

Step by step solution

01

Determine the given quantities

Radius of curvature r=12cm

Object distance p=20cm

Object distance p=4cm

02

Determine the concepts of mirror equation

Use the mirror equation to find the image distance. Using the method given in the problem, then calculate image distance for differentvalues and for different object distance values.

Formula:

1p+1i=1f=2r

localid="1664258469754" f=r2

03

 Step 3: (a) Calculate the position of the image for the given values of α

Position of the image for the given values of for r=12cm and p=20cm:

Given=0.500rad,r=12cm,p=20cm.

The distance from the object to point x is as follows:

d=p-r+x=20cm-12cm+x=8cm+x

Also,

y=dtan0.500rad=28.65

Solve for the value of y as:

y=(8cm+x)tan28.65o=4.3704+0.54630x

From x2 + y2= r2solve as:

x2+(4.3704+0.5463x)2=(12cm)2x=8.1398cm

Solve as:

y=dtan=4.3704+0.5463(8.1398)=8.8172cm

Solve as:

=(8.81728.1398)=0.8253rad

Then:

=2-=20.8233rad-0.500rad=1.151rad=65.980

Solve further as:

tan=y(x+i-r)tantan65.98=8.8172(8.1398+i-12)i=7.799cm.

In a similar way, solve as:

For=0.100rad,i=8.544cm

For =0.0100rad,i=8.571cm

Now, the mirror equation relates an object distance p, mirror鈥檚 focal length f and the image distance i as:

1p+1i=1f=2r

120cm+1i=212cm=i=8.571cm

Thus, the mirror equation yields the value i = 8.571cm.

While using the given method the values are:

For=0.500rad,i=7.799cm

For =0.100rad,i=8.544cm

For =0.0100rad,i=8.571cm

The position of the image for the given values of (0.500rad,0.100rad,0.0100rad)when r=12cm and p=20 cm is7.799cm,8.544cm,8.571cm.

04

(b) Solve for the part (a) for p=4.00cm

Repeat calculation for p=4cm:

For=0.500rad,r=12cm,p=4cm.

The distance from the object to point x is

d=p-r+x=4cm-12cm+x=-8cm+x

Solve as:

y=dtan0.500rad=28.65

y=(8cm+x)tantan28.655=-4.3704+0.54630x

From x2 +y2=r2solve as:

x2+(-4.3704+0.5463x)2=(12cm)2x=-8.1398cm

Solve further as:

y=dtan=-4.3704+0.5463(-8.1398)=-8.8172cm

Solve for the beta as:

localid="1663050628081" =(-8.81728.1388)=-0.8253rad

Solve further as:

=2-=2-0.8253rad-0.500rad=2.1506rad=132.280

Consider the formula as:

tan=y(x+i-r)

Substitute the value and solve as:

tantan132.28=(-8.8172)(-8.1398+i-12)

i=-13.56cm

In a similar way, the obtained values are:

For=0.100rad,i=-12.05cm

For=0.0100rad,i=-12cm

Now, the mirror equation relates an object distance p, mirror鈥檚 focal length f and the image distance i as:

14cm+1i=212cm

i = -12cm

Thus, the mirror equation yields the value i = -12cm

From the given method the obtained values are鈥

For =0.500rad,i=-13.56cm=0.500rad,i=-13.56cm

For =0.100rad,i=-12.05cm

For=0.0100rad,i=-12cm

The position of the image for the given values of(0.500rad,0.100rad,0.0100rad)when r=12cm and p=4cm is-13.56cm,-12.05cm,-12cm

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Most popular questions from this chapter

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.)

A short straight object of lengthLlies along the central axis of a spherical mirror, a distance pfrom the mirror. (a) Show that its image in the mirror has alength, L'=L(f/(p-f))2(Hint: Locate the two ends of the object.) (b) Show that the longitudinal magnification is equal tom'=(L'/L) is equal to m2, where m is the lateral magnification.

A cheese enchilada is4.00cmin front of a converging lens. The magnification of the enchilada is-2.00. What is the focal length of the lens?

The table details six variations of the basic arrangement of two thin lenses represented in Fig. 34-29. (The points labeledF1and F2are the focal points of lenses 1 and 2.) An object is distancep1to the left of lens 1, as in Fig. 34-18. (a) For which variations can we tell, without calculation, whether the final image (that due to lens 2) is to the left or right of lens 2 and whether it has the same orientation as the object? (b) For those 鈥渆asy鈥 variations, give the image location as 鈥渓eft鈥 or 鈥渞ight鈥 and the orientation as 鈥渟ame鈥 or 鈥渋nverted.鈥


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:

m=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 (鈥渆ffective鈥 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?

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