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Light travels from point A to B point via reflection at point O on the surface of a mirror. Without using calculus, show that length AOB is a minimum when the angle of incidence is equal to the angle of reflection .

Short Answer

Expert verified

For the surface of a mirror, the length AoBof is minimum when the angle of incidence is equal to angle of reflection .

Step by step solution

01

The given data

Light travels from pointA to pointB via reflection at point role="math" localid="1662978767434" Oon the surface of a mirror.

02

Understanding the concept of the reflection

Reflection is the change in direction of a wavefront at an interface between two different media so that the wavefront returns to the medium from which it originated. Using the concept of reflection, the ray direction of the light can be traced as per the reflection through the media surfaces.

03

Calculation to prove that the length AOB is minimum when angle of incidence is equal to angle of reflection

Hint: Consider the image of Ain the mirror.

Consider the ray diagram as shown below:


From the ray diagram, we can get that

+y=+y(:+y=2=+y)=

The angle of incidence is equal to angle of reflection.

Consider an incident rayAOwith reflected rayO'Bwheretheangle of incidence is not equal totheangle of reflection.

From the above figure, we get that

AO'B=AO'+O'BAO'B=A'O'BAO'+O'B=A'O+O'B

But

localid="1662980270688" A'O'+O'B>A'B("Twosidesofthesumofthetwosidesofatriangle>hypotenuse")

And

A'B=A'O+OBA'B=AO+OBAO+OB=AOB

Thus, from all above options, we get that the shortest path as:

AO'B=AO'+O'B=A'O+O'B>A'B=A'O+OB=AO+OB=AOB

Thus, the length AOBof is less than A'OB and AOB.

Hence, the length of AOBis minimum.

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Most popular questions from this chapter


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?

You grind the lenses shown in Fig. 34-53 from flat glass disks (n=1.5)using a machine that can grind a radius of curvature of either 40cmor 60cm. In a lens where either radius is appropriate, you select the 40cmradius. Then you hold each lens in sunshine to form an image of the Sun. What are the (a) focal length fand (b) image type (real or virtual) for (bi-convex) lens 1, (c)f and (d) image type for (plane-convex) lens 2, (e) f and (f) image type for (meniscus convex) lens 3, (g) f and (h) image type for (bi-concave) lens 4, (i) fand (j) image type for (plane-concave) lens 5, and (k) f and (l) image type for (meniscus concave) lens 6?

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?

An object is moved along the central axis of a spherical mirror while the lateral magnification m of it is measured. Figure 34-35 gives m versus object distance p for the rangepa=2cm and pb=8.0cm. What is m for p=14cm?

A peanut is placed 40cmin front of a two-lens system: lens 1 (nearer the peanut) has focal length f1 =20cm, lens 2 has f2=-15cm and the lens separation is d=10cm. For the image produced by lens 2, what are (a) the image distance i2(including sign), (b) the image orientation (inverted relative to the peanut or not inverted), and (c) the image type (real or virtual)? (d) What is the net lateral magnification?

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