/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 31 A short straight object of lengt... [FREE SOLUTION] | 91Ó°ÊÓ

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A short straight object of length \(L\) lies along the central axis of a spherical mirror of focal length \(f\), a distance \(o\) from the mirror. (a) Show that its image in the mirror has a length \(L^{\prime}\) where $$L^{\prime}=L\left(\frac{f}{o-f}\right)^{2}$$ (Hint: Locate the two ends of the object.) (b) Show that the longitudinal magnification \(m^{\prime}\left(=L^{\prime} / L\right)\) is equal to \(m^{2}\), where \(m\) is the lateral magnification.

Short Answer

Expert verified
The image length is \(L^{\prime} = L\left( \frac{f}{o-f} \right)^2\) and longitudinal magnification \(m^{\prime = m^2\)\.

Step by step solution

01

Understanding the Problem

The problem involves a short straight object placed along the central axis of a spherical mirror. The goal is to determine the image length and the longitudinal magnification.
02

Recall the Mirror Equation

The mirror equation relates the object distance (\(o\)), image distance (\(i\)), and focal length (\(f\)): \[ \frac{1}{f} = \frac{1}{o} + \frac{1}{i} \]
03

Express Image Distance

Rearrange the mirror equation to express the image distance (\(i\)): \[ i = \frac{of}{o-f} \]
04

Locate Image Positions of Two Ends

Consider the ends of the object located at \(o\) and \(o + L\): \[ i_1 = \frac{of}{o-f} \] and \[ i_2 = \frac{(o + L)f}{o + L - f} \]
05

Approximate for Small Lengths

If \(L\) is small compared to \(o\), approximate the difference between the image distances of the two ends using a binomial expansion: \[ i_2 \approx \frac{of}{o-f} + \frac{Lf^2}{(o-f)^2} \]
06

Calculate the Image Length

The length of the image (\(L^{\prime}\)) is the difference \[(i_2 - i_1)\]: \[ L^{\prime} = \frac{Lf^2}{(o-f)^2} \]
07

Express Longitudinal Magnification

Longitudinal magnification (\(m^{\prime\)) is defined as: \[ m^{\prime} = \frac{L^{\prime}}{L} = \left(\frac{f}{o-f}\right)^2 \]
08

Relate to Lateral Magnification

Recall the lateral magnification (\(m\)): \[ m = -\frac{i}{o} = \frac{f}{o-f} \]. Thus, longitudinal magnification is: \[ m^{\prime} = m^2 \]

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

spherical mirror
A spherical mirror can be either concave or convex. These mirrors have a surface that forms a part of a sphere. When light rays reflect off these mirrors, they follow specific paths determined by the shape of the mirror. The key parts of a spherical mirror include:

  • Center of Curvature (C): The center of the sphere from which the mirror is a section.
  • Principal Axis: A straight line passing through the center of curvature and the center of the mirror.
  • Focal Point (F): The point where parallel rays of light either converge (concave) or appear to diverge (convex) after reflecting off the mirror.
  • Focal Length (f): The distance between the focal point and the mirror's surface.
Understanding these terms helps in analyzing the behavior of light and the image formation in spherical mirrors.
mirror equation
The mirror equation is crucial for determining the relationship between object distance ( o ), image distance ( i ), and focal length ( f ). The equation is expressed as:

\[ \frac{1}{f} = \frac{1}{o} + \frac{1}{i} \]
This means that for any object placed at a distance o from the mirror, there is a corresponding image formed at distance i .
The equation allows us to predict where the image will form if we know the object distance and the focal length. Rearranging the equation to solve for the image distance gives:

\[i = \frac{of}{o-f}\]
So, if we know the focal length and the object distance, we can easily calculate where the image will appear.
lateral magnification
Lateral magnification ( m ) describes how the size of the image compares to the size of the object in a mirror. It tells us how much larger or smaller the image is compared to the actual object.
  • Formula: \[m = \frac{h_i}{h_o} = \frac{-i}{o}\] where h_i is the image height, h_o is the object height, i is the image distance, and o is the object distance.
If the magnification is positive, the image is upright compared to the object. If the magnification is negative, the image is inverted.

In our problem, we found that the longitudinal magnification ( m' ) is related to the lateral magnification by:
  • Formula for longitudinal magnification: \[m' = m^2\]
This shows that as the image gets larger or smaller laterally, its length changes quadratically. This helps in understanding the detailed nature of image formation and precise calculations required for spherical mirrors.

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Most popular questions from this chapter

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