Telescope Magnification: Calculating Linear Magnification and Magnifying Power

Click For Summary

Homework Help Overview

The discussion revolves around calculating the linear magnification and magnifying power of a telescope with given focal lengths for the objective and eyepiece. The original poster expresses confusion regarding the difference between linear magnification and magnifying power, as different answers are provided in their textbook.

Discussion Character

  • Conceptual clarification, Assumption checking, Mixed

Approaches and Questions Raised

  • Participants explore the definitions of linear magnification and magnifying power, with some suggesting that they are distinct concepts. There is a discussion about the application of the lens formula and the conditions under which different types of magnification are calculated.

Discussion Status

Several participants have provided insights into the definitions and calculations related to magnification. There is an ongoing exploration of the differences between linear and angular magnification, with some participants questioning the assumptions made in the calculations. The discussion is active, with no clear consensus reached yet.

Contextual Notes

Participants note that the object is not at a very large distance, which affects the application of the lens formula. There is also mention of a discrepancy between the calculated magnifying power and the answer provided in the textbook.

Amith2006
Messages
416
Reaction score
2
Please help!
# A telescope has an objective of focal length 50 cm and an eye piece of focal length 5 cm. It is focused for distinct vision on a scale 200 cm away from the objective. What is the linear magnification of the telescope numerically? Also what is the magnifying power of the telescope numerically?
Could someone tell me, if linear magnification of the telescope different from magnifying power of the telescope? I think they both mean the same. I have this doubt because 2 different answers are given in my book for linear magnification and magnifying power of the telescope.
 
Physics news on Phys.org
Oddly, I've never actually heard the term "linear magnification." The magnification of the telescope is just the focal length of the objective divided by the focal length of the eyepiece. Therefore, this telescope-eyepiece system achieves a magnification of 10x.

- Warren
 
I think...
The linear magnification is the ratio of the length of the image to the length of object.

This is called in such a way because some times we find the ratio of the area of image to the area of object this is called aerial magnification which is square of the linear magnification.

The linear magnification hear is not fo/fe because the object (200 cm.) is not at very large distance and the rays, from a point of the object, can not be considered parallel. You have to apply the lens formula to find the object distance and the image distance for the distance of the image from the optical center of objective and so on... This is not simply fo as in the case if the object is at long distance. Try this and you will learn automatically.
 
There is a word linear magnification in physics in terms of optical instruments. It is a unitless number that is the ratio of the height of the image and the height of the object.

Additionally, I think you are talking about the angular magnification of the telescope for the magnifying power. Angular magnification is different for linear magnification.


WDJr
 
Last edited:
According to my Physics 11 textbook, linear magnification is "the ratio of the size of an image to the size of the object". I'm not so sure about the term "magnifying power". WDJr seems to be correct:

"The angular size of the virtual image seen by the observer will be larger than the actual angular size of the object. The ratio of these two sizes is the magnifying power and is equal to the ratio of the focal lengths of the objective and ocular."
-- http://www.infoplease.com/ce6/sci/A0861462.html
 
Last edited:
I solved it in following way:
Assuming it to be an astronomical telescope and the final image is formed at the least distance of distinct vision(D). Let f(o) & f(e) be the focal length of objective and eye piece. We know that,
Magnifying power = Angular Magnification = [f(o)/f(e)]{1 + f(e)/D}
= (50/5){1 + 5/25}
= 12
Is it right? But the answer given in my book is 16.
 

Similar threads

  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 12 ·
Replies
12
Views
3K
Replies
3
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
Replies
2
Views
2K
  • · Replies 11 ·
Replies
11
Views
3K
  • · Replies 3 ·
Replies
3
Views
4K
  • · Replies 2 ·
Replies
2
Views
2K