Optical instruments: Microscope and Telescope

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Discussion Overview

The discussion revolves around the formulas for calculating the magnifying power of microscopes and telescopes, including the application of sign conventions. Participants explore the differences between angular and linear magnification as well.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants present formulas for the magnifying power of telescopes and microscopes, noting the use of negative signs to indicate image inversion.
  • One participant states that the angular magnification of a telescope is equal to the ratio of the focal lengths of the objective and eyepiece, with the formula M.P. = - (fobjective / feyepiece).
  • Another participant provides the formula for the magnifying power of a microscope as M.P. = -(g / fobjective) * (25 cm / feyepiece), where g is the tube length.
  • Participants discuss the distinction between angular and linear magnification, with one suggesting that telescopes create an effect of magnification by increasing angles rather than enlarging images.
  • One participant illustrates the difference in magnification by comparing the images produced by a telescope and a microscope on a screen, noting that the telescope does not produce a larger image than the object itself.

Areas of Agreement / Disagreement

Participants present multiple viewpoints on the definitions and implications of angular versus linear magnification, indicating that the discussion remains unresolved regarding the nuances of these concepts.

Contextual Notes

Some assumptions regarding the definitions of magnification types and the conditions under which the formulas apply are not fully explored, leaving room for further clarification.

D. Wani
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What are the different formulas for the calculation of magnifying power of a microscope and a telescope? And how would we use the sign conventions in them?
 
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D. Wani said:
What are the different formulas for the calculation of magnifying power of a microscope and a telescope? And how would we use the sign conventions in them?

If the eye is relaxed for distant viewing, the telescope simply produces an
angular magnification equal to the ratio of the focal length of the objective to the focal length of the eyepiece,
so M.P. = - (fobjective / f eye piece) ( The negative sign indicates that the image is inverted.).

Magnifying power(M.P) of a microscope. = -(g /fobjective).{(25 cm)/feyepiece.} , where g is The tube length .
It is the distance between the secondary focal point of the objective and the primary focal point of the eyepiece.
25 cm. is the least distance of distinct vision of human eye.
here also the negative sign indicates that the image is inverted.
 
What is the difference between angular and linear magnification
 
D. Wani said:
What is the difference between angular and linear magnification
Perhaps I can illustrate this difference by using the two instruments to project their images onto a white screen. For instance, a telescope projecting the Sun's image on to a card and a microscope projecting an image of a cell on to a card. You will notice that the Sun's image is smaller than the actual object, but the cell's image is larger than the object. So the telescope does not make an image that is bigger than the original, but makes the eye think so by increasing the angles. I was taught to refer to "magnifying power" for telescopes, rather than magnification.
 

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