Understanding Angular Magnification in Simple Magnifiers and Telescopes

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SUMMARY

The discussion clarifies the principles of angular magnification in simple magnifiers and telescopes. Maximum angular magnification occurs when the object is positioned at the near point (25 cm from the eye) for magnifiers, while for telescopes, it is achieved when the image is at infinity, necessitating the object to be at the focal length. The distinction between the two devices is emphasized, highlighting that the eyepiece focal point is crucial for telescopes. Additionally, the conversation touches on the limitations of "Mickey Mouse" equations and the advantages of parabolic reflectors in reducing aberrations.

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  • Understanding of basic optics principles
  • Familiarity with the concept of focal length
  • Knowledge of angular magnification calculations
  • Experience with lens aberrations and their effects
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  • Explore the derivation of angular magnification formulas for thin lenses
  • Study the differences between simple magnifiers and telescopes in detail
  • Investigate the design and benefits of parabolic reflectors in telescopes
  • Learn about the application of Pythagorean theorem in optics
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Optics students, amateur astronomers, and anyone interested in understanding the mechanics of magnification in optical devices.

ThatDude
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So basically, in the text below, they say that maximum angular magnification is achieved when the object is placed 25 cm from the eye, i.e. at the near point. The minimum angular magnification is achieved when the object is placed at the focal length.

However, for the chapter on the telescope, they explain that to achieve maximum angular magnification, you need the image at infinity, therefore the object must be at the focal length!

Is this not contradictory?
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I think you may be confused on the difference between the telescope and the magnifier. The highest angular magnification still occurs at the eye's focal point, which would be at the focal point of the eye piece of the telescope, the object lens on the telescope is what needs to see the image at infinity. Please note that these are also "Mickey Mouse" equations that only deal with special scenarios and thin lens, because a real lens will have some type of aberration, and the better telescopes will use a parabolic-reflector which offers no aberration (a simple derivation of this would be a good exercise as I did it yesterday and was quite fun!)
 
Also think about what happens when an image is infinitely far away, using Pythagoras theorem we see that the object is very very tall, but judging it from very far we can also use a small angle approximation.
 

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