OpticsLesson 3 of 3 in the course Geometric Optics and Image Formation

Compound Microscopes and Refracting and Reflecting Telescopes

5 flashcards · 5 quiz questions · 5 match pairs · 5 fill-in sentences · English

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Summary

A compound microscope uses two convex lenses in sequence to reveal details too small to see clearly with the unaided eye. Understanding what each lens does helps explain how the instrument produces a large, viewable image.

A compound microscope commonly contains two convex lenses. The objective is close to the specimen and has a short focal length, giving it high optical power. Typical objective magnifications range from about 5× to 100×. The eyepiece, also called the ocular, has a longer focal length and acts much like a magnifying glass.

All flashcards

Objective lens in a compound microscope
The short-focal-length convex lens near the specimen; it forms the real intermediate image.
Eyepiece magnification at the near point
For relaxed conventions with the final image at the near point, its angular magnification is 1+25 cm/feye1+25\text{ cm}/f_{eye} when feyef_{eye} is in centimeters.
Refracting telescope angular magnification
For a simple two-lens telescope, M=−fobj/feyeM=-f_{obj}/f_{eye}; the minus sign indicates inversion.
Newtonian reflecting telescope
A concave primary mirror focuses light onto a small secondary mirror, which redirects it sideways to the eyepiece.
Chromatic aberration
Color fringing and image blur caused by different colors refracting by different amounts through a lens.

Quiz questions

  1. In many microscopes described by the standard tube-length convention, what distance is called the tube length?Answer: The distance between the objective's image-side focal point and the eyepiece's object-side focal point.
  2. For a simple two-lens refracting telescope, which expression gives angular magnification?Answer: M=−fobj/feyeM=-f_{obj}/f_{eye}
  3. In a Newtonian reflecting telescope, what does the small secondary mirror do?Answer: It redirects light from the primary mirror sideways to the eyepiece.
  4. Why can a reflecting telescope avoid chromatic aberration from its primary light-gathering element?Answer: Reflection does not refract different colors by different amounts.
  5. What distinguishes the secondary-mirror arrangement of a Cassegrain telescope?Answer: A convex secondary sends light back through a hole in the primary mirror.

Based on University Physics Volume 3 by Samuel J. Ling, Jeff Sanny, William Moebs (OpenStax), licensed CC BY 4.0. Adapted into a summary, flashcards and quizzes.

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