How Do You Calculate the Focal Length of a Planar Convex Lens?

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SUMMARY

The focal length of a planar convex lens can be calculated using the formula \(\frac{1}{f} = \left(\frac{n}{n_M} - 1\right) \left(\frac{1}{r_1} + \frac{1}{r_2}\right)\). In this case, with a curvature radius |r| of 50cm, the refractive index n is 1.491, n_M is 1, r_1 is 50cm, and r_2 is considered infinitely large. The focal length is determined under the assumption that only paraxial rays, which are rays close to the optical axis, are considered, ensuring the validity of the formula.

PREREQUISITES
  • Understanding of lens optics and refraction principles
  • Familiarity with the lens maker's equation
  • Knowledge of paraxial approximation in optics
  • Basic mathematics involving fractions and algebraic manipulation
NEXT STEPS
  • Study the derivation of the lens maker's equation in detail
  • Learn about the significance of paraxial rays in optical systems
  • Explore the impact of different refractive indices on focal length calculations
  • Investigate practical applications of planar convex lenses in optical devices
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Students of optics, physics enthusiasts, and professionals in optical engineering who are involved in lens design and analysis.

Icheb
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Light is falling on the planar side of a thin planar convex glass lens. The curvature radius |r| is 50cm. I have to calculate the distance of the focal point to the curved surface of the lens, which to my understanding is the focal length, since it's a thin lens. Additionally I am supposed to only look at rays that are close to the axis, and I'm not sure what exactly that means.

From my understanding the only equation I need is [tex]\frac{1}{f} = (\frac{n}{n_M} - 1) (\frac{1}{r_1} + \frac{1}{r_2})[/tex]. n would be 1,491, n_M would be 1, r_1 would be 50cm and r_2 would be infinitely big (since the lens is planar convex).

Would that be sufficient to solve it? If so, what does it mean that I'm only supposed to look at rays that are close to the axis? What does that change?
 
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If you study the derivation of the formula for ##\frac{1}{f}##, you'll see that the derivation assumes that the rays are close to the axis ("paraxial rays"). So, the formula is generally valid only for paraxial rays.

When using the formula, you need to be sure to use the sign conventions for ##r_1##, ##r_2##, and ##f## that are associated with the formula.
 

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