Calculating Light Spot Size on the Moon for a Diffraction-Limited Laser Beam

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Homework Help Overview

The discussion revolves around calculating the size of a light spot produced by a diffraction-limited laser beam on the surface of the moon, given specific parameters such as the beam diameter and wavelength. The problem involves concepts from optics and diffraction.

Discussion Character

  • Exploratory, Assumption checking, Conceptual clarification

Approaches and Questions Raised

  • Participants discuss the application of the small angle approximation and its implications for calculating the angle related to the width of the central maximum. There are questions about whether the angle pertains to the width of the central spot or the first minimum, leading to differing interpretations of the problem.

Discussion Status

The discussion is ongoing, with participants exploring different interpretations of the angle and its relevance to the size of the light spot. Some guidance has been offered regarding the role of the distance to the moon in the calculations, but there is no explicit consensus on the correct approach or final answer.

Contextual Notes

Participants are navigating assumptions about the definitions of spot width and the significance of the distance to the moon in their calculations. There is a concern regarding the reasonableness of the calculated spot size.

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Homework Statement


A laser is a light source that emits a diffraction-limited beam (like waves diffracting through a wide slit) of diameter 2 mm. Ignoring any scattering due to the Earth's atmosphere, calculate how big a light spot would be produced on the surface of the moon, 240,000 miles away. Assume a wavelength of approximately 600 nm.

Homework Equations


d = 2mm
L = 240,000 miles
λ = 600nm

The Attempt at a Solution



I am using a small angle approximation where Θ = λ/d from dsinΘ = λ

And so, converting the proper units, we have
Θ = (6e-7)/0.002 = 0.0003

Angle is a dimensionless unit, so this seems to be correct.

Now, if I wanted to find how big the light spot is, do I simple do
tanΘ = x/240,000 => 240,000*tan(0.0003) = x = 72 miles

Looking good?
 
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RJLiberator said:
I am using a small angle approximation where Θ = λ/d from dsinΘ = λ
Is that the angle for the width of the central spot ?
 
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Yes, I believe that is true. It is the angle for the width of the central maximum.
 
These guys think differently. Depends on how you define the width, I suppose. I had in mind this is the expression for the angle for the first minimum and was inclined to multiply by 2.
 
So, the 240,000 miles plays no part in this question then? eh?
 
Er, my answer seems to be incorrect. A laser would create a 72 mile bright spot on the moon? That doesn't seem reasonable. mmm.
 
RJLiberator said:
So, the 240,000 miles plays no part in this question then? eh?
It does play a role and you did that correctly. My hunch is they want the distance between the two minima on either side. And a 144 miles spot isn't all that big when seen from Earth (namely a viewing angle of ## \arctan 0.0006## :smile:).
 
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BvU, you were absolutely correct. He accepted both answers, but he did mention the factor of 2.

Thank you for the help.
 

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