Solve Optics Problem: Diameter of Star Imaged w/ 18" Telescope

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Homework Help Overview

The discussion revolves around an optics problem involving a telescope with an 18-inch aperture and a focal length of 120 inches. Participants are tasked with determining the diameter of a star imaged at the focal plane, specifically related to the first minimum in the diffraction pattern, using a wavelength of 550 nm.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants inquire about the equation for diffraction at a circular aperture and discuss the integral formulation related to the diffraction pattern. There is mention of Rayleigh's criterion in relation to the angular width of the central maxima.

Discussion Status

The discussion includes various approaches to understanding the diffraction pattern and its implications for the imaging of a star. Some participants have provided hints and references to established principles, but there is no explicit consensus on a complete solution yet.

Contextual Notes

Participants are working within the constraints of the problem as posed, including the specific parameters of the telescope and the wavelength provided. The discussion reflects an exploration of diffraction theory without resolving the final outcome.

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Optics Problem( pleasez help me)

Consider a telescope with an aperture of 18 inches and focal length of 120 inches.
what is the diameter of the star imaged in focal plane of telescope? Take the image diameter to be associated with the first minimum in the diffraction pattern of the image. Use wavelength of 550nm.

Hint: By Using lens diffraction theory.
 
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What is the equation for diffraction at a circular aperture?
 


hiiiiiiii friend.,

for the circular aperture

U= C exp(ikr) * integral of Exp(ikysin@) 2sqrt(R^2-Y^2) dy
bet ween the limits (-R,R)
 
Last edited:


The nice Mr Rayleigh solved it for you
 


In other words 1.22 times wavelength divided by aperture diameter for the half angular width of the central maxima.
 

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