Find Telescope Diameter to Resolve Two Stars

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SUMMARY

The discussion focuses on calculating the diameter of a telescope required to resolve two stars separated by an angle of 3x10-5 radians, emitting monochromatic light at 600nm. Using the formula for angular resolution, Δθ = 1.22 λ / D, the diameter D is determined to be 2.44 cm. The constant 1.22 is derived from Rayleigh's criterion, which relates to the diffraction pattern produced by a circular aperture. The final conclusion confirms that a telescope diameter of approximately 2.5 cm is necessary for resolution.

PREREQUISITES
  • Understanding of Rayleigh's criterion in optics
  • Familiarity with Fraunhofer diffraction patterns
  • Basic knowledge of monochromatic light properties
  • Ability to manipulate and rearrange mathematical formulas
NEXT STEPS
  • Study Rayleigh's criterion in detail to understand its applications in telescope design
  • Learn about Fraunhofer diffraction and its significance in optics
  • Explore the properties of monochromatic light and its impact on resolution
  • Investigate the mathematical derivation of Bessel functions related to diffraction patterns
USEFUL FOR

Astronomy students, optical engineers, and anyone involved in telescope design or studying light diffraction will benefit from this discussion.

dimensionless
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I have two stars that are separated by an angle of 3x10^5 radians. They are both emitting monochromatic light on 600nm. I would like to find the diameter of the smallest telescope that can resolve the two stars.

For the angular limit of resolution I have
[tex] \Delta \theta = \frac{1.22 \lambda}{D}[/tex]

Where D is the diameter of the lens.

Rearranging I get
[tex] D = \frac{1.22 \lambda}{\Delta\theta}=\frac{1.22*600*10^{-9}}{3*10^{-5}} = 2.44 cm[/tex]

I'm quite sure that the answer is 2.5 cm. Where am I going wrong? Where does the 1.22 come from?
 
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dimensionless said:
I'm quite sure that the answer is 2.5 cm. Where am I going wrong?
I don't think you're going wrong at all.
Where does the 1.22 come from?
The resolution limit you are using is called Rayleigh's criteria. The 1.22 comes from calculating the diameter of the first dark ring of the Fraunhofer diffraction pattern due to a circular aperature (which involves finding the zeros of a Bessel function--look it up if you want more).
 

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