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resources/links/Angular resolution.md
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**_SO THE GOAL BECOMES HOW TO MAKE IMAGES WITH SMALL ANGULAR RESOLUTIONS._**
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It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength
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$\lambda$ giving by $$ \theta = 1.22 \frac{\lambda} {D} $$
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- Where $D$ is the diameter of the telescope.
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- to get better resolution (small $\theta$), we need:
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- Large lenses ($D$)
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