A beam of parallel light is incident normally on a diffraction grating having 550 lines per mm. A
 telescope is used to observe the second order in the spectrum. Calculate the angular separation in radians of two spectra lines of wavelengths 559nm and 563nm.
Here,
"\\lambda=559\\ nm\\\\\\lambda+\\Delta \\lambda=563\\ nm"
"\\Delta \\lambda=(563-559)nm=4\\ nm"
"m=1\\\\d=1\/550\\ =2\\times 10^{-6}m"
 Now,
sinα1= mλ1/d
sinα2= mλ2/d
Substracting the two gives:
sinα1- sinα2= m(λ1-λ2)/d
Since the angles are small, we approximate sinα≈α to get the separation:
Angular separation "\\alpha_1- \\alpha_2=\\dfrac{m(\\lambda_1-\\lambda_2)}{d}"
"= \\dfrac{1(563-559)\\times 10^{-9}} {2\\times 10^{-6}}=2\\times 10^{-3}"
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