Physics πŸ“šπŸ“Œ

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    • The above observations are only valid when the distance between the slit and the screen is large
    • Spectrograph

      An instrument used to obtain and record an astronomical spectrum by splitting or dispersing the light from an object into its component wavelengths
    • Ways to split or disperse light into a spectrum
      • Using a prism
      • Using a diffraction grating
    • Most astronomical spectrographs use diffraction gratings rather than prisms
    • Diffraction gratings

      • Consist of thousands of narrow, closely spaced parallel slits
      • Due to interference, the intensity of the light travelling through the slits depends on the wavelength and direction of propagation
    • Diffraction gratings are more efficient than prisms, which absorb some of the light passing through them
    • Every incident photon is precious when trying to get a spectrum from a faint source, so scientists prefer using a diffraction grating
    • The response of a diffraction grating is linear, whereas a prism disperses the blue light much more than the red part of the spectrum
    • Main components of a modern slit spectrometer
      • Slit
      • Collimating mirror
      • Diffraction grating
      • Detector
    • The slit allows only a small portion of incident light required for the spectral analysis to enter the spectrograph, and helps to filter out any stray light
    • The collimator focuses the light onto the diffraction grating
    • The diffraction grating splits the light into its constituent colours
    • The spectrum is finally captured by a detector or a camera lens and fed into a computer for further analysis
    • Figure 9.32 shows the schematic diagram and the main components of a slit spectrograph used for spectral analysis of the light from the stars
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