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The above observations are only valid when the distance between the slit and the screen is large
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Spectrographβ¨
An instrument used to obtain and record an astronomical spectrum by splitting or dispersing the light from an object into its
component
wavelengths
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Ways to split or disperse light into a spectrum
Using a
prism
Using a
diffraction grating
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Most astronomical spectrographs use
diffraction gratings
rather than
prisms
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Diffraction gratings
β¨
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
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Diffraction gratings
are more
efficient
than prisms, which absorb some of the light passing through them
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Every incident photon is precious when trying to get a spectrum from a
faint source
, so scientists prefer using a
diffraction grating
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The response of a diffraction grating is
linear
, whereas a
prism
disperses the blue light much more than the red part of the spectrum
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Main components of a modern slit spectrometer
Slit
Collimating mirror
Diffraction grating
Detector
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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
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The collimator focuses the
light
onto the
diffraction grating
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The
diffraction grating
splits the light into its
constituent colours
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The
spectrum
is finally captured by a
detector
or a camera lens and fed into a computer for further analysis
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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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