# How does this spectroscope work?

• Phys12
In summary, the spectroscope works by focusing a light source onto an entrance slit and then using a lens or concave mirror to direct the parallel rays onto a prism or diffraction grating. The light then emerges as parallel rays at different angles depending on the wavelength, and these rays are brought to focus on an exit slit. By rotating the prism or diffraction grating, the colors of the rainbow can be rotated and only one color will be focused on the exit slit at a time. This explains why the spectrum changes when the orientation of the spectroscope changes. Additionally, the difference in what is seen through a camera and with the human eye is due to the different angles that each can view the spectroscope at.
Phys12
I build the following spectroscope:

However, I'm not sure how it works. I thought that the light entered the slit, diffracted from the CD (because the tracks in them are comparable to the wavelength of visible light) and then we observe the different components in the camera.(https://www.exploratorium.edu/snacks/cd-spectroscope)

The explanation here (https://www.livescience.com/41548-spectroscopy-science-fair-project.html) says that light gets diffracted from the slit by interfering itself forming the interference pattern (the rainbow) and then reflects off the CD and then that's what we see.

Which one is true?

P.S. When I look at light from one angle, I see the following:
https://ibb.co/mSvo1x
But when I rotate it by 90 degrees, I see:
https://ibb.co/j6UsTc
Why is it the case of the orientation of the spectroscope changes the spectrum seen? If the orientation of the slit and the CD are the same, shouldn't it stay the same?

Also, I don't see the same two distinct spectrum when I look at the spectroscope with my eyes, I see multiple in different directions. Why is it different for a camera vs eyes?

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Usually the slit widths of a spectrometer are chosen wider than what would cause appreciable diffraction. The light source whose spectrum is to be measured is focused onto the entrance slit. ## \\ ## Inside of the spectrometer is a lens or concave mirror whose focal point is on the entrance slit. This way the light comes off of the first optic as parallel rays that are incident onto either a prism or diffraction grating. The light emerges from the prism or diffraction grating as parallel rays that have a direction that is wavelength dependent, i.e. parallel rays of wavelength ## \lambda_1 ## will emerge at angle ## \theta_1 ##, parallel rays of wavelength ## \lambda_2 ## will emerge at angle ## \theta_2 ##, etc. In general, for a broad spectrum source, parallel rays emerge at a wide variety of angles ## \theta ##, where ## \theta ## is a function of wavelength ## \lambda ##, i.e. ## \theta=\theta(\lambda) ##. ## \\ ## The parallel rays are then brought to focus in the plane of the exit slit by a second lens or concave mirror.(The spectrum will appear across the focal plane of this second lens or concave mirror as the colors of the rainbow). The exit slit is located at a position in the focal plane. It only gets light from one specific angle, i.e. the (focused) colors of the rainbow are spread out on both sides of the exit slit, and only one color will be focused on the exit slit at a time, so there will only be light of one wavelength emerging from the exit slit. To change the wavelength that comes out of the exit slit, the prism or diffraction grating is rotated (about a vertical axis), causing the whole pattern of the colors of the rainbow to rotate horizontally. (Note:The spectrometer slits are in the vertical direction). ## \\ ## Note: If you start with a monochromatic source, the prism or diffraction grating needs to be rotated to the proper angle to get the light coming off of the prism or diffraction grating to focus onto the exit slit. (Otherwise, it will come to a focus in the focal plane, but at a different location than right on the exit slit). When it does, the light that is focused onto the exit slit will have an image whose shape is just like that of the illuminated entrance slit. It's not completely necessary, but often times, the exit slit is chosen to be the same width as the entrance slit.

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Usually the slit widths of a spectrometer are chosen wider than what would cause appreciable diffraction. The light source whose spectrum is to be measured is focused onto the entrance slit. ## \\ ## Inside of the spectrometer is a lens or concave mirror whose focal point is on the entrance slit. This way the light comes off of the first optic as parallel rays that are incident onto either a prism or diffraction grating. The light emerges from the prism or diffraction grating as parallel rays that have a direction that is wavelength dependent, i.e. parallel rays of wavelength ## \lambda_1 ## will emerge at angle ## \theta_1 ##, parallel rays of wavelength ## \lambda_2 ## will emerge at angle ## \theta_2 ##, etc. In general, for a broad spectrum source, parallel rays emerge at a wide variety of angles ## \theta ##, where ## \theta ## is a function of wavelength ## \lambda ##, i.e. ## \theta=\theta(\lambda) ##. ## \\ ## The parallel rays are then brought to focus in the plane of the exit slit by a second lens or concave mirror.(The spectrum will appear across the focal plane of this second lens or concave mirror as the colors of the rainbow). The exit slit is located at a position in the focal plane. It only gets light from one specific angle, i.e. the (focused) colors of the rainbow are spread out on both sides of the exit slit, and only one color will be focused on the exit slit at a time, so there will only be light of one wavelength emerging from the exit slit. To change the wavelength that comes out of the exit slit, the prism or diffraction grating is rotated (about a vertical axis), causing the whole pattern of the colors of the rainbow to rotate horizontally. (Note:The spectrometer slits are in the vertical direction). ## \\ ## Note: If you start with a monochromatic source, the prism or diffraction grating needs to be rotated to the proper angle to get the light coming off of the prism or diffraction grating to focus onto the exit slit. (Otherwise, it will come to a focus in the focal plane, but at a different location than right on the exit slit). When it does, the light that is focused onto the exit slit will have an image whose shape is just like that of the illuminated entrance slit. It's not completely necessary, but often times, the exit slit is chosen to be the same width as the entrance slit.
I don't think that answers my question. In the setup that I have, is the spectrum caused by diffraction of light when it passes through the slit or when it passes through the gap between the tracks on the CD?

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## What is a spectroscope?

A spectroscope is a scientific instrument used to study the properties of light. It is able to break down light into its component wavelengths, allowing scientists to analyze the chemical composition of a substance.

## How does a spectroscope work?

A spectroscope works by directing a beam of light through a prism or diffraction grating, which separates the light into its component wavelengths. This creates a spectrum, which can then be analyzed and interpreted by scientists.

## What are the main components of a spectroscope?

The main components of a spectroscope include a light source, a prism or diffraction grating, a slit to control the amount of light entering the spectroscope, and an eyepiece or detector to observe and record the spectrum.

## What can a spectroscope be used for?

A spectroscope can be used to study the chemical composition of a substance, identify elements present in a sample, and analyze the properties of light emitted or absorbed by a substance. It is commonly used in fields such as chemistry, astronomy, and forensics.

## What are the limitations of a spectroscope?

One limitation of a spectroscope is that it can only detect wavelengths of light that are within the visible range. It is also limited in its ability to distinguish between elements with similar properties. Additionally, the accuracy of a spectroscope's measurements can be affected by factors such as the quality of the light source and the calibration of the instrument.

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