AQA A Level Physics

Revision Notes

9.1.8 Charge-Coupled Devices (CCDs) in Astronomy

Charge-Coupled Devices (CCDs)

  • A charge-coupled device (CCD) is a detector which is highly sensitive to photons, making it ideal for use in the detection system of modern telescopes
    • Incident photons cause electrons to be released
    • The number of electrons released is proportional to the intensity of the incident light
    • An image is formed on the CCD, which can be processed electronically to give a digital image

A charged-coupled device

9-1-8-ccd

A charged-couple device has had a huge impact on modern astronomy

Quantum Efficiency

  • Quantum efficiency (QE) is defined as

The percentage of incident photons which cause an electron to be released

  • It can also be written as

quantum efficiency (QE) = fraction numerator n u m b e r space o f space e l e c t r o n s space p r o d u c e d space p e r space s e c o n d over denominator n u m b e r space o f space p h o t o n s space a b s o r b e d space p e r space s e c o n d end fraction cross times 100 percent sign

  • In a perfect device, the quantum efficiency will be 100% if every photon generates a photoelectron
    • However, in practice, the quantum efficiency will be less than 100% since there will usually always be unavoidable losses
  • Some values of QE for different devices are shown in the table
Device Quantum efficiency (%)
human eye 1−4%
photographic film 4−10%
CCD 70−90%

 

  • Comparison of the eye and a CCD:
    • CCDs are renowned for achieving high values of quantum efficiency, generally upwards of 80%, whereas a human eye is only capable of achieving around 1%

Resolution of a CCD

  • The resolution of a CCD is related to the total number of pixels per unit area, and their size
    • The smaller the size of the pixel, the better the resolution, hence the clearer the image will be
  • The typical resolution of a CCD is about 10 μm
  • In comparison, the typical resolution of the human eye is about 100 μm, but it can vary widely
  • In most cases, the overall resolution of a telescope is limited by the diameter of the objective
    • Hence, the resolution of the CCD (or the eye) is not likely to make a difference to the final image observed

Convenience of a CCD

  • CCDs have an edge over the eye in terms of convenience because:
    • The number of images captured in a time period and exposure time can be easily adjusted
    • The information stored on a CCD can be accessed remotely
    • The generated images can be stored and analysed digitally
    • They can detect a larger range of wavelengths, including beyond the visible spectrum

Comparison of a CCD with the human eye 

  • The main comparisons between the eye and a CCD are summarised in the table
Device Quantum efficiency (%) Resolution Convenience of use
human eye
  • Very low ~1%
  • Typical resolution ~100 μm
  • No additional equipment required
CCD
  • Very high 70%+
  • Able to detect much fainter objects
  • Typical resolution ~10 μm
  • Resolution can be increased by using smaller pixels
  • Remote viewing
  • Images can be stored and analysed digitally
  • Long exposure times
  • Can detect a wider range of wavelengths

Exam Tip

You may see past exam questions on the operation and structure of the CCD, but this knowledge is no longer required - the focus is now on the comparison between the CCD and the eye.

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