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Proud to be part of LJMU,
in partnership with the Dill Faulkes Educational Trust

 

You can use the Liverpool Telescope to observe features on the Moon’s surface. This is because the telescope has a field of view that shows small areas of the sky in lots of detail. This means that you would need to combine about 49 images from the LT to cover the entire full Moon.

In this project, you will plan observations of 3 features of the Moon during different lunar phases. You then use Go Observing to request the images of specific areas of the Moon at specific times within the lunar phase cycle. The images you collect will allow you to show and investigate how these features appear to change over time.

By the end of this activity you will:

  • Have used your knowledge of the phases of the Moon to plan a series of observations
  • Have produced detailed images of features on the Moon using the Liverpool Telescope and image software
  • Have demonstrated how the appearance of those features changes with the phases of the Moon
  • Have produced a report of your results and analysis

 

To complete this activity you will need: 

 

IT Equipment

  • Access to the internet
  • Software for viewing astronomical data files

Image
An image showing a close-up view of the moon's surface with craters on the left, alongside a grid diagram on the right. The diagram highlights a small red square, representing the small field of view of the Liverpool Telescope, which allows for detailed observations of specific areas on the moon.
Credit
This work by The Schools' Observatory is licensed under All rights reserved
The Liverpool Telescope’s small field of view allows it to observesmall areas of the Moon in great detail