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in partnership with the Dill Faulkes Educational Trust

 

Space-based Telescopes

The best thing about putting telescopes in space is that there is no atmosphere to look through! 

This means that they can look at all wavelengths of light, including ones that never reach the surface of the Earth because the atmosphere blocks them out!

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Artist's illustration of the James Webb Space Telescope. There is a gold mirror on top made of connected small, hexagon shapes. This sits on a triangular base that appears to have a pink hue underneath it. A small solar panel is visible towards the back. The background is a black-grey night sky with countless small, white dots of stars, varying in size. Most of the stars are located towards the middle, forming a brighter, thick band that runs from almost the top-left corner to the middle-right of the image.
Credit
This work by NASA GSFC/CIL/Adriana Manrique Gutierrez is licensed under Creative Commons Attribution 4.0 International
Artist's conception of the James Webb Space Telescope

Instruments

When people first used telescopes, they looked through them and made drawings or notes of what they saw. Then cameras were invented, and we could save this information as a picture instead.

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A 2.6-metre telescope, pointing upwards, inside its enclosure.
Credit
This work by ESO is licensed under Creative Commons Attribution 4.0 International
The VLT Survey Telescope inside of its enclosure

Optics

Optics is an area of physics which looks at how light behaves and how we can observe it. 

This usually involves using mirrors and lenses to magnify, focus, and direct the path of light.

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There is an illustration of a bulging lens on the left. A dashed line runs through the centre across the image. Two red parallel lines hit the lens towards the top and bottom and then become diagonal, crossing paths at a point labelled "F" some distance after the lens. This distance is noted with a black arrow labelled "f'".
Credit
This work by JiPaul (based on work by Henrik) is licensed under Creative Commons Attribution Share Alike 4.0 International
Light (red lines) passing through a convex lens. The point at which the light meets (F') is called the focus. The distance from the lens to the focus (f') is called the focal length.