Refraction: Lens And Reflection

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The refractor telescope is a telescope that uses lenses and refraction in order to magnify images.

Light travels in a wave with differing speeds. A medium (or media) is any one type of transparent matter e.g. Air, Glass, Water or a lack of matter (A vacuum) . The optical density of a medium is the amount that it slows light down when light is passing through it .This means light travels at different speeds in different mediums Because of this the light wave will refract (bend) when it passes from one medium to another. Not all of the light rays will undergo reflection while the others will undergo refraction. Refraction is where when light travels from one one medium to another it changes speed and this causes the light waves to bend as seen …show more content…

The effect of these refractions is that the image is magnified and if the second eyepiece is convex is inverted.

The equation used to calculate lenses (descartes formula) can be also used to calculate the refractor telescope. The equation is:
1f=1d0+1di
This is equation can be applied to the refractor telescope to find the nature of the image and where the image will form. This is important because it gives us insight into the image and its properties which allows us to better understand the light rays.

A refracting telescope magnifies a distant object by using a large aperture objective lens a large objective lens focal length compared to the eyepiece lens focal length. The following equation is used to calculate the magnification of an image through a telescope:
Magnification(m)=Focal length of objective lens(F)/Focal length of eyepiece lens(f)
This equation gives the relationship between the focal lengths of the two lenses in the refracting telescope. This relationship can be observed below with an example of the two lenses and the difference in focal

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