Stargazing Telescope Illumination: Mirror Diameter & Focal Length

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Illumination in telescopes, defined as flux per unit area, is directly influenced by the mirror diameter; larger apertures capture more light. The relationship between focal length and illumination is more complex, particularly for viewing telescopes with eyepieces. Point objects like stars and extended objects such as nebulae may exhibit different illumination characteristics due to their distinct light profiles. Understanding these principles is essential for optimizing telescope performance. Resources like Sky and Telescope provide valuable insights into these topics for amateur astronomers.
CaptainMarvel
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Hi there,

Could somebody explain how illumination - by which I mean flux per unit area - depends on the mirror diameter of a telescope and/or its focal length?

Is this different for point objects like stars and for extended objects like nebulae?

Thanks in advance,

Nick :-)
 
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In simple terms the larger the aperture, the more light you can capture.
It's a terrible shame to be a little photon thqat has made it across the universe and then hits the ground just outside your telescope lens!
The effect of focal length and magnification is a little more complicated, assumign you are talking about a viewing telescope (ie with an eyepiece rather than a camera)
This article is a good introduction http://www.skyandtelescope.com/equipment/basics/3077091.html?page=1&c=y Sky and Telescope is a good source of articles on amateur astronomy.
 
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