Why does the 500 rule divide by focal length in astrophotography?

Asked 8/15/2018

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I’m new to astrophotography and trying to understand the 500 rule for avoiding star trails. Why do you divide by focal length? How does focal length affect visible star trailing on the sensor? I know the rule is only approximate, but I’m curious about the reason behind it.

Originally by Photography Stack Exchange contributor. Source · Licensed CC BY-SA 4.0

Photography Stack Exchange contributor

7y ago

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Because longer focal length is greater magnification increasing the size of image objects, including the length of of star trail blur.

The original 500 rule was for 35 mm film. However, it does not take other sensor size into account, but that is also a trail length factor. See my calculator about the 500 rule, https://www.scantips.com/lights/stars.html

Originally by user38978. Source · Licensed CC BY-SA 4.0

user38978

7y ago

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Because focal length changes magnification. The stars are moving across the sky at the same apparent rate, but a longer lens magnifies that motion more on the sensor, so the same exposure time produces a longer visible trail.

With a wide-angle lens, that motion is spread across a larger field of view, so the stars appear to move less during the exposure. With a telephoto lens, the field of view is narrower, so the same sky movement takes up more pixels and blur becomes obvious sooner.

That’s why the rule uses exposure time divided by focal length: as focal length increases, your maximum shutter speed before trails show up gets shorter.

Also, the original 500 rule was based on 35mm film, so sensor size matters too. Smaller sensors effectively crop the image, making star movement look larger in the final image, so the basic 500 rule is only a rough guideline.

UniqueBot

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7y ago

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