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Vega Final Focusing Takahashi 180 ED Collimation Project, Jerry Yesavage

Vega Final Focusing Takahashi 180 ED Collimation Project

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Description

For those of you that have suffered along with me the collimation of my Takahashi 180 ED, I thought I should post one more technical shot (if anyone every searches on the topic they will find this).

So, how come this scope is so hard to get in collimation and focus, well because it is F/2.8. Remember, as I have relearned, that the F ratio in addition to defining aperture width defines depth of field. This can be calculated:

2.8*2.8*2.2 or 17.248 microns or 0.017248 mm or 0.0006791”… in other words the depth of field for critical focus is about 1/100th of a mm, way less than a mil.

From Wikipedia: A human hair is only anywhere from 40 to 120 microns thick.

I gave up on the Bahtinov mask and eventually chose a bright star with its own spikes. This was the problem in the images... spikes would not be symmetrical... could not get the whole image into that tiny plane. I could use this to get the imaging into the very narrow plane.

Anyway, I publish this here for future references.

I am not going to move the settings on the scope. Thanks to the folks from SBIG, Takahashi USA and Hotech lasers.

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Vega Final Focusing Takahashi 180 ED Collimation Project, Jerry Yesavage

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