SCT CollimationPosted By Ron Zick |
For the optics experts out there,
I have noticed on my Meade 12" LX200, which stays on a permanent pier mount in my observatory, that the apparent collimation seems to change with temperature conditions, or more precisely with the guide tube lube viscosity. My scope does not have any more more slop than any other sct I've seen and actually less than most.
The question I have for the optics experts is, "At what rate does the primary mirror tilt cause image degradation?"
I have not taken my scope a part to take some measurements but by making some assumptions:
1) .00015in. clearance between the slide tube and mirror carrier
2) the tempature expansion coefficient for the tube and the carrier is the same
3} the effect of the slide tube grease on clearance is zero, which I know is incorrect but I am only trying to simplify the problem definition
4) the mirror o.d. is 12in. and the slide tube od. is 3in.
I have concluded that the .00015 clearance on the tube, which probably is on the tight side, would yield a total tilt envelope of +- .0024" at the outer mirror edges. This is about double what we can manual resolve the focus to on our scopes and with an electric focuser we can probably resolve the focus increments to .0005" or less.
It seems to me +-.0024" is a lot of probable error compared with the focusing movement resolution and that this would have to have a huge effect on image quality. All of the formulas I have come across, always assume an optical system in perfect collimation.
If what I have observed is true, is this why the larger scopes don't tend to perform on average to the smaller counter parts and especially the refractors, central obstruction issues aside?
thanks in advance for any insights and answers
I have noticed on my Meade 12" LX200, which stays on a permanent pier mount in my observatory, that the apparent collimation seems to change with temperature conditions, or more precisely with the guide tube lube viscosity. My scope does not have any more more slop than any other sct I've seen and actually less than most.
The question I have for the optics experts is, "At what rate does the primary mirror tilt cause image degradation?"
I have not taken my scope a part to take some measurements but by making some assumptions:
1) .00015in. clearance between the slide tube and mirror carrier
2) the tempature expansion coefficient for the tube and the carrier is the same
3} the effect of the slide tube grease on clearance is zero, which I know is incorrect but I am only trying to simplify the problem definition
4) the mirror o.d. is 12in. and the slide tube od. is 3in.
I have concluded that the .00015 clearance on the tube, which probably is on the tight side, would yield a total tilt envelope of +- .0024" at the outer mirror edges. This is about double what we can manual resolve the focus to on our scopes and with an electric focuser we can probably resolve the focus increments to .0005" or less.
It seems to me +-.0024" is a lot of probable error compared with the focusing movement resolution and that this would have to have a huge effect on image quality. All of the formulas I have come across, always assume an optical system in perfect collimation.
If what I have observed is true, is this why the larger scopes don't tend to perform on average to the smaller counter parts and especially the refractors, central obstruction issues aside?
thanks in advance for any insights and answers