If you are building a telescope or if you want to see if a telescope primary mirror has a good 'figure' before you buy it, you need to perform an optical test of the mirror.

A properly figured primary Newtonian mirror is a near-perfect parabola. How close to perfect does it need to be? A good telescope mirror has less than 1/4 wavelength of light error on its surface! This means that the surface imperfections should be smaller than 100 nm.  This is a very small margin for error but amateurs telescope makers can achieve this and better if they are persistent and careful.

In order to test the figure of the primary mirror we must build the following:
Mirror mount,
Optical tester,
Optical mask

Then I'll describe how to use these tools to determine the figure.

Step 1: Theory of Operation

The 100 nm accuracy of the surface requirement is a very tight tolerance and can not be measured directly using such things as rulers or depth gauges.  These tight tolerances can indeed be achieved using normal hand tools by magnifying the surface angles.  We can find the focus point of the mirror by shining a narrow slit of light onto the mirror and observing the shadows as a knife edge is passed in front of the returning light.

Let us assume that we have a perfectly shaped spherical mirror and our knife edge is near the focus point of the mirror.

See Figure A.
Looking down from the top, if we illuminate the mirror at the focus point the light will hit the mirror and return exactly to the focus point.

See Figure B.
If we move a knife edge inside the focus and on the right, the knife edge blocks the light returned from the right side of the mirror and does not affect the light from the left side of the mirror.

See Figure C.
If we move the knife edge outside the focus and on the right, the knife edge blocks the light returned from the LEFT side of the mirror.

So, when the knife edge is inside the focus, moving the knife edge left and right makes a shadow move across the mirror in the same direction as the movement of the knife edge.
When knife edge is outside the focus, moving the knife edge left and right makes a shadow move across the mirror going in the opposite direction of the knife edge.
When the knife edge is exactly at the focus point and the knife edge is moved from left and right, the mirror dims uniformly, i.e. the shadow doesn't appear to move left or right but the entire mirror dims.

A good telescope mirror does not have a spherical shape but a parabolic shape. For a parabola, the outer areas of the mirror focuses farther away from the inner areas of the mirror. We can therefor use this knowledge to determine the precise shape of the mirror by finding the focus points of each area of the mirror.
This is a great explanation of the results of the knife edge test, which for some reason are very hard to find. Lots of people talk about this device but don't explain what the results indicate. My mirror has issues, but now I can (maybe) pinpoint them. Thank you for this.
Thanks for your kind words and best of luck with your mirror!
decades ago when i was doing my own mirror, one had to do that with the ' Foucault test' and basically just eyeball it, which I never could grasp. This seems to be the same principle but with a bit more measuring behind it. Great
Yes, this method requires precise measurement to achieve the 1/4 wavelength or better surface. Thanks.
Great 'ible ! <br> <br>Steve
At last some easy way to do tjis. From many years I wanted to build a telescope, but this part of the process allways stoped me. Now I dont'n have but to start.
The WEB has a lot of information that can help you. One noteworthy site is: http://stellafane.org/tm/atm/index.html <br> <br>Best Wishes!
Very nice. <br>I got an education as i didn't know about measuring a mirror's focal point or even a tool to do this.
Thank you for your kind comments!
Great instructible! I never understood how people could grind their own mirrors, but this makes sense.
Thank You. This is one of those instructables I started over a year ago and thought I'd just finish it up. It is amazing to me that Sir Isiac Newton and others knew these techniques many many years ago. <br> <br>The grinding process (not discussed) employs a glass or ceramic 'tool' rubbed against the glass disk with successively finer grits of aggregate and water. <br> <br>To actually polish the glass to a smooth figure you use pitch which I believe is a petrolium product. It is like a very think liquid, hard to the touch but yet maluable as you can leave a mark with your thumbnail. How it works is still a bit of a mystery to science (so I'm told) but it appears the glass is melted and refrozen on a microscopic scale as the tool with the pitch layer is rubbed against the glass disk. <br> <br>Thanks again for the nice comments. <br> <br>Best Wishes

About This Instructable




Bio: I'm an aerospace engineer by trade but am interested in astronomy, robotics, CNC machines, Arduinos, you name it.
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