<blockquote>
  <p>How is it ensured that a parabolic shape forms while polishing a telescope mirror?</p>
</blockquote>

<p>While a spherical shape is fairly easy to abtain, a parabolic shape definitely isn't!</p>

<p>It's a combination of special polishing strokes, and feedback via control and testing.</p>

<p><a href="https://stellafane.org/tm/atm/mirror-refs/strokes.html" rel="nofollow noreferrer">https://stellafane.org/tm/atm/mirror-refs/strokes.html</a></p>

<p>Normal polishing strokes (center over center, 1/3 diameter amplitude) tend to make a sphere. When all goes well, the surface of the mirror tends to become spherical, or very close to it. This is not different from grinding, only more precise. When two surfaces are rubbing against each other in a ball-and-socket type of joint, any irregularities will be removed and both surfaces will "want" to become spherical, or close to it.</p>

<p>When making telescope mirrors, the so-called "normal stroke" is what accomplishes that in the best way.</p>

<p><a href="https://i.sstatic.net/dKj1j.gif" rel="nofollow noreferrer"><img src="https://i.sstatic.net/dKj1j.gif" alt="enter image description here"></a></p>

<p>Now here's the essential detail: no matter what other curve you're trying to obtain (parabola, hyperbola, ellipse), for the purpose of making telescope mirrors all these curves are very close to a circle, within a fraction of a micron.</p>

<p>So a typical process has an initial goal of making a sphere (cross-section is a circle). This is not mandatory, but it's easier to first make a sphere, and then apply "corrections" to it. You can definitely make a parabola directly, but the process is more complex.</p>

<p>For telescope mirrors, the parabola that's needed is basically a circle that's deeper in the center, and more shallow towards the edge. So, if you start with a spherical mirror (circular section) and use polishing strokes that tend to deepen the center in a gradual way, you can get pretty close to a parabola. This is known as a "parabolizing stroke".</p>

<p><a href="https://i.sstatic.net/JAzZK.gif" rel="nofollow noreferrer"><img src="https://i.sstatic.net/JAzZK.gif" alt="enter image description here"></a></p>

<p>Keep in mind that as you apply that stroke, the center keeps deepening. At some point the correction will become deeper than a parabola and the mirror will become hyperbolic. That's sometimes what you actually need (if you make a hyperbolic mirror for a Ritchey-Chretien telescope). Or if you stop too early, the mirror is elliptic, which is used in other designs. The parabola is the thin edge between the elliptic and hyperbolic domains.</p>

<p>You start with a mirror where the cross-section is a circle (spherical mirror). You begin to apply the W stroke. The circle immediately becomes a very shallow ellipse, which keeps deepening. At some point, for a very short time, that ellipse becomes a parabola. As you keep doing the W stroke, the parabola then changes quickly and now you have a hyperbola which just becomes more and more deep.</p>

<p>The key here is testing. You apply the parabolizing stroke for a short while, then stop and test the mirror. There are many testing techniques; the Couder mask is simple enough and very popular; or you could use an interferometer if you have (or can build) one. Is it still elliptic? Keep parabolizing. Has it become hyperbolic? Reset to a sphere and try again. Or adjust the stroke if either the edge or the center are being corrected too fast.</p>

<p>Apply parabolizing strokes. Test. Modify technique if necessary. Repeat. That's all there is to it.</p>

<hr>

<p><strong>Note:</strong> I am using jargon in the text above. "Deeper" really means "more strongly curved". "Shallower" really means "less strongly curved". The difference between circle and parabola is that the parabola is more strongly curved in the center, while the curvature at the edge is less strong. The circle has constant curvature everywhere, by definition.</p>

<p>This doesn't necessarily mean the center of the mirror is physically more depressed; while doing any strokes, the whole surface keeps being polished down all the time. But the relative curvatures of center vs. edge may change.</p>

<p>Deeper vs shallower are terms that reflect the physical process, whether the tool applies more or less pressure on a certain area of the mirror (so polishing goes faster or slower there). But the geometric attribute that the process actually changes, that we are interested in, is the radius of curvature. Where the tool applies more pressure, the radius of the curvature decreases rapidly (the surface becomes more strongly curved).</p>

<p>Deeper and shallower are practical terms related to process. More or less strongly curved are theoretical terms related to geometry. When you make mirrors, after a while these terms become linked in your mind.</p>

<hr>

<p>It helps if you're familiar with the conic sections:</p>

<p><a href="https://en.wikipedia.org/wiki/Conic_section" rel="nofollow noreferrer">https://en.wikipedia.org/wiki/Conic_section</a></p>

<p><a href="https://i.sstatic.net/dqfIN.png" rel="nofollow noreferrer"><img src="https://i.sstatic.net/dqfIN.png" alt="enter image description here"></a></p>

<p><a href="https://i.sstatic.net/tRMfS.png" rel="nofollow noreferrer"><img src="https://i.sstatic.net/tRMfS.png" alt="enter image description here"></a></p>

<p>red = circle</p>

<p>orange = ellipse</p>

<p>green = parabola</p>

<p>blue = hyperbola</p>

CC BY-SA 4.0
2019-09-12T11:16:30.180Z
`+1` I hope you don't mind the small edit to this excellent answer! fyi I've just asked the following mirror-making-relaged question: [Why is this telescope so short? How hard is it to make such a fast primary?](https://astronomy.stackexchange.com/q/33337/7982)
uhoh
CC BY-SA 4.0
2018-02-13T20:45:14.143Z
2019-09-12T11:15:20.513Z
2019-09-12T11:15:20.513Z
Florin Andrei
<p>I understand polishing the mirror with a successively finer abrasive can create a curvature, but how is it possible to obtain a uniform curve that forms a parabola while polishing by hand?</p>

CC BY-SA 3.0
2018-02-14T13:10:55.973Z
@FlorinAndrei  I've seen machines with precision better than that, albeit expensive.  However, what I was suggesting was a jig which cuts a parabolic shape to begin with, rather than starting with a sphere and 'morphing' to a parabola via radius-dependent grind time.
Carl Witthoft
CC BY-SA 3.0
2018-02-16T02:59:26.173Z
@CarlWitthoft If you're talking about lens and mirror making machines, I've built one myself. But the precision of the generated surface doesn't come from the machine in the way most people think - i.e. you can't say the machine has a precision of 0.1 microns or less. The process has that precision, and that's different.
Florin Andrei
CC BY-SA 3.0
2018-02-16T11:02:55.017Z
Also, in grinding the precision is far too low to even matter whether you're aiming for a sphere or a parabola. It doesn't matter at all. Don't waste your time making jigs. The emphasis in this stage is not on precision, but on removing glass (rough grinding) and smoothing out the surface (fine grinding). It's only later in polishing and figuring that the distinction is meaningful. I'm talking here exclusively about optics for the IR / visible / UV range. All this would be much clearer if you actually go through the process of making optics at least once.
Florin Andrei
CC BY-SA 3.0
2018-02-13T14:17:02.967Z
These are two useful links : [Joy of Mirror Making](http://www.bbastrodesigns.com/JoyOfMirrorMaking/RoughGrinding.html) and [Parabolizing a Telescope Mirror](http://www.bbastrodesigns.com/JoyOfMirrorMaking/Parabolizing.html) both from the same very useful web site.
StephenG - Help Ukraine
CC BY-SA 3.0
2018-02-13T16:05:13.387Z
@StephenG nice pages there -- but sadly no discussion of a parabolic grinder, just how to test curve while in process.  I seem to recall some articulated jigs based on the pencil-and-string geometry approach, http://www.gizmology.net/parabola.htm , that allow you to lap the surface parabolically, but can't find a design online.
Carl Witthoft
CC BY-SA 3.0
2018-02-13T20:30:29.627Z
@CarlWitthoft No jig will ever be precise enough to polish a parabola into a telescope mirror. The acceptable error is less than 0.1 microns. The process is all about special polishing techniques that adjust an initial high precision surface, pushing it towards the desired shape.
Florin Andrei
<amateur-observing><observational-astronomy><telescope-lens><telescope-making><mirror-making>
How is it ensured that a parabolic shape forms while polishing a telescope mirror?
Maverick139
# How is it ensured that a parabolic shape forms while polishing a telescope mirror?

(Asked by: username_0 on 2018-02-13)

I understand polishing the mirror with a successively finer abrasive can create a curvature, but how is it possible to obtain a uniform curve that forms a parabola while polishing by hand?

**Tags:** amateur-observing, observational-astronomy, telescope-lens, telescope-making, mirror-making
> **Comments:**
> **username_3**: These are two useful links : [Joy of Mirror Making](http://www.bbastrodesigns.com/JoyOfMirrorMaking/RoughGrinding.html) and [Parabolizing a Telescope Mirror](http://www.bbastrodesigns.com/JoyOfMirrorMaking/Parabolizing.html) both from the same very useful web site.  
> **username_1**: @StephenG nice pages there -- but sadly no discussion of a parabolic grinder, just how to test curve while in process.  I seem to recall some articulated jigs based on the pencil-and-string geometry approach, http://www.gizmology.net/parabola.htm , that allow you to lap the surface parabolically, but can't find a design online.  
> **username_2**: @CarlWitthoft No jig will ever be precise enough to polish a parabola into a telescope mirror. The acceptable error is less than 0.1 microns. The process is all about special polishing techniques that adjust an initial high precision surface, pushing it towards the desired shape.  
> **username_1**: @FlorinAndrei  I've seen machines with precision better than that, albeit expensive.  However, what I was suggesting was a jig which cuts a parabolic shape to begin with, rather than starting with a sphere and 'morphing' to a parabola via radius-dependent grind time.  
> **username_2**: @CarlWitthoft If you're talking about lens and mirror making machines, I've built one myself. But the precision of the generated surface doesn't come from the machine in the way most people think - i.e. you can't say the machine has a precision of 0.1 microns or less. The process has that precision, and that's different.  
> **username_2**: Also, in grinding the precision is far too low to even matter whether you're aiming for a sphere or a parabola. It doesn't matter at all. Don't waste your time making jigs. The emphasis in this stage is not on precision, but on removing glass (rough grinding) and smoothing out the surface (fine grinding). It's only later in polishing and figuring that the distinction is meaningful. I'm talking here exclusively about optics for the IR / visible / UV range. All this would be much clearer if you actually go through the process of making optics at least once.  

---

## 1 answers

### Answer by username_2 on 2018-02-13. Score: 6

> How is it ensured that a parabolic shape forms while polishing a telescope mirror?

While a spherical shape is fairly easy to abtain, a parabolic shape definitely isn't!

It's a combination of special polishing strokes, and feedback via control and testing.

<https://stellafane.org/tm/atm/mirror-refs/strokes.html>

Normal polishing strokes (center over center, 1/3 diameter amplitude) tend to make a sphere. When all goes well, the surface of the mirror tends to become spherical, or very close to it. This is not different from grinding, only more precise. When two surfaces are rubbing against each other in a ball-and-socket type of joint, any irregularities will be removed and both surfaces will "want" to become spherical, or close to it.

When making telescope mirrors, the so-called "normal stroke" is what accomplishes that in the best way.

[![enter image description here](https://i.sstatic.net/dKj1j.gif)](https://i.sstatic.net/dKj1j.gif)

Now here's the essential detail: no matter what other curve you're trying to obtain (parabola, hyperbola, ellipse), for the purpose of making telescope mirrors all these curves are very close to a circle, within a fraction of a micron.

So a typical process has an initial goal of making a sphere (cross-section is a circle). This is not mandatory, but it's easier to first make a sphere, and then apply "corrections" to it. You can definitely make a parabola directly, but the process is more complex.

For telescope mirrors, the parabola that's needed is basically a circle that's deeper in the center, and more shallow towards the edge. So, if you start with a spherical mirror (circular section) and use polishing strokes that tend to deepen the center in a gradual way, you can get pretty close to a parabola. This is known as a "parabolizing stroke".

[![enter image description here](https://i.sstatic.net/JAzZK.gif)](https://i.sstatic.net/JAzZK.gif)

Keep in mind that as you apply that stroke, the center keeps deepening. At some point the correction will become deeper than a parabola and the mirror will become hyperbolic. That's sometimes what you actually need (if you make a hyperbolic mirror for a Ritchey-Chretien telescope). Or if you stop too early, the mirror is elliptic, which is used in other designs. The parabola is the thin edge between the elliptic and hyperbolic domains.

You start with a mirror where the cross-section is a circle (spherical mirror). You begin to apply the W stroke. The circle immediately becomes a very shallow ellipse, which keeps deepening. At some point, for a very short time, that ellipse becomes a parabola. As you keep doing the W stroke, the parabola then changes quickly and now you have a hyperbola which just becomes more and more deep.

The key here is testing. You apply the parabolizing stroke for a short while, then stop and test the mirror. There are many testing techniques; the Couder mask is simple enough and very popular; or you could use an interferometer if you have (or can build) one. Is it still elliptic? Keep parabolizing. Has it become hyperbolic? Reset to a sphere and try again. Or adjust the stroke if either the edge or the center are being corrected too fast.

Apply parabolizing strokes. Test. Modify technique if necessary. Repeat. That's all there is to it.

---

**Note:** I am using jargon in the text above. "Deeper" really means "more strongly curved". "Shallower" really means "less strongly curved". The difference between circle and parabola is that the parabola is more strongly curved in the center, while the curvature at the edge is less strong. The circle has constant curvature everywhere, by definition.

This doesn't necessarily mean the center of the mirror is physically more depressed; while doing any strokes, the whole surface keeps being polished down all the time. But the relative curvatures of center vs. edge may change.

Deeper vs shallower are terms that reflect the physical process, whether the tool applies more or less pressure on a certain area of the mirror (so polishing goes faster or slower there). But the geometric attribute that the process actually changes, that we are interested in, is the radius of curvature. Where the tool applies more pressure, the radius of the curvature decreases rapidly (the surface becomes more strongly curved).

Deeper and shallower are practical terms related to process. More or less strongly curved are theoretical terms related to geometry. When you make mirrors, after a while these terms become linked in your mind.

---

It helps if you're familiar with the conic sections:

<https://en.wikipedia.org/wiki/Conic_section>

[![enter image description here](https://i.sstatic.net/dqfIN.png)](https://i.sstatic.net/dqfIN.png)

[![enter image description here](https://i.sstatic.net/tRMfS.png)](https://i.sstatic.net/tRMfS.png)

red = circle

orange = ellipse

green = parabola

blue = hyperbola

> **Comments:**
> **username_4**: `+1` I hope you don't mind the small edit to this excellent answer! fyi I've just asked the following mirror-making-relaged question: [Why is this telescope so short? How hard is it to make such a fast primary?](https://astronomy.stackexchange.com/q/33337/7982)  

---

