Tony Gondola avatar

I’m wondering about the best ways to clean up the diffraction effects that Newtonians produce. I know that the diffraction from the clips and a rough mirror edge can me mitigated with a mask but I ‘d wondering if there are other common sources. Here’s an example from my system:

📷 Untitled hair.jpgUntitled hair.jpgI can see the clips as dark lanes but I’m wondering about the extra spike at 10:30 and doubling of the vane spike on the left side. It first I thought it was simply a misalignment but I’m puzzled as to why it’s origin is way over on the right side rather than the center.

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Brian Puhl avatar

I believe this is due to one of your spider vanes being slightly bent.

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andrea tasselli avatar
You can always apodize your aperture but apart for aesthetics there is nothing to gain and aperture to loose.
Tony Gondola avatar

andrea tasselli · Sep 7, 2025, 05:53 PM

You can always apodize your aperture but apart for aesthetics there is nothing to gain and aperture to loose.

I know and that’s my dilemma. In terms of figure the mirror’s edge is great so there’s no need to mask it from that point of view.

Tony Gondola avatar

Brian Puhl · Sep 7, 2025, 05:48 PM

I believe this is due to one of your spider vanes being slightly bent.

I’m going to have to carefully measure that. If opposite vanes are not exactly 180 degrees to each other I can see getting doubled vanes, but I would have though it would be the same pattern on both sides.

andrea tasselli avatar
Not if only ONE vane is off, then its periodicity is 360 deg.
Rick Krejci avatar

That looks like clips/mirror edge effects to me. They look like they’re 120 degrees apart. Do you have a mask around the mirror’s edge?

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Tony Gondola avatar

Rick Krejci · Sep 7, 2025, 09:50 PM

That looks like clips/mirror edge effects to me. They look like they’re 120 degrees apart. Do you have a mask around the mirror’s edge?

No, that’s one of the things I’m thinking about doing. I think the clips and mirror edge are what are causing the pattern you’re seeing.

John Hayes avatar

Bond the mirror to the cell and get rid of the clips. Just be sure to bond it properly so that you don’t distort the optical figure. Before you do that, test the system with an aperture mask to insure that you know what is causing what in the PSF.

That double vane could be caused by a few things. Is there a focuser tube that extends down into the light path on one side? Are there any heater wires running along a spider vane? There is something with a straight edge at right angles to that pattern that is cutting into some part of the marginal ray path somewhere in the light path. You just have to figure out what it is.

John

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Tony Gondola avatar

John Hayes · Sep 8, 2025, 12:40 AM

Bond the mirror to the cell and get rid of the clips. Just be sure to bond it properly so that you don’t distort the optical figure. Before you do that, test the system with an aperture mask to insure that you know what is causing what in the PSF.

That double vane could be caused by a few things. Is there a focuser tube that extends down into the light path on one side? Are there any heater wires running along a spider vane? There is something with a straight edge at right angles to that pattern that is cutting into some part of the marginal ray path somewhere in the light path. You just have to figure out what it is.

John

No wires and no focuser intrusion so I think I just have to look closely at the vanes.

What would be your suggested method for bonding the primary? My first thought was remove the pads and clips, then apply 3 small blobs of silicone adhesive at the 70 percent zone. Along with that I would think it would make sense to remove the side pads and drill and tap for three nylon screws for centering.

📷 post-337676-0-68492700-1609709222.jpgpost-337676-0-68492700-1609709222.jpg

Jochen Schambach avatar

My TS Photon (GSO) Newton had the same problem.

I ordered a spider and mask from BU. That solved the problem, and as a side effect, the collimation of the secondary mirror holds better. Fits perfectly.
During the modification, I also sprayed the inside of the tube and the back side of the secondary mirror with black paint (Noctutec SL94) to reduce reflections.

There are also spiders with 3 vanes, which then produce 6 spikes, like on the James Webb Telescope.

TS/GSO - Backyard Universe

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John Hayes avatar

Tony Gondola · Sep 8, 2025 at 03:23 AM

John Hayes · Sep 8, 2025, 12:40 AM

Bond the mirror to the cell and get rid of the clips. Just be sure to bond it properly so that you don’t distort the optical figure. Before you do that, test the system with an aperture mask to insure that you know what is causing what in the PSF.

That double vane could be caused by a few things. Is there a focuser tube that extends down into the light path on one side? Are there any heater wires running along a spider vane? There is something with a straight edge at right angles to that pattern that is cutting into some part of the marginal ray path somewhere in the light path. You just have to figure out what it is.

John

No wires and no focuser intrusion so I think I just have to look closely at the vanes.

What would be your suggested method for bonding the primary? My first thought was remove the pads and clips, then apply 3 small blobs of silicone adhesive at the 70 percent zone. Along with that I would think it would make sense to remove the side pads and drill and tap for three nylon screws for centering.

📷 post-337676-0-68492700-1609709222.jpgpost-337676-0-68492700-1609709222.jpg

I like your concept. 70% zone with three “glue-points” sounds very reasonable. The best thing to do is to first experiment to make sure that you are using the right kind of adhesive. You don’t want it to fail and have the mirror fall out, you don’t want it to distort the mirror, and it should be safe over a wide temperature range. I don’t have a recommendation off the top of my head but there are a lot of optical adhesives on the market so a little research will go a long way. We used to use a small hard point (like a recessed ball bearing) to mechanically define the position of the mirror and put the “blob” of glue over the hard point. Then push the component against the hard point and let the glue cure. That way the mirror is held by the glue but the position is well defined by the hard points. That avoids having the mirror “float” on the adhesive.

John

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Tony Gondola avatar

That sounds like a great approach. I don’t imagine that it takes much flex in the adhesive to allow the mirror to maintain figure. It might also be worthwhile to make the bond at a temperature that’s in the middle of the expected range for the component. In my case, about 10C.

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John Hayes avatar

I don’t think that the temperature during bonding is super critical. The important things are:

1) Strength of the surface adhesion with glass and the mount material (aluminum?)

2) Temperature stability. It shouldn’t fail when it gets hot or cold and it shouldn’t put a lot of stress on the mirror when the temperature changes. Low CTE is a good thing but that may be hard to find.

3) Some level of elasticity is good. There are a lot of adhesives that cure to be rock-hard but that’s not desirable. My recommendation would be to look at two-part RTV adhesives. Also pay close attention to any recommendations for surface prep. A few adhesives require a primer for best strength.

4) Try to keep the diameter of the glue “circle” as small as possible—maybe 0.5” - .8”. You just want it large enough to safety support the weight of the mirror but not much more. The larger the diameter of the bonding area, the higher the chance of distorting the mirror figure.

Before bonding your mirror, I recommend getting a scrap piece of glass to practice the procedure. You can also use that sample to do some pull testing to gauge the strength of the bond. That will provide a lot of peace of mind after you mount your mirror.

Come to think of it, you could also do this with double sided tape. That’s how Celestron mounts all of their secondary mirrors. Give me a little time and I’ll search my PC. I think that I might have some records on the kind of tape they use. It is totally permanent and if you mount it correctly, it shouldn’t deform the mirror at all.

John

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andrea tasselli avatar
As alternative I'd use a central bar/bolt glued at the center of the back of the mirror with one of those ceramic-metal epoxies and locked to the back of the cell with a 3 arm spider. Just make everything with the same material of the cell and you'll have no issue with differential thermal expansion. Remove the clips and you are done.
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Tony Gondola avatar

John Hayes · Sep 8, 2025, 05:01 PM

I don’t think that the temperature during bonding is super critical. The important things are:

1) Strength of the surface adhesion with glass and the mount material (aluminum?)

2) Temperature stability. It shouldn’t fail when it gets hot or cold and it shouldn’t put a lot of stress on the mirror when the temperature changes. Low CTE is a good thing but that may be hard to find.

3) Some level of elasticity is good. There are a lot of adhesives that cure to be rock-hard but that’s not desirable. My recommendation would be to look at two-part RTV adhesives. Also pay close attention to any recommendations for surface prep. A few adhesives require a primer for best strength.

4) Try to keep the diameter of the glue “circle” as small as possible—maybe 0.5” - .8”. You just want it large enough to safety support the weight of the mirror but not much more. The larger the diameter of the bonding area, the higher the chance of distorting the mirror figure.

Before bonding your mirror, I recommend getting a scrap piece of glass to practice the procedure. You can also use that sample to do some pull testing to gauge the strength of the bond. That will provide a lot of peace of mind after you mount your mirror.

Come to think of it, you could also do this with double sided tape. That’s how Celestron mounts all of their secondary mirrors. Give me a little time and I’ll search my PC. I think that I might have some records on the kind of tape they use. It is totally permanent and if you mount it correctly, it shouldn’t deform the mirror at all.

John

That would be great, certainly the simplest approach. Would you have the same size constraints when using tape verses RTV?

Tony Gondola avatar

andrea tasselli · Sep 8, 2025, 05:28 PM

As alternative I'd use a central bar/bolt glued at the center of the back of the mirror with one of those ceramic-metal epoxies and locked to the back of the cell with a 3 arm spider. Just make everything with the same material of the cell and you'll have no issue with differential thermal expansion. Remove the clips and you are done.

That’s an interesting solution. I can see that also as the basis for focusing using the primary. Something I’ve always been interested in.

Tareq Abdulla avatar

Once you fix the issue then please post back and show us, i have similar problem once with my 8” Newt, i didn’t use my 6” yet but i believe it will have same issue as well, i had an issue of collimating my 6” and not with 8”, but i think i will modify both then will use them again and see, waiting to see your solution.

Tony Gondola avatar

Will do, the remount as John suggested will be fairly quick to do over the next stretch of cloudy weather.

Tareq Abdulla avatar

Good to hear, can’t wait

andrea tasselli avatar
Jochen Schambach:
My TS Photon (GSO) Newton had the same problem.

I ordered a spider and mask from BU. That solved the problem, and as a side effect, the collimation of the secondary mirror holds better. Fits perfectly.
During the modification, I also sprayed the inside of the tube and the back side of the secondary mirror with black paint (Noctutec SL94) to reduce reflections.

There are also spiders with 3 vanes, which then produce 6 spikes, like on the James Webb Telescope.

TS/GSO - Backyard Universe

That is a 8.9% reduction in area. There must be a better way...
John Hayes avatar

Tony Gondola · Sep 8, 2025, 05:42 PM

John Hayes · Sep 8, 2025, 05:01 PM

I don’t think that the temperature during bonding is super critical. The important things are:

1) Strength of the surface adhesion with glass and the mount material (aluminum?)

2) Temperature stability. It shouldn’t fail when it gets hot or cold and it shouldn’t put a lot of stress on the mirror when the temperature changes. Low CTE is a good thing but that may be hard to find.

3) Some level of elasticity is good. There are a lot of adhesives that cure to be rock-hard but that’s not desirable. My recommendation would be to look at two-part RTV adhesives. Also pay close attention to any recommendations for surface prep. A few adhesives require a primer for best strength.

4) Try to keep the diameter of the glue “circle” as small as possible—maybe 0.5” - .8”. You just want it large enough to safety support the weight of the mirror but not much more. The larger the diameter of the bonding area, the higher the chance of distorting the mirror figure.

Before bonding your mirror, I recommend getting a scrap piece of glass to practice the procedure. You can also use that sample to do some pull testing to gauge the strength of the bond. That will provide a lot of peace of mind after you mount your mirror.

Come to think of it, you could also do this with double sided tape. That’s how Celestron mounts all of their secondary mirrors. Give me a little time and I’ll search my PC. I think that I might have some records on the kind of tape they use. It is totally permanent and if you mount it correctly, it shouldn’t deform the mirror at all.

John

That would be great, certainly the simplest approach. Would you have the same size constraints when using tape verses RTV?

I made a trip out to my workshop where I’m sure that I have a spare sample of the tape; but as hard as I tried, I couldn’t find it. It will probably turn up as soon as I stop looking for it! I’m pretty sure that it’s a 3M VHB tape. It was black and about 2-3 mm thick. 3M makes a wide variety of VHB tapes for different applications and temperature ranges. You’ll have to look through the 3M specs to see which type would meet your requirements. I’d recommend using three round pieces of tape—probably ~0.7” in diameter. Again, I’d pull test it before mounting the mirror. The stuff that I used on the Celectron secondaries was super strong. It was virtually permanent. You could remove it with a lot of heat and some hard work but there was no concern about it letting go.

John

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Jochen Schambach avatar

andrea tasselli · Sep 8, 2025, 09:01 PM

Jochen Schambach:
My TS Photon (GSO) Newton had the same problem.

I ordered a spider and mask from BU. That solved the problem, and as a side effect, the collimation of the secondary mirror holds better. Fits perfectly.
During the modification, I also sprayed the inside of the tube and the back side of the secondary mirror with black paint (Noctutec SL94) to reduce reflections.

There are also spiders with 3 vanes, which then produce 6 spikes, like on the James Webb Telescope.

TS/GSO - Backyard Universe


That is a 8.9% reduction in area. There must be a better way...

This has already been discussed in German forums. Most attempts using different kinds of glue or tape ended up introducing astigmatism, especially when the scope was pointed close to the horizon.

The mirror clips are really just there to keep the mirror from falling out; ideally, they shouldn’t put any pressure on it. Maybe someone (not me) could 3D print a retaining ring that does the same job but covers less of the mirror than a traditional retaining ring. Basically a slim ring that also takes over the function of the clips. Whether that would actually work though – I have no idea.

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John Hayes avatar

Jochen Schambach · Sep 9, 2025 at 07:21 AM

This has already been discussed in German forums. Most attempts using different kinds of glue or tape ended up introducing astigmatism, especially when the scope was pointed close to the horizon.

That’s probably because the mounting wasn’t done properly. We used to mount reference flats in the range of diameters from 4” up through 12” for interferometers using potting compound and that was a super critical application. Any surface distortion greater than 1/40 wave (~ 12 nm) over a fairly wide temperature range would exceed the specified optical accuracy for the component. Adhesives are used all the time to mount ultra-precision optical parts but to work well, it has to be done properly. As I’ve said, Celestron uses tape to mount SCT secondary mirrors and the primary mirrors are all bonded using potting compound. I’ve spent a bit of time working with the folks at Carl Zeiss in Oberkochen and they were very well versed in this stuff so I’m not sure who is participating on the German forums but I would have to wonder about their level of expertise.

John

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Tony Gondola avatar

John Hayes · Sep 8, 2025, 11:34 PM

Tony Gondola · Sep 8, 2025, 05:42 PM

John Hayes · Sep 8, 2025, 05:01 PM

I don’t think that the temperature during bonding is super critical. The important things are:

1) Strength of the surface adhesion with glass and the mount material (aluminum?)

2) Temperature stability. It shouldn’t fail when it gets hot or cold and it shouldn’t put a lot of stress on the mirror when the temperature changes. Low CTE is a good thing but that may be hard to find.

3) Some level of elasticity is good. There are a lot of adhesives that cure to be rock-hard but that’s not desirable. My recommendation would be to look at two-part RTV adhesives. Also pay close attention to any recommendations for surface prep. A few adhesives require a primer for best strength.

4) Try to keep the diameter of the glue “circle” as small as possible—maybe 0.5” - .8”. You just want it large enough to safety support the weight of the mirror but not much more. The larger the diameter of the bonding area, the higher the chance of distorting the mirror figure.

Before bonding your mirror, I recommend getting a scrap piece of glass to practice the procedure. You can also use that sample to do some pull testing to gauge the strength of the bond. That will provide a lot of peace of mind after you mount your mirror.

Come to think of it, you could also do this with double sided tape. That’s how Celestron mounts all of their secondary mirrors. Give me a little time and I’ll search my PC. I think that I might have some records on the kind of tape they use. It is totally permanent and if you mount it correctly, it shouldn’t deform the mirror at all.

John

That would be great, certainly the simplest approach. Would you have the same size constraints when using tape verses RTV?

I made a trip out to my workshop where I’m sure that I have a spare sample of the tape; but as hard as I tried, I couldn’t find it. It will probably turn up as soon as I stop looking for it! I’m pretty sure that it’s a 3M VHB tape. It was black and about 2-3 mm thick. 3M makes a wide variety of VHB tapes for different applications and temperature ranges. You’ll have to look through the 3M specs to see which type would meet your requirements. I’d recommend using three round pieces of tape—probably ~0.7” in diameter. Again, I’d pull test it before mounting the mirror. The stuff that I used on the Celectron secondaries was super strong. It was virtually permanent. You could remove it with a lot of heat and some hard work but there was no concern about it letting go.

John

Ok John, I appreciate the effort! I’ll investigate the VHB line to see what’s best. It sounds like it would be handy to have around anyway.

I’m looking at it now and realized I’ve used this stuff before. I used it to secure a wooden frame to a tiled banco to bring it to a more comfortable height. Surprisingly, it’s still solid after many years of use.

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