Monthly Archive for October, 2008

12 1/2″ Dobsonian Project

October 15th 2008

This project has been ongoing for some time. I actually started on this one first but decided against grinding it before I had experience with a smaller size.

It started as a full thickness Pyrex blank from Vancouver Telescope, which I got for $100 because someone had started it, and made a mess of it. It had an uneven grind to it, resulting in an off-center depression in it that required some 5 hours to center up. Once that was done, it only took another 5 hours of grinding with 46/70 and 80 grit to get the f ratio to around f/5, giving it a 60 inch focal length, a good compromise in shortness of tube and magnification, a wider field but still doesn’t have large amounts of coma.

There were pits left from the 46/70, so I gave it 5 more “wets” of 80 grit to level it a bit more.

The tile tool was easy to make but I learned the hard way to take my time a bit. I poured the base out of plaster in 4 separate pours to give me a 1 3/4 ” tool. I used epoxy to fix the titles but there was one problem with them as they tended to ‘float’ a bit and slide down the slope of the tool. I solved this by using a fingertip to bed them in when placed. None moved after that. I heard later on that some have problems with the pieces falling off, but those in ’pools’ of epoxy did not tend to do this.  Given the size involved, I didn’t bother to go completely to the edge with tiles by cutting tiles, just used the broken ones. This way, the tool acts a bit like a sub-diameter tool. After 220 grit, I cleaned it up with care, using epoxy to fill in holes or fix suspicious areas.

I used a bit of extra weight on it in the form of one of my mounts counterweights, one that was around 15 pounds. Later on, I used just the weight of the tool and my hands on the back of it. I theorize that a turned edge is caused by excessive overhang on a tool that has too much weight for its thickness, which lets the tool flex slightly on the overhang, resulting in the start of a turned edge. I also took my time in doing the 1/3 strokes with the tool. I did make a mistake in this stage though. I was letting the blank rest on the bare formica of my plywood backed surface thinking there would be no trouble with astigmatism. The blank has a 1/4″ raised rim on its bottom, which supports ALL the weight of the glass blank while I work on it. I checked contact when I changed grits at 220 and found I had good contact, so I used some old rubber sheeting and cut three circles of it to rest the mirror on when working “tool on top” or TOT.

I used a straight-edge and some feeler gauges to measure the depression, but I now own a spherometer good to 5 decimal places. I found I overshot my f/5 to f/4.8, so I did 120, 220 and now 320 grit with the tool on top. This is actually easier but I am not learning what I wanted from this. By changing TOT and MOT, you get control of the depth of your curve, very important if you plan on making refractive optics.

After 220 grit, I poured plaster and dental stone for the backing of the pitch lap. The finer grits after this will not change the curve all that much, so the plaster cast will be close enough for the pitch to conform properly. I found the dental product, while being slightly more expensive, is much more fluid when mixed. I plan on using it for all my later projects.

I have also made plans for the construction of the mechanics  of the scope. I really like some of the light-weight upper cages connected to the mirror enclosure with trusses. I plan that route. I found some of the upper cage assemblies a bit flimsy though. Too much empty space with the eyepiece looking at open air behind the secondary. Lots of people put up thin plastic shields to combat this issue. My plan is to use my router and a 1/4″ straight bit on 5/8″ baltic plywood. I will make two rings with a shallow cut in the middle. I will then bridge the two parts with an epoxied piece of formica (cuts well with a good blade on a table saw), and use truss poles to link upper and lower sections. I will build a small version of this for my polished 6″ f4.7 to see how well it works before commiting to a big version.

For grinding with 320 grit, I started with Al2O3 instead. I found this was a bit slow, so I returned to silicon carbide after just 4 wets. I did 15 more this way, then finished up with 5 wets of aluminum oxide. I got this in a box of grits, from Aurora Astro who got it from Bill Cook, of the ATM book fame. He had had enough and cleared out his stuff. I did this as an experiment mostly. The Al2O3 grinds more slowly in a more controlled fashion, important for getting to and keeping a curve at the correct amount. For a tough glass like Pyrex, it is rather slow at 320 grit. It also seems to break down a bit slower, confirming what more experienced workers say about it. It has grains which have a flat red blood cell shape, not a sharp, angular form.

I now have to clean up my work area to prepare for the fine grinding stages. I don’t want to return to 220 grit because of a mistake. I set the tool aside on a shelf where it can keep until I’m certain I won’t need it again.

The plaster for the polishing tool is dry but needs some clean-up to make it nice and smooth. I nearly used SANDPAPER on it but used files instead.

I used the 25 micron on the mirror and did some 25 wets. Some people like to use more but I plan to go through 15, 9 and 5 micron as well for a smooth surface. I had to take a break and repair old holes in the tool with epoxy resin to trap any old grit in them permanently.

January 11th 2010

I have gone through 15u, 9u and 5u; 30 wets each with one minor mishap. The tool stuck fast to the mirror at around the 4 1/2 minute mark of a 9u wet,  needing force to separate them. I had been playing with the ratio of grit to water and I believed it was due to the grit being worn too far, so I shortened the wets to 4 minutes from 5. No further problems arose. The mirror now has that buttery smooth surface to my fingers and the hint of mist it holds disappears when I breath on it, the signs of good fine grinding. No pits seem to remain.

I built a 8″ and 12 1/2″ pitch laps. That went well, in spite of forgetting to use parting compound (an alcohol spray mix) on the mold. It came off but took a few tiles near the edge with it. There was one damaged in the interior area and I might have to replace it to avoid a zone being created.

I ran out of my old hard pitch, so will need to open a container to make other laps. I did add a few tablespoons of turpentine to each batch to soften it up a bit.

It did a variation of warm pressing by using a bowl of hot water that was steeply curved, allowing the lap to be suspended over the water, making it a bit more controlled with how heat is applied.

I did try to do some polishing and it seemed to work but with catching and uneven friction,  the classic problem with incomplete contact between mirror and polishing lap. It will need more pressing to even it out. The main problem now is while humidity is high enough to slow evaporation of the rough/water mix, the temperature is too low to get effective polishing action. I will have to wait for better weather to allow the shop to be warmer. It is also quite hard to move. With 4 times the contact area of a 6″, the amount of work is that much larger. I seriously doubt I could do a mirror much larger by myself, and I was optimistic enough to buy 2 more 16″ blanks. I took some photos that show the wide polished area on the outer portion, with a central blank area that doesn’t show a reflection at all.  This is the classic result of only polishing with the pitch lap in the upper position. Most books recommend you swap them to go evenly. I did it this way because as you polish pitch lap on top, the polish moves from the outside to the center of the mirror. If you check the center for remaining pits, if the center checks out fine, then you KNOW the rest has a complete polish.

May 23,2010

The intervening weeks have been a mash-up of work, weekends away, the flu, cool conditions and now a shoulder/neck injury causing a pinched nerve. With the shoulder usable again, I restarted my efforts. I had wanted to finish in time for Table Mountain in August, but that seems unlikely now. I did the usual warming of mirror and lap, 30-45 minutes, followed by at least 30 minutes for warm pressing. I used a red plastic mesh bag for onions between them to add micro-facets to the lap. I had wanted to do this before but didn’t have a piece of mesh that could cover completely. This does two things: it forms the pitch to the mirror AND brings them both to similar thermal conditions. This will give the best polishing action and a better spherical surface. I am trying to maintain a better form for the polish stroke also: 2 inches or so back and forth, some variation in length and placement of tool, smaller number of strokes say 6 to 18 per position before moving and letting the rouge thin out and adding some water to lengthen each wet.

The lap is very hard to push around and changes to the rouge mixture does little to alter this. In most cases I only managed 1 1/2 hours of actual polishing time. It is true that the longer you go, the better the two pieces accommodate each and the better the figure you have. So far, there have been a total of 9 sessions with perhaps 12 hours of polishing.  I have changed my cleanliness as well. My shop has woodworking tools in it and bits of grit on the floor. I have avoided cleaning it out, as    this would raise dust contamination making the possibility of scratches while polishing. In between work sessions, I put each piece into a plastic bag folded over and weighed down to prevent breezes or drafts from getting dust inside. I am considering using mirror on top to finish but that means pushing around a 24 lb mirror, not the 12 lb tool.. Also rouge would not go as far, and since the mirror has to be lifted more  often, it increases the likelyhood of dropping it.

Since the mirror now holds some polish across the entire surface, I have started testing it. The Folcault tester from RASC still works, using an old 12V lamp for light. It is a virtual copy on the one in Texeraeu’s book, right down to the brass pieces used to make the slit light source. I removed that to give more light to help me align the apparatus. I puzzled over how to do this and realized that I could use a sheet of paper to find where the reflection was ending up. I had to use a mirror support meant for an 8 inch mirror. I realized I could just tip the 12 1/2″ forward, rather than raise the tester up some 2 inches. There are some tricks to know: the distance between source and return is the geometric center.  The image should be in focus when it gets back tot he tester, and pass between the light source and 1/4″ from where your knife edge is. You also need to have the TRAVEL portion of the knife edge at 90 degrees to the returning beam or the shadows that you see will be meaningless. Once I did that, I replaced the slit mask. With a few adjustments, I could now see a squarish oval with a series of interferance bands running vertically, more or less what should be visible. I need make a knife edge, as this is missing. I though I could use a piece of stainless steel for it and tired to cut it on my tablesaw. It went flying off like the piece of shrapnel it had become.

August 20th.

I have used  an 8″ lap for parabolizing/smoothing this large mirror and have found it anating so I rebuilt it using softer (added 4 Tbs turpentine) pitch for better conformity. I have used this for 4 spells of polishing totaling some 5 hours. With my semi-working left shoulder 80 minutes is the maximum I can go without serious pain or compromised polishing.

Tests have looked better now, with only a slightl trace of roughness present and it seems to be of the shape called an “ellisepoid”, half way from a sphere to the classic paraboloid. I am still thinking about my support structure. A classic Dobsonian would be easy but also a Porter Equatorial is workable with not that much extra labour. DSC04015 (Large)

ATM 6″ Mirror/Binoscope

Currently, I have a polished but not parabolized 6″ f/5 plate mirror made. I may get to test it later this year but I need to work out the bugs of the Foucault tester.

Grinding it went well as can be expected without any major problems, with no pits showing up after polishing. I used a tile tool, rather than the more standard glass tool as I wanted to use this small piece of glass for practice.

In other news, I will go ahead with the roughing in of the two pieces for a binoscope. I plan on using two tools, working each one for a set amount of time, switching, then continuing on. This should give me a pair of blanks with the same ROC, provided I switch them often enough. The blanks are both pyrex this time from Willman Bell and being tougher than plate, the ROC will only move with a lot of effort.

I was going through old S & T magazines (a great resource BTW, a much better magazine then than it is now) and found an article [Dec 1979] by Sinnott on a 6″ binoscope. I had seen it before and was going to file it but its unusual optics caught my eye.

It featured an unobstructed light-path that allows the pencil of light to exit the tube through the side into prisms that rotate and invert the image. With 3 additional reflections (all internal, less light loss) you end up with a normal view like a true binocular.

The only problem is that while you grind them like a 6″ f/6, you need to parabolize them like a 12″ f/3. This means each mirror has to be deepened in an offset manner. How far offset depends on how much you want the light pencil from center. This also means a very difficult Foucault Test.

NOVA Newsletter: Mount Kobau 2008 Star Party Report, etc.

NOVA is the RASC Vancouver Centre bimonthly newsletter.

From the  current edition:

Mt. Kobau Star Party Report 2008

“…. Tuesday night was a wonderful night with the Milky Way bright and visible from horizon to horizon. Pomponia’s 12-inch dob and Ron Jerome’s 16-inch were having a great time finding faint fuzzies with M82 being especially entertaining. ….”

Previous editions are available in the archives.

The Antony Overton Memorial Observatory

Observing at this site is mainly for members interested in learning about amateur research astronomy. At the present time small public groups are welcome to tour our facility by making arrangements with the AOMO Chairperson ( lyonsww@shaw.ca).

Any RASC-Vancouver Centre members wishing to be actively involved in using the equipment are welcome.  Telescope operators are expected to participate in the following:

· Complete 15 hours training in the operation of the observatory. This will include completing an operational checklist at each session.

· Volunteer time with the maintenance and training at the observatory. Attend at least one work party a year at the observatory. (Work parties are to clean up the inside and outside areas of the site. We have permission to clear a 20 metre perimeter around the observatory)

· Volunteer with RASC-Vancouver Centre’s public outreach activities such as the operation of the Gordon MacMillan Southam Observatory, Astronomy Day, or any of the Sidewalk Astronomy Sessions planned by the Centre.

· Qualified members will be expected to be available to help train other RASC-Vancouver Centre members in the operation of the observatory.

Qualified members will be able to submit observing projects and make use of the observatory on a scheduled basis.

Please contact:

Wayne Lyons,

Chairperson, AOMO

e-mail: lyonsww@shaw.ca

tel: (604) 467-2956

Current clear Sky forecast for observers

Click here for information on how to use it.

October 9th: Observations of a Telescope Designer – Building the Thirty meter telescope

This is the Royal Astronomical Society of Canada – Vancouver monthly meeting.

Craig Breckenridge and members of the world’s premier Observatory design team at Empire Dynamic Structures took a trip to see the facility currently hailed as the largest optical telescope in the world. This marvel of engineering is soon to be eclipsed by the construction of the Thirty Meter Telescope which is currently being designed by this local company located in Port Coquitlam. Facets of the LBT’s design seldom seen by outsiders will be presented in all their glory with commentary by our resident expert designer.

We meet at 7:30 p.m. on the second Thursday of each month, downstairs in the auditorium of the H.R. MacMillan Space Centre.

Free Admission, Open to the public

Astro-coffee and astro-cookies will be served at the Southam Observatory after the meeting.