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shibumi 16” F3.5 Supremax 33 primary P201407i-01 1

16in Cellular Primary

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Structural simulation of a 16" cellular primary mirror for an astronomical instrument

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16 F3.5 Supremax 33 primary

16 F3.5 Supremax 33 primaryP201407i-011shibumiProblemsBorosilicate glass (Pyrex/Supremax) is getting expensive. The open market price of telescope mirror blanks in the profitable size range (16 up) is nearly USD1000.Need to reduce glass use or use something else. Epoxy/CFRP still too bleeding edge. Conical hub-mount is good but polishers dont like working with them. So cellular is the way to go for now.Requirements/customer expectations changing. The demand is for short F-ratio force-cooled precision optics for CCD photographic use, in a transportable package. Demand for cheap light buckets now being met from China with machine-polished BK7 and plate glass optics unprofitableNeed to focus on eliminating forced cooling (vibration, cost and simplicity) through better passive cooling dynamicsReliable precision optical figure requiredControlled mirror mounting (no interference by amateurs)Only sell blanks to most reputable polishersProfessionally tested interferometry or (preferably) Shack-Hartmann wavefront analysis.Mirror cell designs are crap. Very few meet the reasonable tip/tilt requirements of short F/R optics. Almost none eliminate all mirror movement with different instrument pointing position. None offer electric collimation. None offer primary mirror focusing to reduce equipment clutter around the focal plane/focuser.Integrate the primary and the mirror cell and use RTV bonded mirrorsProvide edge & face protection (front baffle) which also masks turned-edgeEngineer tip/tilt/focus mount with wireless control appSell as a premium package

2shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 4429609Structural design

3Support surfaces for optician are in red16 F3.5 borosilicate optic optimised for minimal print-thru and very low gravitational shape change.Located by central pin and RTV ring bond.Designed for fast thermal equilibration and minimum mass and cost.shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 44296090.25Psi Polishing pressure; back supported on flat areas only

4It appears that the thin faceplate will lead to minimal print thru effects provided that polishing pressure is well-controlled.shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 44296090.25 Psi Polishing pressure: support side of optic

5shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 442960945 deg Altitude pointing6

shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 442960945 deg Altitude pointing (rear)

7shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 4429609Zenith Altitude pointing

8shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 4429609Mounting surfaces for Optic

9shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 4429609

10shibumi | www. shibumi-consulting.net | [email protected] | ++353 (0)1 - 4429609