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AO opto -mechanical design architectures Cost Impact. Don Gavel NGAO Team Meeting #5 February 5, 2009. Impact of Build to Cost on the Opto-mechanical design. One tier (140 mm beam) vs two-tier (100 mm beam) designs
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AO opto-mechanical design architecturesCost Impact Don Gavel NGAO Team Meeting #5 February 5, 2009
Impact of Build to Cost on the Opto-mechanical design • One tier (140 mm beam) vs two-tier (100 mm beam) designs • Woofer DM cost – impacted by the likely inability to reuse the current system’s DM • Cilas: • increasing DM from 100mm to 140mm could increase cost 15% • increasing diamter 100mm to 140mm decreases TT bandwidth by 30% • cost of TT stage 50-100% of DM cost. • Xinetics • Not much difference between 100mm and 140mm DM regarding cost, probably also not resonant frequency. • No ROM cost response yet
One-tier vs Two-tier • Support structure for the K-mirror derotator - $90K engineering cost makes it a wash with eliminating the second tier. • Switchyard choice impact (essentially none – both switchyard options doable for both first relay design options
Tip/Tilt Stages • DM on Tip/tilt stage • Tip/tilt stage cost (baseline is to put woofer on a t/t stage, possibly a “woofer” tt stage) • Cilas: cost of TT stage 50-100% of DM cost - I believe this is what we costed at SDR: $200K on woofer, $20K on tweeter. • Xinetics: Have done 2 designs of TT with heavy mirror insert – 100Hz bandwidth at 0.5 mrad mechanical displacement, or 0.62mrad of TT to 1.4kHz • PI: to get back to us • Lick shops: gimbaled TT stages for both woofer and tweeter look reasonably doable at low cost • Bottom line: there is room for reducing the $220K cost significantly, perhaps by as much as $100K, but at some risk
Switchyard • Dichroic set (6 keyhole designs) and changer mechanism vs single focal plane and common pickoff design • Dichroics • Custom Scientific • T>80% in the transmission region and R>90% in the reflection region • Tavg>90% and Ravg>98% but that would require more layers in the coating and that could significantly degrade the lambda/10 surface • Cost $10,000-$25,000 per piece • Barr Associates • J trans/HK reflect will be difficult to make • Cost ROM pending • Cost of changer mechanisms (NGAO_SD_Cost_Estimate_Don_Gavel_Penult6.xls 4.2.4FSD) $30K • Cost of dichroics $10K per, 6 post relay 1 dichroics (KAON 550) = $60K
Switchyard • Pickoffs • Cost of pickoff mechanisms – note: cost of mechanisms is same as in split to IFS/LOWFS design, so zero delta cost • Single focal plane pickoff approach requires care in packing LOWFS and IFS packages to allow narrow field second relay room to be mounted. Preliminary layout design shows this is doable. There is still plenty of room for post second relay switchouts (to NGSWFS, IR Imager/Spectrograph, VisImager) • Science impact: • Pickoffs may need to enter 30 arcsec narrow field if a tt star is there No provision to use the science object itself as the tt star in LGS mode observing. This effects only some science scenarios (asteroids, companions to low mass stars, AGNs, between v=12-20) • Should be able to use 3 TT stars in the 30-120 arcsec annulus and still get good sky coverage • And we have a proposed work-around to this problem
Refrigerator-free low surface count single relay option? • Memo of Jan 28 shows high leverage of cooling leads to no improvement or even worse emissivity for this option • Gain in LGS throughput with no windows and no K-mirror (or K-mirror after LGS splitter). But new data concerning window AR coatings mitigates LGS throughput (see Drew Phillip’s chart). (1/2% per surface vs 1% loss per surface assumed earler). K-mirror has 3-reflections loose 1% each, so total double pane window plus K-mirror loss is 5% instead of pessimistic 7% in memo. +$273K cost of laser light compared to +$383K.
Cost Impact of not refrigerating the LGS WFS assembly • Requires another double-pane window that LGS light must pass through. (2% loss on 75 W = 1.5 W at $73K/W = $109K)
Cost Impact of Reduced RTC • 4-plus-3, with 4 on 1 arcmin field, vs 9 on 2 arcmin field • Reduces size of tomography engine (which scales with field) • Reduces number of processors needed for wfs (7 vs 9) but this may be negligible because these processors are reused in the tomography engine step of the algorithm, and the tomography engine processor need is larger • Lower cost of the telemetry disk array (fewer raw camera outputs) • We are still investigating this. Possible cost gains: • Less tomography hardware (but capped by $450K total cost of all computer and interface boards) • Fewer WFS cameras, and camera interface boards ($2632K savings on cameras, $5K on interface boards) • Less complexity and hence lower I&T costs • We do not anticipate any decrease in programming costs, perhaps even a modest increase due to need to add point-and-shoot algorithm support.