CRaTER CDR Mechanical Design Mechanical Design, CRaTER Assembly and Electronics Assembly Critical Design Review Matthew Smith (617)-252-1736 matt@space.mit.edu Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 1 CRaTER CDR Mechanical Design Overview Assembly Description Mechanical Environments and Requirements Mechanical Design Details Near Term Tasks Back-up slides Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 2 CRaTER CDR Mechanical Design Assembly Description • Crater integrates two main sub-assemblies: The Telescope Assembly and The Electronics Assembly. – – – – The Telescope Assembly is being designed and built by The Aerospace Corporation The Analog Board is being designed by Aerospace. The Flight Analog Boards will be built by MIT The Digital Board and Electronics Enclosure Assembly are being designed and built by MIT. MIT will integrate the two sub-assemblies and perform all functional, environmental and acceptance testing. L13.5”x W9” x H 6” Weight 6.4Kgs max. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 3 CRaTER CDR Mechanical Design Assembly Description Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 4 CRaTER CDR Mechanical Design Overview Assembly Description Mechanical Environments and Requirements – Imposed – Internal Mechanical Design Details Near Term Tasks Back-up slides Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 5 Mechanical Environments - Imposed • CRaTER CDR Mechanical Design From 431-RQMT-000012, Rev A, Environments Section 3.1. Section Description Levels 3.1.1.2 Net cg limit load 28.9 g* 3.1.4.2 Sinusoidal Vibration Loads Protoflight; Frequency (Hz) 5 - 17.7 17.7 – 50 Level 1.27cm D.A. 8 g’s 3.1.5 Acoustics Delta IV Medium: Protoflight OASPL 140.0 dB Atlas V 401: Protoflight OASPL: 137.0 dB 3.1.6.1 Random Vibration See Random Vibration slide 3.1.7 Shock environment See Shock Environment slide 3.1.8 Venting Minimum of .25 in^2 of vent area per cubic foot volume * Interpolated from Table 3-1 for CRaTER at 6.4Kgs. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 6 CRaTER CDR Mechanical Design Mechanical Environments, Imposed Random Vibration Random Vibration Levels Random Vibration Spec Protoflight/ Qual Acceptance 20 0.026 50 0.16 800 0.16 2000 0.026 Overall 14.1 Grms Frequency (Hz) 1 10 100 1000 0.013 0.08 0.08 0.013 10.0 Grms 10000 Protoflight/ Qual 1 0.1 Acceptance Power Spectral Density (g^2/Hz) Freq (Hz) 0.01 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 7 CRaTER CDR Mechanical Design Mechanical Environments, Imposed Shock Environment Table 3-12 LRO/PAF Shock Response Spectrum Delta IV (1194 PAF) Frequency (Hz) 100 100-1,000 1,000-10,000 Level (Q=10) 150 g +9.2 dB/Octave 5,000 g Atlas (Type B1194 PAF) Frequency (Hz) 100 100-1,400 1,00-10,000 Level (Q=10) 100 g +7.6 dB/Octave 2,800 g Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 8 CRaTER CDR Mechanical Design Mechanical Environments, Imposed Shock Environment Table 3-13 Deployable Separation Mechanism Shock Response Spectrum Separation Nut (SN9423-2) Frequency (Hz) 100 100-3,000 3,000-10,000 Level (Q=10) 50 g +7.8 dB/Octave 4,000 g Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 9 CRaTER CDR Mechanical Design Mechanical Requirements and Verification • From 431-RQMT-000012, Rev A, Frequency Requirements Section 3.2. Section Description Levels 3.2.2.1 Fundamental frequency, Hz > 35 Hz Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 10 Mechanical Requirements and Verification • CRaTER CDR Mechanical Design From 431-RQMT-000012, Rev A, Verification Requirements Section 3.3. Section Description Levels/Comments 3.3.1 Factors of Safety See FOS table 3.3.2 Test factors See Test Factors table 3.3.3.2 Perform frequency verification test for Instruments with frequencies above 50 Hz.. Verify and report frequencies up to 200Hz Low level sine sweep 3.4 Finite Element Model requirements: Instruments with predicted first frequencies below 75 Hz shall provide Finite Element Models. CRaTERs first fundamental frequency is well above 75Hz. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 11 CRaTER CDR Mechanical Design Mechanical Requirements- Imposed Factors of Safety Table 3-1 from 431-SPEC-000012 Design Factor of Safety Type of Hardware Yield Ultimate Tested Flight Structure - Metallic 1.25 1.4 Tested Flgiht Structure - Beryllium 1.4 1.6 Tested Flight Structure - Composite N/A 1.5 Pressure Loaded Structure 1.25 1.5 Pressure Lines and Fittings 1.25 4.0 Untestest Flight Structure - Metallic Only 2.0 2.6 These are applied to the protoflight level testing Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 12 Mechanical Requirements - Imposed CRaTER CDR Mechanical Design Test Factors Table 3-16 Test Structural Loads Level Duration Centrifuge Sine Burst Protoflight Comments 1.25 x Limit Load 30 seconds 5 Cycles Full Level Acoustic Level Duration Will be tested at LRO Level Limit Level +3 dB 1 minute Random Vibration Level Duration Limit Level +3 dB 1 minute per axis Sine Vibration Level Sweep Rate 1.25 x Limit Level 4 Octave/Minute per Axis Shock Actual Device Simulated 2 Actuations 1.4 x Limit Level 1 Actuation/Axis Will be tested at LRO Level Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 13 CRaTER CDR Mechanical Design General Thermal Subsystem Requirements from 431-Spec-000091 Section Description 4.1 Exterior facing MLI blankets shall have 3 mil Kapton with VDA in outer Coating. 4.2 MLI Blanket Grounding: All blankets shall be grounded per 431-ICD-00018 4.3 MLI Blanket Documentation: The location and shape documented in as-built ICDs. 4.4 Attachment to MLI Blankets: All exterior MLI blankets shall be mechanically constrained at least at one point. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 14 CRaTER CDR Mechanical Design Overview Assembly Description Mechanical Environments and Requirements – Imposed – Internal Mechanical Design Details Near Term Tasks Back-up slides Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 15 CRaTER CDR Mechanical Design Internal Requirements for the Electronics Assembly • Derived Internal Mechanical Requirements for Electronics Assembly – – – Have adequate contact area (.5 in^2 min) to the spacecraft to support Thermal requirements. Provide safe structure, within Factors of Safety specified, to support Telescope Assembly. Provide for mounting 2 Circuit Card Assemblies. • – – – Provide means to route cable from telescope to the Analog side of the Electronics Assembly to minimize noise. Electrically isolate the Electronics Enclosure from the Telescope, yet provide sufficient thermal conductance path. Electrical connector interface to the Spacecraft to be on one side of the Electronics Enclosure. • – – The Analog Board and Digital Board must be separated by an aluminum plate. The interface connectors to be on the Digital side of the Electronics Enclosure (separate from the Analog side) Provide GN2 purge interface inlet that routes to the telescope assembly and an outlet port at the digital board side of the internal volume. Follow the octave rule for natural frequency of the PWAs to the Electronics Enclosure. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 16 CRaTER CDR Mechanical Design Overview Assembly Description Mechanical Environments and Requirements Mechanical Design Details Near Term Tasks Back-up slides Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 17 DESIGN DETAILS –Natural Frequencies • CRaTER CDR Mechanical Design Natural Frequency Estimates – From SOLID WORKS cosmos package, 2005 • CRaTER Assembly – – First frequency at 326 Hz (bottom cover) Dominant Frequency at 1516 Hz (main assembly) • Analog Board- 195 Hz • Digital Board- 161 Hz • Bare E-box – – First mode frequency is 1002 Hz at the side with connectors. Third mode Frequency is 1239 Hz at the middle plate that holds the two Circuit Card Assemblies. • Top Cover- 284 Hz • Bottom Cover - 351 Hz • Telescope Assembly – – First frequency- 1910 Hz Dominant Frequency- Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 18 CRaTER CDR Mechanical Design Random Vibration Loads • Load levels are dominated by random vibration spec. • For resonances in the Random Vibration Spec, Miles’ Equation shows 3 sigma loading on the order of 85-154 g • Assume Q=20 Description CRaTER Assembly Analog Board Digital Board E-Box Enclosure Top Cover Bottom Cover Part No. Frequency (Hz) ASD (g^2/Hz) Associated g load (g) 3 sigma load (g) 32-10000 1516 0.055 51.3 153.9 30-10201 195 0.160 31.3 93.9 32-10202 161 0.160 28.4 85.3 32-10203 1239 0.084 49.4 148.3 32-10204 284 0.084 27.3 81.9 32-10205 351 0.160 42.0 126.0 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 19 DESIGN DETAILS Stress Margins, Electronics Assembly Pieces • • • CRaTER CDR Mechanical Design Load levels are driven by random vibration spec Factors of Safety used for corresponding material from 431-SPEC-000012. – Metals: 1.25 Yield, 1.4 Ultimate – Composite: 1.5 Ultimate Margin of Safety = (Allowable Stress or Load)/(Applied Stress or Load x FS) – 1 Description Material Desc. MS Yield MS Ultimate CRaTER Assy Aluminum, 7075 and 6061 + 1.7 + 1.8 Top Cover Aluminum 7075 +12.8 +12.9 Bottom Cover Aluminum 7075 +1.5 +1.5 Digital Board Polyimide glass brittle +0.9 Analog Board Polyimide glass Brittle +0.1 E-box Structure Aluminum 7075 +17.7 +17.9 Note 1. From SOLID WORKS, COSMOS excluding top and bottom covers in the model. All components have positive Margin of Safety Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 20 CRaTER CDR Mechanical Design DESIGN DETAILS Stress Margins, Hardware • • • Load levels are driven by random vibration spec Factors of Safety used for corresponding material from 431-SPEC-000012. – Metals: 1.25 Yield, 1.4 Ultimate Margin of Safety = (Allowable Stress or Load)/(Applied Stress or Load x FS) – 1 Description Location/ # of bolts Material Desc. MS Yield MS Ultimate Comments #4-40 SHCS Analog Board/30 CRES, A 286 +14.2 > +19.5 4 Bolts # 4-40 SHCS Digital Board/35 CRES, A 286 +13.4 > +18.4 8 Bolts #4-40 SHCS Top Cover/37 CRES, A 286 brittle > +1.5 4 Bolts #2-56 SHCS Bottom Cover/32 CRES, A 286 Brittle > +0.2 4 Bolts #10-32 SHCS Mounting Feet/6 CRES, A 286 +2.8 +3.1 6 Bolts Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 21 CRaTER CDR Mechanical Design Mechanical Design Details Summary • The first fundamental frequency is estimated to be 327 Hz. – Not required to submit an FEM since our predicted first frequency is >75 Hz. – Meets stowage and deployed frequency requirements • • Design meets all factors of safety. All positive margins of safety. No Fracture Critical Items. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 22 CURRENT BEST ESTIMATE, MASS PROPERTIES grams lbs Analog CCA 340 0.75 Electronics Assembly Digital CCA 362 0.80 DC/DC converters and EMI filter 100 0.22 Interconnect Cable, A/D 91 0.20 Internal E-box wire, heater, Thermostats, connectors 227 .50 Mechanical Enclosure 1848 4.08 Top Cover 195 0.43 Connector access cover 32 0.07 Bottom Cover 240 0.53 InternalHardware 163 0.36 Purge system 113 0.25 Electronics Assembly Sub-Total 3710 8.19 Detector Assembly Sub- Total 1309 2.89 MLI and TPS Sub-Total 249 .55 Mounting Hardware Sub-Total 41 .09 5309 11.72 CRaTER CBE Total CRaTER CDR Mechanical Design Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 23 CRaTER CDR Mechanical Design Engineering Unit Drawing List Drawing Number Drawing Title Rev. Layout Complete 32-20000 CRaTER Assembly 90% 32-20200 Electronics Assembly 90% 32-20201 Digital Electronics, PWA 32-20201.0101 Digital Electronics, PWB 32-20201.01 Digital Electronics, Outline Dwg. 32-20202 Analog Electronics PWA 32-20202.0101 Analog Electronics, PWB Dwg 32-20202.01 Analog Electronics, Outline Dwg. 32-20203 Electronics Enclosure 32-20204 Cover, Top 32-20205 Cover, Bottom 32-20206 Cover, Access 32-20208 Cable, Interconnect D/A Drawing Created Checked Released B 100% √ √ √ A 100% √ √ √ √ √ √ A 100% √ √ 01 100% √ √ √ 01 100% √ √ √ 01 100% √ Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 24 CRaTER CDR Mechanical Design Material Properties Density 1 1 1 2 Material Aluminum 6061-T6 Aluminum 7075-T651 A286 AMS 5731 Polyimide 30% glass 3 (lb/in ) 0.098 0.101 0.287 0.065 Young's Tensile Tensile Modulus Ultimate Yield (ksi) (ksi) (ksi) 9,900 35 42 10,300 58 68 29,100 85 130 450 24 Poisson's Ratio 0.33 0.33 0.31 - Where Used Access Cover Covers, Structure Fasteners Circuit Board 1. MIL-HDBK-5J 2. Efunda materials list via efunda.com Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 25 CRaTER CDR Mechanical Design Mechanical Requirements and Verification Summary Requirement Section Description Method 3.1.1.2 Net cg limit load 3.1.4.2 Sinusoidal Vibration Loads A,T 3.1.6.1 Random Vibration A,T 3.1.7 Shock environment A,T 3.1.8 Venting A, I Stowed fundamental Frequency A,T 3.2.2.1 A 3.3.1 Factors of Safety A 3.3.2 Test Factors A Frequency verification and reporting T 3.3.3.2 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 26 CRaTER CDR Mechanical Design Mechanical Requirements and Verification Summary • We also meet all of our internal requirements: – – – – – – – – – – Have adequate contact area (.5 in^2 min) to the spacecraft to support Thermal requirements. (min is .51 in^2) Provide safe structure, within Factors of Safety specified, to support Telescope Assembly. Provide for mounting 2 Circuit Card Assemblies. • The Analog Board and Digital Board must be separated by an aluminum plate. The Analog Board to provide direct linear path for electronics from the telescope interface to the Digital Board interface to reduce noise. Provide means to route cable from telescope to the Analog side of the Electronics Enclosure with minimizing noise. Electrically isolate the Electronics Enclosure from the Telescope, yet provide sufficient thermal conductance path. Provide adequate surface area for mounting electrical components. Interface to the Spacecraft to be on one side of the Electronics Enclosure. • The interface connectors to be on the Digital side of the Electronics Enclosure (separate from the Analog side) Provide GN2 purge interface inlet and outlet ports. Follow the octave rule for natural frequency of the PWAs to the Electronics Enclosure. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 27 CRaTER CDR Mechanical Design Overview Assembly Description Mechanical Environments and Requirements – Imposed – Internal Mechanical Design Details Near Term Tasks Back-up slides Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 28 CRaTER CDR Mechanical Design NEAR TERM TASKS FROM PDR – Update MICD to reflect latest configuration. • Released the MICD. – Further develop analysis on natural frequencies and stresses using SOLID WORKS and COSMOS on the complete CRaTER Assembly. • Completed all natural frequency and stress analysis. – Finalize interface between Telescope Assembly and Electronics Box Assembly. • Specify the electrical isolation material between the telescope and the E-Box. – Identify the GN2 purge system (mechanical interface to the spacecraft, internal flow, pressure measurements…) • Completed the design of purge system. – Complete the drawings for part and assembly fabrication. • Completed the fabrication drawings for the engineering unit. Assembly drawings are in process. • Flight drawings to be completed shortly after engineering unit is completed and tested. – Define attachment points and outline for thermal blankets. • To be completed after Engineering unit is finished. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 29 CRaTER CDR Mechanical Design NEAR TERM TASKS-Post CDR – – – – Finish assembly of the Engineering Unit. Complete the drawings of FLIGHT parts and assembly for fabrication. Define attachment points and outline for thermal blankets. Vibration testing of Engineering Unit. Generate procedures for Vibe tests. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 30 CRaTER CDR Mechanical Design Backup Slides Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 31 Stress Margins Results • Load levels are dominated by random vibration spec. • Factors of Safety, FS, used for corresponding material (MEV 5.1) * - Metals: 1.25 Yield, 1.4 Ultimate - Composite: 1.5 Ultimate CRaTER CDR Mechanical Design Margin of Safety (MOS)= (Allowable Stress or Load)/(Applied Stress or Load x FS)-1 Description CRaTER Assembly Analog Board Digital Board E-Box Enclosure Top Cover Bottom Cover First Frequency (Hz) Q Associated g load (g) 3 sigma load (g) 1516 30 62.8 188.5 195 20 31.3 93.9 15212 4.8 - 0.1 198 20 31.5 94.6 8646 2.8 - 0.9 1239 50 90.3 270.8 284 50 43.2 129.5 351 50 66.4 199.2 Max Stress Min FOS Y Min FOS U (psi) #VALUE! MOS MOS Yield ULT #VALUE! #VALUE! #VALUE! #VALUE! #VALUE! #VALUE! 5738 10.11 11.9 7.1 7.5 43497 1.33 1.6 0.1 0.1 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 32 CRaTER Assembly Resonance CRaTER CDR Mechanical Design • First Mode 326 Hz • Dominant Mode 1516 Hz Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 33 CRaTER Assembly Stresses CRaTER CDR Mechanical Design • Using Miles Equation, Assume Q=20, • 3 sigma g loading= 154 g • Max Stress is 21,400 psi • MOS Y= 1.7 • MOS U= 1.8 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 34 Analog Board Resonance CRaTER CDR Mechanical Design • First Mode 195 Hz Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 35 Analog Board Stresses CRaTER CDR Mechanical Design • Using Miles Equation • Assume Q=20, • 3 sigma g loading= 93.9g • Max Stress is 15,212 psi • MOS Ult= 0.1 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 36 Digital Board Resonance CRaTER CDR Mechanical Design • First frequency is 198 Hz. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 37 Digital Board Stresses CRaTER CDR Mechanical Design • Using Miles Equation • Assume Q=20, • 3 sigma g loading= 85.3 g • Max Stress is 8,646 psi • MOS Ult= 0.9 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 38 Top Cover Resonance CRaTER CDR Mechanical Design • First Mode 288 Hz Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 39 CRaTER CDR Mechanical Design Top Cover Stresses • Using Miles Equation, Assume Q=20, • 3 sigma g loading= 98 g • Material is aluminum • Max Stress is 4248 psi • MOS Y= 6.9 • MOS U= 6.1 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 40 Bottom Cover Frequency CRaTER CDR Mechanical Design • First frequency is 351 Hz. Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 41 Bottom Cover Stresses CRaTER CDR Mechanical Design • Using Miles Equation, • Assume Q=20, • 3 sigma g loading= 126 g • Max Stress is 23.8 kpsi • FOS= 3.1 • MOS Y= 1.5 • MOS U= 1.5 Cosmic RAy Telescope for the Effects of Radiation 7/15/2016 42