Results from the JWST Testing Assessment Team Review Erin Elliott 18 November 2010 Context • Testing Assessment Team (TAT) was tasked by NASA HQ to review JWST’s integration and test plans. • Prompted by a request for review from Senator Mikulski. • Members: John Casani, Chair, Jet Propulsion Laboratory Alan Dressler, Carnegie Observatories Matt Mountain, Space Telescope Science Institute Jerry Nelson, University of California–Lick Observatory Jim Oschmann, Ball Aerospace Al Sherman, Allan Sherman, LLC Georg Siebes, Jet Propulsion Laboratory Erick Young, USRA Bill Irace, Jet Propulsion Laboratory Milt Heflin, NASA Johnson Space Center Jeff Kegley, NASA Marshall Space Flight Center Mike Ryschkewitsch, NASA • Review focused on: – ISIM testing at GSFC – OTIS testing at JSC (OTIS = OTE + ISIM) November 18, 2010 2 JWST Architecture November 18, 2010 3 Overview of JWST I&T November 18, 2010 4 ISIM Testing Overview • ISIM testing uses an OTE simulator (OSIM) • Each cryo cycle takes 20 weeks (7 wks of cooldown & warmup) • Thermal tests include – Measurement of total load ISIM puts on cryocooler – Measurement of ISIM radiators and straps • Optical tests include – SI to ISIM pupil shear and focus – SI wavefront errors – Data needed for ISIM to AOS alignment – Plate scale measurements – WFSC calibrations November 18, 2010 5 OTIS Testing November 18, 2010 6 OTIS Testing • Single cryo cycle planned, taking 170 days. • Cost is about $1,000,000 per day! • Thermal tests include: – OTE temperature – Core isolation performance – ISIM electronics compartment isolation performance – ISIM & line loads Optical tests include: • Primary / secondary alignment to the AOS • Primary / secondary actuator ranges • ISIM to AOS alignment • Final plate scales • Primary mirror ROC, conic, astigmatism, tilt • Closed-loop WFSC demonstration • Rogue, truant path checks November 18, 2010 Cryo Position Metrology Primary Mirror LF WFE & Stability SM PG PG AOS PG PG PM 7 TAT Conclusions The TAT Team concluded that the ISIM testing at GSFC can be reduced from 14 months to 10 months and believes the OTIS testing at JSC can be reduced from 167 days to 90 days with acceptable reduction in pre-launch predictability of performance and without predictable loss of science capability. This reduction could shorten the critical path, avoiding significant cost growth. November 18, 2010 8 TAT Recs – Science & Testing Priorities • Prioritize key system requirements, and design and implement the test program using those priorities. • Conclude OTIS testing in 90 days. Continued work is only justified by substantial risk to Level 1 science requirements. • Prioritize functional tests over performance tests. Complete functional tests early in the test sequence. • There is a range of test temperatures in which all instruments but MIRI can be verified. MIRI verification should not drive a second OTIS cycle nor prolong the first test cycle. – Test plan should be driven by NIRCam, FGS, and NIRSpec. • Test all detectors at temperatures up to at least 60 K. – NIRSpec data wasn’t taken at the time. • Make an effort to obtain new NIRSpec flight detectors with improved dark-current performance. – Observatory could operate over wider range of on-orbit temps. November 18, 2010 9 TAT Recs – Organization and Decision Making • Establish an I&T Lead responsible for defining and documenting a clear I&T approach. • Adopt overall I&T plan that maximizes efficiencies over the entire test program. Goal is to minimize risk of cost and schedule growth during OTIS testing. – High risk of needing a second cryo cycle at OTIS. • Develop decision criteria and contingency plans for OTIS testing. • Employ a command-and-decision structure during OTIS testing similar to the one used for the Hubble Servicing Missions. • Assess implications of proposed SE reorg. Make sure GSFC has the necessary staff to support it. November 18, 2010 10 TAT Recs – Optical Testing • Priorities at JSC should be: – Mechanism tests – Photogrammetric optical alignment – AOS to ISIM alignment – Verification of integrated FSM/ FGS functionality – COC testing of the primary mirror • Establish clear pass/fail criteria. Put cross-checks and extrapolations to on-orbit performance as optional tests. • Eliminate cryo frill and rogue-path tests and reduce the scope of the pass-and-a-half testing. • Eliminate CPT testing at the ISIM and OTIS levels. Do at SI level. • Reduce WFSC demonstrations, concentrating on functional testing and polarity checks. • Increase concurrent optical and thermal testing during ISIM testing. November 18, 2010 11 TAT Recs – Thermal Testing • Combine the two thermal balance points in the OTIS testing to a single test. – Add a core test, updated to the current flight design. – Add thermal testing to the Pathfinder testing. • Eliminate the first ISIM cryo test. – Add a cryo test with OSIM and the NIRCam ETU (off the critical path). – Measure SI displacements during proof-load testing. • Postpone installation of OTIS GSE until after chamber commissioning. • Shorten thermal model turnaround times to a few hours. – Prevents costly delays during OTIS testing. • Develop tiered criteria that permit progressive assessments based on information as it evolves, and reduce test time where possible. • Increase parallel optical and thermal testing during OTIS testing. • Apply available radiator margin to reduce stabilization times. November 18, 2010 12 How do we build and test larger missions? • Interesting higher-level discussion during TAT proceedings. • “Test as you fly” is a well-established NASA rule. – Waivers required when testing doesn’t meet the requirement. • JWST already in the regime where that is not possible. – OTIS testing takes place with a sunshield and spacecraft simulator. • Electrical connections, etc., made after OTIS testing won’t be performance-tested at cryo. – A return flat isn’t available for a full-aperture end-to-end optical test. • Three small flats are used instead. – The JSC chamber doesn’t recreate the flight thermal environment. • Clearly can’t build larger chambers and test mirrors as the collecting areas increase. • How do we build systems in pieces and guarantee that the system will work correctly after assembly? November 18, 2010 13 How do we ensure thermal performance in JWST and larger missions? • Two schools of thought on thermal testing: 1. Test in a very flight-like environment. – Thermal models used during design stage only. 2. Accept testing in a non-flight-like environment and use thermal models to predict on-orbit performance. • • • • JWST uses approach # 2. – Facility large enough to create a flight-like environment doesn’t exist. – JWST is passively cooled. Error in thermal design could equal lost mission, not just a shorter mission lifetime. – Accuracy and turnaround times for the thermal models is a constant struggle. – Thermal balance tests are very time-consuming and $. Several NASA missions launched recently are running warmer than predicted. These are actively cooled missions, so leads to shorter mission lifetimes. There is a need to review the missions as a group to look for common issues. But also: How do we make systems more robust w.r.t. operating in varying thermal environments? – Part of the answer is to pursue detectors with improved dark current vs. T performance. November 18, 2010 14