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RLEP Overview. James G. Watzin GSFC/Code 430 (RLEP) August 16-17, 2005. LRO Identified in Exploration Vision.
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RLEP Overview James G. Watzin GSFC/Code 430 (RLEP) August 16-17, 2005
LRO Identified in Exploration Vision “Starting no later than 2008, initiate a series of robotic missions to the Moon to prepare for and support future human exploration activities”- Space Exploration Policy Directive (NPSD31), January 2004 Rationale • Environmental characterization for safe access • Global topography and targeted mapping for site selection and safety • Resource prospecting and assessment of In-Situ Resource Utilization (ISRU) possibilities • Technology “proving ground” to enable human exploration LRO SRR - RLEP
Robotic Lunar Exploration Program- A Historical Context - • GSFC RLEP office established several weeks after announcement of Exploration Vision • RLEP directed to implement LRO “In-House” • The fastest option, with the best assurance of meeting the Exploration objectives by the 2008 launch readiness date, with the lowest risk and the lowest cost reserves required • Advanced (unfunded) concept work could begin immediately despite the fact that the payload and program budget were not yet established • Flexible and robust, in that any changes due to the evolving nature of Exploration could be accommodated without modification of contracts • LRO mission objectives, scope and development strategy quickly outlined by RLEP and OSS, with guidance from the ORDT, for Code T • Identified LRO as “Discovery” class mission • Led to joint AA (codes T, S, U, M) approval of Mission Objectives (2 months) • Enabled rapid development and release of AO (4 months) • Skeletal staff further defined LRO mission until AO selections and funding received one year later • Subsequent maturation of Exploration (and resultant series of reorganizations) brings us to the current construct • Program Director (OSS → SMD → ESMD), Program Management (GSFC → ARC), LRO (GSFC) LRO SRR - RLEP
James Watzin, RLEP Program Manager Date RLEP Organization Robotic Lunar Exploration Program Manager J. Watzin Secretary - TBD Program Director (HQ) R. Vondrak Deputy Program Manager TBD Program Scientist (HQ) T. Morgan Program Business Manager P. Campanella 400 EPO Specialist N. Neal Program Support Manager K. Opperhauser Program DPM/Resources TBD Procurement Manager TBD System Assurance Manager R. Kolecki Future Mission Systems J. Burt 100 400 Program Financial Manager W. Sluder Contracting Officer J. Janus Safety Manager D. Bogart Mission Flight Engineer M. Houghton General Business P. Gregory K. Yoder 200 Manufacturing Engineer N. Virmani 400 Scheduling A. Eaker Avionics Systems Engineer P. Luers Mission Business Mgr. J. Smith Materials Engineer P. Joy 500 CM/DM D. Yoder Resource Analysts TBD RM Coordinator A. Rad MIS A. Hess J. Brill 300 Payload Systems Manager A. Bartels Ground Segment Manager R. Schweiss Launch Vehicle Manager T. Jones Lunar Reconnaissance Orbiter (LRO) RLE 2 RLE 3 400 400 400 RLE 4 Project Manager C. Tooley RLE n Mission 2 400 400 Mission 3 Mission 4 Mission n 07/15/2005 LRO SRR - RLEP
Path to LRO SRR Vision RLEP established at GSFC by OSS ORDT $500K Established Scope, Scale & Risk Posture LRO PM & SE Objectives PIP POP 04-1 submitted AO SMD $500K AO Proposals $300K Conducted Limited Preliminary Project Planning & Mission Trades Program Review AO Selection $40M -$13M POP 05-1 submitted Executed Rapid Combined Phase A/B $12M ESMD Level 1 Req’ts AMES SRR LRO SRR - RLEP
The PIP (companion to AO) was the project’s 1st product and contained the result of the rapid formulation and definition effort. The PIP represents the synthesis of the enveloping mission requirements drawn from the ORDT process with the defined boundary conditions for the mission. For the project it constituted the initial baseline mission performance specification. Key Elements: Straw man mission scenario and spacecraft design Mission profile & orbit characteristics Payload accommodation definition (mass, power, data, thermal, etc) Environment definitions & QA requirements Mission operations concept Management requirements (reporting, reviews, accountabilities) Deliverables Cost considerations LRO Development – PIP Strawman Orbiter One year primary mission in ~50 km polar orbit, possible extended mission in communication relay/south pole observing, low-maintenance orbit LRO Total Mass ~ 1000 kg/400 W Launched on Delta II Class ELV 100 kg/100W payload capacity 3-axis stabilized pointed platform (~ 60 arc-sec or better pointing) Articulated solar arrays and Li-Ion battery Spacecraft to provide thermal control services to payload elements if req’d Ka-band high rate downlink ( 100-300 Mbps, 900 Gb/day), S-band up/down low rate Centralized MOC operates mission and flows level 0 data to PI’s, PI delivers high level data to PDS Command & Data Handling : MIL-STD-1553, RS 422, & High Speed Serial Service, PowerPC Architecture, 200-400 Gb SSR, CCSDS Mono or bi-prop propulsion (500-700 kg fuel) LRO Development AO & PIP LRO SRR - RLEP
How LRO Measurement Objectives Will Be Met by the Selected Instrumentation • Specific measurement sets solicited on the basis of the objectives stated in LRO AO: • Characterization of deep space radiation in lunar orbit, including neutron albedo (> 10 MeV): biological effects and properties of shielding materials • NS (neutron albedo beyond 10 MeV, globally) → partially addresses (neutrons only) • Rad (Tissue Equiv. GCR response) → partially addresses (GCR uncertainty) • Geodetic lunar topography (at landing-site relevant scales) • Lidar (10-25 m scales in polar regions; 10 m along track globally) → Completes (definitive) • High spatial resolution hydrogen mapping of the lunar surface • NS (5-20km scale H mapping globally, 5kmin polar regions) → Completes (best achievable) • Temperature mapping of the Moon’s polar shadowed regions • IR (300m scale at ~3K from 40-300K) → Completes • Landform-scale imaging of lunar surfaces in permanently shadowed regions • Lidar (topo, 1 um reflectivity in polar regions at 25m scales) • IR (mid IR imaging at 300m scale) • Imaging (near UV imaging at 400m scale) • NS (“imaging” H at ~5km scales) • Identification of putative deposits of appreciable near-surface water ice in lunar polar cold traps • NS (5km scale h mapping in upper meter at 100 ppm sensitivity) → Completes (@ 5km scale) • Lidar (via reflectivity at 10m scales) → Partially addresses (depends on sampling) • Assessment of meter or small-scale features to facilitate safety analysis for potential lunar landing sites • Imaging (<50 cm/pixel GSD across > 100 km2 areas) → Completes • Characterization of the Moon’s polar region illumination environment at relevant temporal scales (i.e., typically that of hours) • Imaging (100m scale UV-VIS-NIR images per orbit) → Completes (with Lidar 3D context) • Lidar (via topography and reflectivity) → Completes at 10’s m scales in 3D, with IR Completes (except for regolith characterization [3D]) Expected data products are captured as the LRO Level 1 Requirements LRO SRR - RLEP
Evolution of the LRO Programmatic Requirements • Program prescribed by the Vision • Schedule defined by the Vision • Scope and scale derived (by OSS and RLEP) from original budget guidelines and schedule • Mission concept and implementation strategy derived (by RLEP and OSS) for code T • Mission measurements outlined by ORDT and definitized through the selection of AO proposals • Level 1 requirements codified selected data products The LRO development is the living history of the evolution of its’ mission requirements The baselining of Level 1 requirements enables a structured and disciplined path forward into development LRO SRR - RLEP