Planetary Science Division Update
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1 Planetary Science Division Update Jim Adams Deputy Director, Planetary Science NASA Headquarters May 10, 2011 Presentation to the Planetary Protection Subcommittee
2 Outline PSD Plan to Respond to the Decadal Survey Recent Discovery Selections
3 Planetary Program Architecture Recommended by the Planetary Decadal Survey Large Missions ( Flagship -scale) Recommended Program (budget increase for JEO new start) 1) Mars Astrobiology Explorer-Cacher descoped 2) Jupiter Europa Orbiter (JEO) descoped 3) Uranus Orbiter & Probe (UOP) 4/5) Enceladus Orbiter & Venus Climate Mission Cost Constrained Program (based on FY11 Request) 1) Mars Astrobiology Explorer- Cacher descoped 2) Uranus Orbiter & Probe (UOP) Less favorable budget picture than assumed (e.g., outyears in FY12 request) Descope or delay Flagship mission Discovery $500M (FY15) cap per mission (exclusive of launch vehicle) and 24 month cadence for selection New Frontiers $1B (FY15) cap per mission (exclusive of launch vehicle) with two selections during Research & Analysis (5% above final FY11 amount then ~1.5%/yr) Technology Development (6-8%) Current Commitments (ie: Operating Missions)
4 Planetary Funding Profiles FY11 and FY12 Requests President s FY11 Budget + inflation Decadal planning budget R&A President s FY12 Budget* Disco NF Lunar Assumed Flat Budget Mars *Notional Budget in RY$ Outer Planets
5 Decadal Decision Rules Page 9-6: NASA s suite of planetary missions should consist of a balanced mix of Discovery, New Frontiers, and Flagship missions, enabling both a steady stream of new discoveries and challenges Page 9-21: It is also possible that the budget picture could turn out to be less favorable If cuts to the program are necessary, the committee recommends that the first approach should be descoping or delaying Flagship missions. Changes to the New Frontiers or Discovery programs should be considered only if adjustments to Flagship missions cannot solve the problem. Actions based on Decadal Guidance: Maintain a balanced program small, medium, large missions Maintain a partnership with ESA Descope flagship missions as a first resort due to tight budgets If flagship descopes are not sufficient then stretch out New Frontiers and Discovery A/Os
6 PSD Decadal Budget Planning Lay In Current Commitments All Operating Missions Through Expected End of Life Current R&A Awards All missions in development or competition Juno, GRAIL, MSL, LADEE, MAVEN, EMTGO New Frontiers-3, and Discovery 12 In-Space Propulsion Technology Radioisotope Power System Program Pu-238 Production Accommodate Decadal Recommendations Maintain a healthy R&A program Discovery AO s on 2 year Cadence New Frontiers AO s on 5 year Cadence Mars 2018 Cache Rover Directly Tied to MSR Includes initiation of MSR high-priority technologies wedge Per OMB $10M/year set aside for cooperative activities with Human Exploration Full decadal recommendations greatly exceed President s FY12 Budget Must use decision rules from decadal to develop a balanced budget
7 Approach to Develop new Notional Budget Capped R&A at $200M/year Next Discovery AO on current <36 month cadence All subsequent AO s accelerated to 24 Month Cycle Select NF-3 planned for NF-4 and NF-5 within decade Will maintain New Frontiers schedule Extended Mission budget for ALL operating missions Senior Review used for determining which missions to be extended Dedicated Lunar R&A wedge transferred to PSD R&A Residual Lunar Quest Program moved to Discovery JEO Descoped to Studies Funded FY11/12 No JEO Instrument AO Budget for some radiation technology efforts
8 Overall Program Content Mars Exploration Program (Negotiated with ESA) EMTGO, MOMA, Mars 2018 (JR-1), Management, Future missions Discovery Program Strofio, LaRa, Disc-12, Management, Future missions New Frontiers Program NF-3, Management, Future missions Technology Program PIDDP, ASTID, ISP, RPS, MSR Tech, OP Tech Planetary R&A Move PIDDP and ASTID to Technology Program Mission Commitments (operating etc.) GRAIL, Juno, MSL, MAVEN, LADEE, MER, MRO, Odyssey, Mars Express, Dawn, New Horizons, LRO, MESSENGER, Deep Impact, Stardust, ASPERA-3, Rosetta, Cassini Other Commitments Pu-238, AMMOS, OPF studies, JGO/ESA MOO, Joint coordination w/hsf Operating Development In Competition
9 9 A PSD Notional Decadal Budget
10 Road to Response March 7, 2011 Decadal Survey Released at LPSC April 5, 2011 Response Strategy Briefing to OMB Budget Guidelines and DS Objectives Reconciled Cataloging of Recommendations (200+) Completed Consolidated into 37 Actionable Recommendations Writing Assignments May 6, 2011 Rough Draft Assembled June 12, 2011 Draft Supplied to PSS June 26, 2011 PSS Comments on PSD Response July, 2011 Final Response Delivered to NRC
11 Discovery 12 Selections
12 031- CHopper: Comet Hopper PI: Jessica M. Sunshine Mission & Science Team: PI: Jessica Sunshine, UMD Deputy PI: M. A Hearn, UMD Project Management: GSFC S/C: LM Mission Ops: LM Science Ops: UMD Mission: Comet Wirtanen rendezvous and landing mission using LM S/C. 4 sorties between 4.5 and 1.5 AU from Sun. Goals: Map spatial heterogeneity of gas & dust emissions and surface solids Determine nucleus structure, geologic processes, coma mechanisms Document changes w/ increasing isolation Instruments: CHIRS- CHopper Infrared Spectrometer CHIMS- CHopper Ion/Neutral Mass Spectrometer CHI- CHopper Imager CHEX- CHopper Heating Experiment PanCams- Panoramic Cameras Mission Details: Flight: 2016 launch with Standard 4m LV, 34-day launch period Mission: 7.3-yr mission, 2022 rendezvous / science ops Science Phase: Remote survey and multiple in situ surface measurements Cruise/Parked Ops: Quiescent ops during cruise and between sorties, science data downlink Spacecraft: high-heritage spacecraft design, flightproven components for reliability and long life, large systems margins, dust covers for robustness in cometary environment, two ASRGs supply continuous power during all mission phases 12
13 008- GEMS: GEophysical Monitoring Station PI: Bruce Banerdt Mission & Science Team: PI: Bruce Banerdt, JPL PM: Tom Hoffman, JPL Deputy PI: Sue Smrekar, JPL Spacecraft: Lockheed-Martin (LM) Operations: JPL/LM Payload: JPL, IPGP (France), DLR (Germany) Mission: Geophysical (seismology, heat flow, planetary rotation) lander mission on Mars using Phoenix heritage spacecraft Goals: Understand formation/evolution of terrestrial planets via interior structure/processes of Mars Determine present tectonic activity and meteorite impact rate Payload: Seismic Experiment for Interior Structure (SEIS) Rotation & Interior Structure Experiment (RISE) Heat Flow & Physical Properties Probe (HP 3 ) Instrument Deployment Arm (IDA) Instrument Deployment Camera (IDC) Mission Details: Flight: 3/2016 launch w/elv, 4m fairing; 9/2016 landing; ~6.5 mo cruise, 1 Mars yr surface ops Selected Systems Features (Phoenix-based design): Cruise: 3-axis stabilized, 3.2 m 2 UTJ solar array, X- band telecom; EDL: Landing radar, UHF telecom; Surface: 4.3 m 2 UTJ solar array, 2 Li-ion batteries, UHF telecom, Rad 750-based avionics Mass: 597.6kg dry launch, margin 31% (depending on ELV) Surface Ops Energy: 881Wh/sol, margin 180% Schedule: 39 mo B/C/D, 98 days sched reserve Threshold Mission: Descope: HP 3, SEIS SP sensors 13
14 TiME: Titan Mare Explorer PI: Ellen Stofan Mission & Science Team: PI: Ellen Stofan, Proxemy Project Mgmt: APL S/C: LM Ops: LM, JPL (nav) Payload: APL, GSFC, MSSS Deputy PI: J. Lunine, UA Project Scientist: R. Lorenz, APL Mission: Lander msn to Titan s Ligeia Mare methaneethane polar sea, 96 days on surface Goals: Understand Titan s methane cycle through study of a Titan sea. Investigate Titan s history & explore the limits of life Instruments: Meteorology & physical properties (MP3) Mass Spec for Lake Chemistry (NMS), Descent and Surface Imaging Cameras Efficient Trajectory: Launch 2016 Cruise 7.5 years (EGA, JGA) Entry 2023 Mission Features: Focused science objectives High-heritage instruments Simple cruise, no flyby science Simple surface operations ASRGs, launch vehicle are GFE 14
15 Flyby, Orbit, Land, Rove, and Return Samples NASA s 15
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