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SMD Perspectives @ ARCtek
       Michael D. Bicay
         Director for Science
      NASA Ames Research Center
               2012.01.18
NRC Decade Survey (2010): Astronomy & Astrophysics

≒     Large Space-Based Programs (priority order)
     1. WFIRST: Wide-Field Infrared Survey Telescope
     2. (Astrophysics) Augmentation to Explorer Program
     3. LISA: Laser Interferometer Space Antenna
     4. ISO: International X-Ray Observatory
     [Note: #3 and #4 have been cancelled; funding for #1 has not been
         identified.]

≒    Medium Space-Based Programs (priority order)
     1. New Worlds Technology Development
     2. Inflation Probe Technology Development
NRC Decade Survey (2011): Planetary Sciences
                                           Flagship Missions

          Recommended                     Cost Constrained                    Less Favorable
≒ Descoped Mars Astrobiology        ≒ Descoped MAX-C                  ≒ Descope/Delay Flagships
  Explorer Cacher (MAX-C)            ≒ UOP
≒ Descoped Jupiter Europa Orbiter
  (JEO)                                                                  We are here!
≒ Uranus Orbiter/Probe (UOP)
≒ Enceladus Orbiter
≒ Venus Climate Mission




      ≒ Discovery-Class Mission every 24 months (<$500M, excl. LV)
      ≒ New Frontiers-Class Mission, two total in 2013-2022 (<$1B, excl. LV)
      ≒ Augmentation to R&A Program (+5% in FY12, +1.5% subsequently)
      ≒ Technology Development (~7% of total Planetary budget)
Fully Competitive SMD Flight Missions
Schedule of SMD Flight Solicitations
SMD Opportunities                                    ARC Capabilities
≒ Roles in Strategic Missions                       ≒ Drilling Technologies, Sample Handling Tech.
       ≒ Mars Sample Return (early 2020s)           ≒ XRD/XRF analysis
              ≒ Cache Box, Drilling                 ≒ Exobiology / Planetary Protection
       ≒ Exoplanet Imaging (late 2020s)             ≒ EDL/TPS
              ≒ Imaging (Internal) Coronagraph      ≒ PIAA Technology Testbed
≒ Fully Competed Missions                           ≒ Kepler Science Operations Management
       ≒ Earth Venture Missions                     ≒ In Situ & Remote Sensing Instruments
              ≒ Airborne, Instruments, Orbital      ≒ ESPO Project Management (airborne)
       ≒ Comet Coma Sample Return (New Frontiers)   ≒ SmallSat Management
       ≒ Mars IceBreaker (Discovery)                ≒ Small Bodies Science (comets, NEOs)
       ≒ DARE (Explorer)                            ≒ Sample Return Science

             Technologies Needed                               Other Needs to Succeed
≒ Drilling Technologies to 2+m depth                ≒ Stable funding for space/Earth sciences
≒ Robust sample handling/archiving                  ≒ Robust Core Competencies
≒ Second-generation CheMin instrument               ≒ Re-invigoration of drilling/analog work
≒ Robust EDL/TPS Program (w/ LaRC)                  ≒ Continued PIAA Coronagraph development
≒ Demonstrated PIAA Coronagraph                     ≒ New EarthSci hires (in process)
       ≒ High contrast, Small IWA                   ≒ Development of strategic partnership w/ APL
       ≒ Compact architecture                       ≒ Fair TMCO assessment of competed proposals
≒ Compact EarthSci Instruments
≒ Comet coma probe & sample acquisition system
≒ Low-cost launch to cislunar space
ACE: Ames Coronagraph Experiment




                                                            2nd-generation PIAA mirrors

                                                  ≒ Setting new contrast benchmarks
                                                      ≒ 1.9e-8 from 2.0 to 3.4 了/D
                                                      ≒ 1.4e-6 from 1.2 to 2.0 了/D
                                                  ≒ Active thermal control system achieved
may detect exo-earths with differencing methods      0.4mK stability rms over ~1 hour.
     can see exo-earths on raw image

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Bicay_Post

  • 1. SMD Perspectives @ ARCtek Michael D. Bicay Director for Science NASA Ames Research Center 2012.01.18
  • 2. NRC Decade Survey (2010): Astronomy & Astrophysics ≒ Large Space-Based Programs (priority order) 1. WFIRST: Wide-Field Infrared Survey Telescope 2. (Astrophysics) Augmentation to Explorer Program 3. LISA: Laser Interferometer Space Antenna 4. ISO: International X-Ray Observatory [Note: #3 and #4 have been cancelled; funding for #1 has not been identified.] ≒ Medium Space-Based Programs (priority order) 1. New Worlds Technology Development 2. Inflation Probe Technology Development
  • 3. NRC Decade Survey (2011): Planetary Sciences Flagship Missions Recommended Cost Constrained Less Favorable ≒ Descoped Mars Astrobiology ≒ Descoped MAX-C ≒ Descope/Delay Flagships Explorer Cacher (MAX-C) ≒ UOP ≒ Descoped Jupiter Europa Orbiter (JEO) We are here! ≒ Uranus Orbiter/Probe (UOP) ≒ Enceladus Orbiter ≒ Venus Climate Mission ≒ Discovery-Class Mission every 24 months (<$500M, excl. LV) ≒ New Frontiers-Class Mission, two total in 2013-2022 (<$1B, excl. LV) ≒ Augmentation to R&A Program (+5% in FY12, +1.5% subsequently) ≒ Technology Development (~7% of total Planetary budget)
  • 4. Fully Competitive SMD Flight Missions
  • 5. Schedule of SMD Flight Solicitations
  • 6. SMD Opportunities ARC Capabilities ≒ Roles in Strategic Missions ≒ Drilling Technologies, Sample Handling Tech. ≒ Mars Sample Return (early 2020s) ≒ XRD/XRF analysis ≒ Cache Box, Drilling ≒ Exobiology / Planetary Protection ≒ Exoplanet Imaging (late 2020s) ≒ EDL/TPS ≒ Imaging (Internal) Coronagraph ≒ PIAA Technology Testbed ≒ Fully Competed Missions ≒ Kepler Science Operations Management ≒ Earth Venture Missions ≒ In Situ & Remote Sensing Instruments ≒ Airborne, Instruments, Orbital ≒ ESPO Project Management (airborne) ≒ Comet Coma Sample Return (New Frontiers) ≒ SmallSat Management ≒ Mars IceBreaker (Discovery) ≒ Small Bodies Science (comets, NEOs) ≒ DARE (Explorer) ≒ Sample Return Science Technologies Needed Other Needs to Succeed ≒ Drilling Technologies to 2+m depth ≒ Stable funding for space/Earth sciences ≒ Robust sample handling/archiving ≒ Robust Core Competencies ≒ Second-generation CheMin instrument ≒ Re-invigoration of drilling/analog work ≒ Robust EDL/TPS Program (w/ LaRC) ≒ Continued PIAA Coronagraph development ≒ Demonstrated PIAA Coronagraph ≒ New EarthSci hires (in process) ≒ High contrast, Small IWA ≒ Development of strategic partnership w/ APL ≒ Compact architecture ≒ Fair TMCO assessment of competed proposals ≒ Compact EarthSci Instruments ≒ Comet coma probe & sample acquisition system ≒ Low-cost launch to cislunar space
  • 7. ACE: Ames Coronagraph Experiment 2nd-generation PIAA mirrors ≒ Setting new contrast benchmarks ≒ 1.9e-8 from 2.0 to 3.4 了/D ≒ 1.4e-6 from 1.2 to 2.0 了/D ≒ Active thermal control system achieved may detect exo-earths with differencing methods 0.4mK stability rms over ~1 hour. can see exo-earths on raw image