Hertz & the 2020 Decadal Survey: a PAG Panel Discussion!

Transcription

1 !Getting a Charge Out of Paul Hertz & the 2020 Decadal Survey: a PAG Panel Discussion! High-Energy Space Missions in the 2020s July 1, 2015 Mark Bautz, Scott Gaudi, Joseph Lazio

2 NASA s Charge to the PAGs. I am charging the Astrophysics PAGs to solicit community input for the purpose of commenting on the small set [of large mission concepts to study], including adding or subtracting large mission concepts.

3 Detailed Charge, Part Each PAG, under the leadership of its Executive Committee, shall broadly solicit the astronomy and astrophysics community for input to the report in an open and inclusive manner. To accomplish this, each PAG is empowered to envision and use its own process. 2. Each PAG will consider what set of mission concepts should be studied to advance astrophysics as a whole; there is no desire for mission concepts to be identified as belonging to a specific Program or PAG. Each PAG shall keep the number of large mission concepts in the set as small as possible. Each PAG is specifically charged to consider modifications and subtractions from the small set, and not just additions. 3. Each PAG shall produce a report, where it shall comment on all large mission concepts in its small set of large missions, including those in the initial small set and those added or subtracted. The PAGs may choose to work together and submit coordinated or joint reports.

4 Detailed Charge, Part Each PAG may choose to have a face-to-face meeting or workshop I in developing its report; said meeting may be scheduled in proximity to an existing community meeting or conference. 5. Although there is no page limit for the report, each PAG shall strive to be succinct. 6. Each PAG shall submit its report in writing no later than two weeks prior to the Fall 2015 meeting of the NAC Astrophysics Subcommittee (meeting schedule not yet known).

5 Timeline for STDTs. 2015: Identify a small set of candidate large missions to study PAG reports due by October 2015 APS meeting : Initiate studies. Conduct studies. Identify technology requirements Deliver results to decadal survey.

6 Initial list of missions. Taken from NASA Roadmap (Surveyors) and Decadal Survey (HabEx) Far IR Surveyor Habitable-Exoplanet Imaging Mission UV/Optical/IR Surveyor X-ray Surveyor

7 Far-IR Surveyor Illustrative Concept Based on Far-IR Workshop Science goals (subset): History of star-formation, black hole growth, and rise of heavy elements with cosmic time from Reionization to the present -- most has been shrouded in dust. Shocks and cooling in primordial H 2 in first collapsed objects. Census of planet-forming gas disks in the Milky Way and its satellites with sensitivity to tens of Earth masses of gas Determine mass and orbital characteristics of the outer solar system population, reaching down to 10 km objects at 60 AU Approach: Cryogenic wide-field surveyor with imaging spectroscopy as its thrust. Wavelength coverage: μm in 6--8 log-spaced bands with R~500 Monolithic telescope diameter ~ 5 m. Telescope actively cooled to < 4 K, instruments cooled to <100 mk. Field of View = 1 deg at 500 μm Mission: 5 years + at Earth-Sun L2 High-resolution (heterodyne) spectroscopy also compelling, possibly for warm phase.

8 HabEx. 4-8m monolith or segmented Needs ~10-10 contrast Coronagraph, wavelength of micron and/or starshade, wavelength of micron Camera IFU, R=70 spectrum of 30 mag exoplanet 1 FOV Optimized for exoplanet direct imaging. Potential for an instrument for spectroscopic characterization of transiting planets. UV-capable telescope/instrument suite would enable compelling COR science. L2 orbit or Earth-trailing

9 Large UVOIR Surveyor 8-16m (likely segmented, obscured primary) HST-like bandpass (91nm ~2-2.5 microns) Suite of imagers/spectrographs Need ~10-10 contrast for planet imaging coronagraph and/or starshade), less contrast for other studies

10 X-ray Surveyor per Astrophysics Visionary Roadmap Effective area ~3 m 2 Sub-arcsecond angular resolution High-resolution spectroscopy (R ~ few x 10 3 ) over broad band via microcalorimeter & grating spectrometer instrumentats FOV 5 Energy range ~ kev

11 Timeline/Meetings for Hertz Charge (completed). *January 2014: Initial discussion at ExoPAG 9. March 2014: APS approves SIG #1. June 2014: Brainstorming session at ExoPAG 10. January 2015: Brainstorming session at ExoPAG 11, Paul s charge. February 2015: First dedicated SIG #1 Meeting, brainstorming & consensus building. March 10 COPAG Virtual Town Hall March 19, 2015: Joint PAG EC meeting. April , Am. Phys. Soc. (Baltimore) - PhysPAG SIGs and PCOS mini-symposium June 2, 2015 ExoPAG Virtual Meeting June 3-5, Far-IR Workshop (Caltech) COPAG June 13-14, ExoPAG #12 (Chicago) - ExoPAG Half to full day to be spent on charge (2 nd day) June 25-25, UV/Vis SIG Meeting, Greenbelt, MD COPAG

12 Timeline/Meetings for Hertz Charge (future). July 1 panel discussion during the HEAD meeting (Chicago) PhysPAG July 14, 2015 ExoPAG Virtual Meeting August 2015 COPAG Virtual Town Hall August 7, Joint PAG Splinter Session at IAU, 1-5pm August 18, 2015 ExoPAG Virtual Meeting July-September 2015: writing, circulating, finalizing report(s?). October 2015: Deliver report to Hertz (two weeks before the APS)

13 COPAG Response to Hertz Charge Process Means for community input Cosmic Origins Website AAS meeting Cosmic Origins UV-Vis and FIR sessions (Jan 4) ExoPAG/COPAG Joint Meeting (Jan 4) Joint PAG Session (Jan 7) NASA Town Hall Meeting (Jan 7) Cross-PAG telecon and joint meetings Virtual Town Hall (March 10) White papers Posted at above COR URL, SIG2 webpages SIG meetings

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15 COPAG Findings on Large Missions in Astro2020 Strong community support for consideration of Far IR Surveyor Habitable Exoplanet Imaging Mission UV/Optical/IR Surveyor Relative paucity of submissions on X-ray Surveyor likely a selection bias Findings dependent upon boundary conditions Proposed missions have broad cross-pag science applications and science synergies Community input would be valuable reference material for Science & Technology Definition Teams (STDTs) Significant interest in Probe-class missions

16 ExoPAG s Response to Paul s Large Mission Charge. Talks, brainstorming, and discussion at ExoPAGs 9, 10, 11, 12, one stand-alone meeting, and one virtual meeting. NASA Astrophysics Roadmap. Solicited (and unsolicited) input from a several dozen members of the community. COPAG White Papers

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18 Past ExoPAG Meetings Devoted to Paul s Charge. SIG #1 Stand-alone Meeting February 10+11, 2015 at JPL. Roughly 45 people attended in person and remotely. Talks, break-out sessions, brainstorming and group discussions. Afternoon of February 11 devoted to Paul s charge. Consensus building. Identified questions and topics for future discussions. SIG #1 Virtual Meeting June 2, 2015 Roughly 40 people attended. Focused on Paul s charge, mostly discussion and consensus building (no talks) SIG #1 Meeting at ExoPAG 12 June 14, 2015 Roughly people attended in person or remotely Talks in the morning, discussions in the afternoon.

19 ExoPAG Points of Consensus. 1. There was a general support for WFIRST with a coronagraph and a starshade. 2. There was a general consensus that a broad range of apertures and architectures for direct imaging missions should be studied, encompassing both the nominal concepts of the HabEx and LUVOIR missions. 3. There was a general consensus that there should be a common executive summary with the other PAG reports. It was agreed that the executive summary should include: a statement that we support these four missions being studied, a recommendation for probe studies, and suggestions for how STDTs should be organized (provided that the other PAGs are in agreement on these points). 4. There was a general consensus that a common table describing the nominal parameters of the four missions should be included in the PAG reports. These parameters are to be determined in future discussions with the ExoPAG and other PAGs. 5. There was a general consensus that we should neither add nor subtract from the four proposed mission concepts (HabEx, LUVOIR, X-ray Surveyor, and Far-IR Surveyor).

20 ExoPAG Points of Consensus, cont. 6. With regards to organization of the HabEx and LUVOIR STDTs, there was a general consensus on the following points: There should be two separate science teams and two separate engineering and technology teams. The science teams should have significant overlap (common members), and should include significant representation from the planetary science community. We should express the following concerns in the report: Exoplanets may get marginalized in the LUVOIR STDT if their representation is too small. The general astronomical community may get fractured if the representation of disciplines is very different between the two STDTs. Thus the members of the science teams should be carefully chosen to ameliorate these concerns. The teams should meet periodically, including the kickoff meeting. There should be a small, independent and unbiased team that is tasked to evaluate the science yield and technical readiness of both mission designs in a consistent and transparent manner.

21 ExoPAG Points of Consensus, cont. 7. There was a general consensus that probe-class (<~$1B) missions should be studied in advance of the next decadal survey, and that the following missions should be presented in the report as examples of possibly compelling probe-class missions. A starshade for WFIRST-AFTA. A transit characterization mission. An astrometry mission.

22 PhysPAG Response to Charge Community discussion and input sought at face-to-face meetings: X-ray-, Gamma- & Cosmic-SIG, PhysPAG & Joint PAG meetings at AAS, January IP-SIG discussions at Minneapolis CMB Pol. Workshop, January Gamma-SIG at Future Space-Based Gamma Observatories, February Joint PAG executives meeting, March Cosmic-, Gravitational-Wave- & Gamma-SIG meetings; PCOS & Gamma Mini-symposia at APS, April Gamma-, X-ray-SIG & various panels, this meeting and in many, many telecons

23 Preliminary PhysPAG Findings On large missions: Supports studies of four Hertz-nominated candidates Strong X-ray community support for X-ray Surveyor Concern that planned US participation in (large) ESA gravitational wave mission must be properly monitored, supported and presented to 2020 Decadal Survey. Concurs that Inflation Probe can be done as a probe; concern that 2010 NWNH recommendations for technology development and mission studies must be carried out. Strong, broad support for NASA attention to probe-class missions as part of its preparation for the 2020 Decadal Survey

24 Reference Material. decadal/

25 Topics of Discussion. Joint PAG Reports? Joint summary. Joint table. Should we add any missions? Should we subtract/merge any missions? The Astrophysics Division s goal is to identify a set of missions that 'advances astrophysics as a whole. Are there major gaps not addressed by this set of missions? How should we organize the STDTs for these missions? Paul Hertz has asked the PAGs for other useful commentary about the set of missions for put forward for study. What commentary would you include? What do we say about probes?

26 Common PAG Points of Agreement? On the reports: Common executive summary. Common table with nominal mission parameters. On large missions: All three PAGs support the study of the four nominated missions. No other new large missions are advocated for study. Broad support for NASA attention to probe-class missions. PAG findings are based on community input subject to boundary conditions imposed by the PAG charge given by Paul Hertz: NASA is implementing the priorities of the 2010 Decadal Survey Additional possible points of agreement that require further discussion: - Concern that planned US participation in (large) ESA gravitational wave mission must be properly monitored, supported and presented to 2020 Decadal Survey. - Structure of STDTs must be carefully considered to avoid fracture within the community