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NASA’s Exoplanet Explora1on Program (ExEP): Technology Selec1on, Priori1za1on, and Investment Dr. Brendan Crill, Deputy Program Chief Technologist Dr. Nicholas Siegler, Program Chief Technologist Exoplanet Explora1on Program Jet Propulsion Laboratory California Ins1tute of Technology 19 October 2017 Copyright 2017 California Institute of Technology. U.S. Government sponsorship acknowledged. Jet Propulsion Laboratory California Ins1tute of Technology Exoplanet Explora1on Program

NASA’s Exoplanet Explora1on Program (ExEP): Technology ... - ExEP...mission or mission concept funded to TRL 5 * funded to TRL 5 * for some mission architectures * for an exo-Earth

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Page 1: NASA’s Exoplanet Explora1on Program (ExEP): Technology ... - ExEP...mission or mission concept funded to TRL 5 * funded to TRL 5 * for some mission architectures * for an exo-Earth

NASA’sExoplanetExplora1onProgram(ExEP):

TechnologySelec1on,Priori1za1on,andInvestment

Dr.BrendanCrill,DeputyProgramChiefTechnologistDr.NicholasSiegler,ProgramChiefTechnologist

ExoplanetExplora1onProgram

JetPropulsionLaboratoryCaliforniaIns1tuteofTechnology

19October2017

Copyright 2017 California Institute of Technology. U.S. Government sponsorship acknowledged.

JetPropulsionLaboratoryCaliforniaIns1tuteofTechnology

ExoplanetExplora1onProgram

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Exoplanet Exploration Program Outline

Request: The APAC requests a joint presentation from the three program Chief Technologists that addresses the strategic technology gaps in each subject area, the progress that is being made to close these gaps, and the chief impediments to closing these gaps in a timely manner.

Outline: •  Overview of the Exoplanet Exploration Program’s

Technology Selection and Prioritization Process •  Investments in ExEP Technologies

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Exoplanet Exploration Program ExEP’s Technology Focus

•  The driving ExEP science goals are to: 1.  Discover planets around other stars 2.  Characterize their properties 3.  Identify candidates that could harbor life

•  As recommended in the 2010 Astrophysics Decadal Survey and planned in NASA’s Astrophysics Implementation Plan, the ExEP develops technologies that will enable the direct imaging and characterization of exoplanets in the habitable zone of Sun-like stars.

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Exoplanet Exploration Program

ExEP Technology Selection and Prioritization Process

4

ExEP Technology List

New technology recommendations from exoplanet community

Reviewed by (1) APD Program

Offices and (2) Exo-TAC

No, but could still benefit exoplanet science

Yes

Watch List Accepted and Prioritized:

(Impact, Urgency, and Trend)

Reviewed by Exo-TAC

No Not

accepted

Technologies carried over from

previous year

Tech Plan Appendix

Informs SAT/TDEM Call

Selection Criteria: Enables or enhances direct detection and/or

characterization of exoplanets?

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Exoplanet Exploration Program Program Offices Coordination

•  COR/PCOS/ExE Program technologists coordinate during the prioritization cycle by reviewing each other’s work and sitting on peer review boards.

•  The three programs work together to determine which program is best suited to advance a particular technology –  For example, sometimes a technology submitted to COR is entirely

driven by exoplanet science needs, and passed to ExEP

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Exoplanet Exploration Program

Click to edit Master title style Starshade Technology Gaps Starlight Suppression

S-2: Starlight Suppression and Model Validation

S-1: Controlling Scattered Sunlight

S-5: Petal Positioning Accuracy and Opaque Structure

S-4: Petal Shape And Stability

Formation Flying

Deployment Accuracy and Shape Stability

S-3: Lateral Formation Sensing

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Exoplanet Exploration Program

Click to edit Master title style

CG-2: Coronagraph Demonstrations

and Modeling

Detection Sensitivity

Angular Resolution

Contrast

CG-3: Deformable mirrors

CG-4: Image post-processing

Contrast Stability

CG-5: Wavefront sensing and control

CG-1: Large monolith mirrors

CG-1: Segmented mirrors

CG-6: Segment phasing and rigid body sensing and control

CG-7: Telescope vibration sensing and control

V-NIR Coronagraph/Telescope Technology Gaps

Ultra-low noise visible (CG-8) and infrared (CG-9) detectors

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Exoplanet Exploration Program

Investments in ExEP Technologies (2017)

8

ID Technology

S-2 StarlightSuppressionandModelValida9on

S-1 ControlEdge-Sca>eredSunlight

S-3 LateralForma9onFlyingSensingS-4 PetalShape

S-5 StarshadeDeploymentandShapeStability

CG-1 LargeApertureMirrors

CG-2 CoronagraphArchitecture

CG-6 MirrorFigure/SegmentPhasing,SensingandControl

CG-7 TelescopeVibra9onControl

CG-9 NIRUltra-LowNoiseDetector

CG-3 WavefrontSensingandControl

CG-5 DeformableMirrors

CG-8 VisibleUltra-LowNoiseDetector

M-1 ExtremePrecisionRadialVelocity

CG-4 Post-DataProcessing

CG-10 UV/NIR/Vismirrorcoa9ngs

CG-11 Mid-IRSpectralCoronagraph

CG-12 UVUltra-lownoisedetector

SAT / APRA

directed

mission or mission concept

funded to TRL 5 *

funded to TRL 5 * for some mission architectures

* for an exo-Earth imaging mission

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Exoplanet Exploration Program

Click to edit Master title style

Additional Slides

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Exoplanet Exploration Program

Technology Selection and Prioritization Process Schedule

10

ID Activity 2017

1 Technology needs input window opens June 1

email ExoPAG announce: Technology Gap Lists, input forms, process explanation

presentation at June ExoPAG

2 Technology window closes Aug 30

3 Technology Selection and Prioritization Criteria Review by APD Program Offices

Aug 30

4 Selection and Prioritization Criteria Review by ExoTAC Sep 15

5 Technology List Assessment Review by APD Program Offices Sep 30

6 Technology List Assessment Review by ExoTAC Oct 15

7 Technology Lists inform TDEM Amendment mid-Nov

8 Technology Amendment released through NSPIRES mid-Dec

9 ExEP Technology Plan Appendix updated and released Dec 15

Presentation at January ExoPAG Jan 15

10 TDEM Proposal Deadline Mar +1 yr

11 TDEM Awards Selected Aug +1 yr

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Exoplanet Exploration Program

ExEP’s Technology Prioritization Criteria

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Impact(weight:10)

4:Cri9caltechnology-requiredtomeetmissionconceptobjec9ves;withoutthistechnology,applicablemissionswouldnotlaunch3:Highlydesirable-notmission-cri9cal,butprovidesmajorbenefitsinenhancedsciencecapability,reducedcri9calresourcesneed,and/orreducedmissionrisks;withoutit,missionsmaylaunch,butscienceorimplementa9onwouldbecompromised

2:Desirable-notrequiredformissionsuccess,butofferssignificantscienceorimplementa9onbenefits;iftechnologyisavailable,wouldalmostcertainlybeimplementedinmissions

1:Minorscienceimpactorimplementa9onimprovements;iftechnologyisavailablewouldbeconsideredforimplementa9oninmissions

Urgency(weight:10)4:reducedriskneededformissionscurrentlyinpre-formula9onorformula9on.

3:In9mefortheDecadalSurvey(2019);notnecessarilyatsomeTRLbutreducedriskby2019. 2:Earliestprojectedlaunchdate<15yr(<2030) 1:Earliestprojectedlaunchdate>15yr(>2030)

Trend(weight:5)

4:(a)noongoingcurrentefforts,or(b)li>leornofundingallocated

3:(a)othersareworkingtowardsitbutli>leresultsortheirperformancegoalsareveryfarfromtheneed,(b)fundingunclear,or(c)9meframenotclear

2:(a)othersareworkingtowardsitwithencouragingresultsortheirperformancegoalswillfallshortfromtheneed,(b)fundingmaybeunclear,or(c)9meframenotclear

1:(a)othersareac9velyworkingtowardsitwithencouragingresultsortheirperformancegoalsareclosetoneed,(b)it'ssufficientlyfunded,and(c)9meframeclearandon9me

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•  HabExGaps:mirrorcoa9ngs,starshadestarlightsuppression,starshadecontrollingsca>eredsunlight,starshadelateralforma9onsensing,starshadepetalposi9onaccuracy,starshadepetalshapeandstability,telescopevibra.oncontrol,deformablemirrors,visibledetectors,largeapertureprimarymirror,wavefrontsensingandcontrol,coronagraphop*csandarchitecture

•  LUVOIRGaps:closed-loopsegmentphasing,vibra.onisola.on,wavefrontsensingandcontrol,mirrorsegments,high-contrastsegmented-aperturecoronagraphy,deformablemirrors,nearInfrareddetectors,visibledetectors,mirrorcoa9ngs

•  LynxGaps:high-resolu9onlightweightX-rayop9cs,non-deformingX-rayreflec9ngcoa9ngs,megapixelX-rayimagingdetectors,large-format,highresolu1onX-raydetectors,X-raygra9ngarrays

•  OSTGaps:far-IR(FIR)detectors,cryogenicreadoutsforlarge-formatFIRdetectors,warmreadoutelectronicsforlarge-formatFIRdetectors,sub-KCoolers,cryogenicFIRmirrorsegments(*)notethatOST’ssciencecaseisdevelopingandthedistribu9onofTRLsmayneedupda9ng

–  Green: technologies being advanced through SAT or directed development, –  Bold: technologies being advanced by WFIRST or ATHENA –  Italics: technologies being worked on through the STDT’s design studies

MissionConcept TRL2Gaps TRL3Gaps TRL4+Gaps Total#Gaps

GapsadvancedbySAT/directed

HabEx 0 6 6 12 12LUVOIR 1 4 4 9 7Lynx 1 3 1 5 4

OST(*) 1 1 3 5 2

Technology Needs of Decadal Survey Concept Studies

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Exoplanet Exploration Program

Investment Details in ExEP Technologies (2017)

13

S-2 StarlightSuppressionandModelValida9on

S-1 ControlEdge-Sca>eredSunlight

S-3 LateralForma9onFlyingSensingS-4 PetalShape

S-5 SSDeploymentandShapeStability

CG-1 LargeApertureMirrors

CG-2 CoronagraphArchitecture

CG-6 MirrorFigure/SegmentPhasing,Sensing&Control

CG-7 TelescopeVibra9onControl

CG-9 NIRUltra-LowNoiseDetector

CG-3 WavefrontSensingandControl

CG-5 DeformableMirrors

CG-8 VisibleUltra-LowNoiseDetector

M-1 ExtremePrecisionRadialVelocity

CG-4 Post-DataProcessing

CG-10 UV/NIR/Vismirrorcoa9ngs

CG-11 Mid-IRSpectralCoronagraph

CG-12 UVUltra-lownoisedetector

Starshade technology development activity

Starshade technology development activity

Starshade technology development activity, WFIRST

Starshade technology development activity

Starshade technology development activity

SAT awards; HabEx/LUVOIR work, APD plans a telescope systems-level study, pending adequate appropriation WFIRST. TDEM awards (Vortex,PIAACMC,HLC,polarization), ExEP’s High Contrast Imaging Testbed & Decadal Survey Testbed HabEx/LUVOIR work; part of systems-level study

HabEx/LUVOIR work ; part of systems-level study Solicited in SAT/TCOR-16, HabEx and LUVOIR are OK with SOA; APRA WFIRST, HabEx/LUVOIR work

WFIRST, TDEM

WFIRST

NN-EXPLORE; ADAP, ATP opportunities for data analysis / stellar jitter theory WFIRST SAT/TCOR awards, part of systems-level study

To be split: 1. mid-IR detectors (SAT/TCOR), 2. cryogenic DMs, and 3. coronagraph architecture SAT / TCOR awards

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Exoplanet Exploration Program 2017 Prioritized Technology List

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ID Technology Impact Urgency Trend Total

Weight: 10 10 5

S-2 StarlightSuppressionandModelValida9on 4 4 2 90

S-1 ControlEdge-Sca>eredSunlight 4 4 2 90

S-3 LateralForma9onFlyingSensing 4 4 2 90S-4 PetalShape 4 4 2 90

S-5 SSDeploymentandShapeStability 4 4 2 90

CG-1 LargeApertureMirrors 4 3 3 85

CG-2 CoronagraphArchitecture 4 3 3 85

CG-6 MirrorFigure/SegmentPhasing,Sensing&Control 4 3 3 85

CG-7 TelescopeVibra9onControl 4 3 3 85

CG-9 NIRUltra-LowNoiseDetector 4 3 3 85

CG-3 WavefrontSensingandControl 4 3 2 80

CG-5 DeformableMirrors 4 3 2 80

CG-8 VisibleUltra-LowNoiseDetector 4 3 2 80

M-1 ExtremePrecisionRadialVelocity 3 3 3 75

CG-4 Post-DataProcessing 4 2 2 70

CG-10 UV/NIR/Vismirrorcoa9ngs 3 3 2 70

CG-11 Mid-IRSpectralCoronagraph 2 3 3 65

CG-12 UVUltra-lownoisedetector 2 3 2 60

https://exoplanets.nasa.gov/exep/technology

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Exoplanet Exploration Program

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Exoplanet Exploration Program

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