1 Transiting Exoplanet Survey Satellite Daryl Swade Archive Team Meeting June 16, 2014.

Slides:



Advertisements
Similar presentations
A Search for Earth-size Planets Borucki – Page 1 KEPLER; Data Validation and Follow Up Observations CoRoT Symposium W.J. Borucki & the Kepler Team 5 February.
Advertisements

MAROON-X: An instrument for identifying another Earth
Destination: A Planet like Earth Caty Pilachowski IU Astronomy Mini-University, June 2011 Caty Pilachowski Mini-University 2011.
K2 Kepler’s Second Mission 1 K2 - a 2-wheel Kepler mission; The second highest peak in the world, a worthy ascent Steve B. Howell NASA Ames Research Center.
Exoplanet Atmospheres: Insights via the Hubble Space Telescope Nicolas Crouzet 1, Drake Deming 2, Peter R. McCullough 1 1 Space Telescope Science Institute.
Prospects for measuring η-Earth from RV David W. Latham Harvard-Smithsonian Center for Astrophysics 5 Octoberber 2013.
Exploring a Nearby Habitable World …. Orbiting an M-dwarf star Drake Deming NASA’s Goddard Space Flight Center.
SEARCHING FOR PLANETS IN THE HABITABLE ZONE. FROM COROT TO PLATO Ennio Poretti – INAF OAB.
Science Opportunities for HARPS-NEF David W. Latham PDR - 6 December 2007.
A Profusion of Exoplanets: Key Science Results from the Kepler Mission Jon M. Jenkins SETI Institute/NASA Ames Research Center Thursday September 22, 2011.
The Search for Earth-sized Planets Around Other Stars The Kepler Mission (2009)
Vulcan South - Extrasolar Planet Transit Search Doug Caldwell SETI Institute A search for transits of extrasolar planets Uses a wide-field (7 x 7 deg)
PLAnetary Transits and Oscillations of stars Thierry Appourchaux for the PLATO Consortium
Detection of Terrestrial Extra-Solar Planets via Gravitational Microlensing David Bennett University of Notre Dame.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
PLAnetary Transits and Oscillations of stars PLATO Consortium kick-off meeting.
Astro 101 Slide Set: Kepler’s Exoplanet Discoveries Exceed 1,000 0 Topic: Exoplanets Concepts: Transit Detection, Exoplanet Statistics Mission: Kepler.
The NASA/NExScI/IPAC Star and Exoplanet Database 14 May 2009 David R. Ciardi on behalf of the NStED Team.
Transiting Exoplanet Survey Satellite Daryl Swade September 24, 2014 TESS DMS Management Meeting.
Gaia, next frontier in Astronomy Jose Hernandez Gaia Data and Calibration Engineer European Space Astronomy Centre (ESAC) Madrid, Spain.
MASSACHUSETTS INSTITUTE OF TECHNOLOGY NASA GODDARD SPACE FLIGHT CENTER ORBITAL SCIENCES CORPORATION NASA AMES RESEARCH CENTER SPACE TELESCOPE SCIENCE INSTITUTE.
Transiting Exoplanet Survey Satellite Daryl Swade Archive Peer Review June 18, 2014.
Blayne Chang Aaron Fujioka Pd. 3. Exoplanets  “Extra-solar”  A planet that orbits a star other than our sun  Therefore is beyond the solar system with.
A Search for Earth-size Planets Borucki – Page 1 Roger Hunter (Ames Research Center) & Kepler Team March 26, 2010.
The Search for Extrasolar Planets Since it appears the conditions for planet formation are common, we’d like to know how many solar systems there are,
Toward Detections and Characterization of Habitable Transiting Exoplanets Norio Narita (NAOJ)
MAST Users Group – July 2009 MAST will provide the archive user interface for Kepler data, primarily light curves and target pixel data. ASB Staffing for.
Diversity of Data in the Search for Exoplanets Rachel Akeson NASA Exoplanet Science Institute California Institute of Technology.
Targets for JWST: Kepler and K2 Steve B. Howell NASA Ames Research Center March 2014.
PDS Geosciences Node Page 1 Archiving Mars Mission Data Sets with the Planetary Data System Report to MEPAG Edward A. Guinness Dept. of Earth and Planetary.
G. Ricker (MIT) George Ricker MIT Kavli Institute Transiting Exoplanet Survey Satellite David Latham SAO 30 May 2008.
1 Leonardo Pinheiro da Silva Corot-Brazil Workshop – October 31, 2004 Corot Instrument Characterization based on in-flight collected data Leonardo Pinheiro.
Travis Metcalfe (NCAR) Asteroseismology with the Kepler Mission We are the stars which sing, We sing with our light; We are the birds of fire, We fly over.
This dataset contains calibrated, to 4.8-micron spectral images of comet 103/P Hartley 2 acquired by the High Resolution Infrared Spectrometer (HRII)
Data Challenges in Astronomy: NASA’s Kepler Mission and the Search for Extrasolar Earths Jon M. Jenkins SETI Institute/NASA Ames Research Center Thursday.
Exoplanet Science Don Pollacco QUB. Overview PLATO’s objectives and space Work packages in the definition phase Timescales and aims of the definition.
Swift HUG April Swift data archive Lorella Angelini HEASARC.
Early science on exoplanets with Gaia A. Mora 1, L.M. Sarro 2, S. Els 3, R. Kohley 1 1 ESA-ESAC Gaia SOC. Madrid. Spain 2 UNED. Artificial Intelligence.
Lecture 34 ExoPlanets Astronomy 1143 – Spring 2014.
Steve B. Howell NOAO.  The Kepler mission consists of a 1- m telescope and CCD camera, designed to measure Earth-like transiting planets orbiting solar-
Kepler Finds Earth’s Cousin
Transiting Exoplanet Search and Characterization with Subaru's New Infrared Doppler Instrument (IRD) Norio Narita (NAOJ) On behalf of IRD Transit Group.
Transiting Exoplanet Survey Satellite May contain MIT, LL, GSFC, OSC proprietary information and be subject to U.S. Government Export Laws; U.S. recipient.
Exoplanet Characterization with JWST
Transiting Exoplanet Working Group Nikole K. Lewis STScI 10/20/2015.
The Role of Transiting Planets Dave Latham (CfA) 30 May 2008.
Transiting Exoplanet Survey Satellite December 8, 2014 TESS Kickoff.
KEPLER TABLE OF CONTENTS Table of Contents: Mission Overview Scientific Objectives Timeline Spacecraft Target Field of View Transit Method Johannes Kepler.
1 SUZAKU HUG 12-13April, 2006 Suzaku archive Lorella Angelini/HEASARC.
Introduction: Goals for JWST Transit Meeting C. Beichman Jonathan Lunine March 11, 2014.
The Search for Another Earth Exoplanets and the Kepler Spacecraft.
Astronomy 3040 Astrobiology Spring_2016 Day-7. Homework -1 Due Monday, Feb. 8 Chapter 2: 1, 3, 16 23, 24, 26 29, 30, , 54, 56 The appendices will.
Spitzer Space Telescope Mww-1 Warm Spitzer and Astrobiology Presented to NASA Astrobiology Institute Planetary System Formation Focus Group Michael Werner.
Kepler Finds Earth’s Cousin
The Kepler Mission S. R. Kulkarni.
Kepler/K2, TESS, and Opportunities for Australia
Exoplanets: Indirect Search Methods
Kepler Mission Alex Kang Exoplanet History Scientific Goals
Habitability Outside the Solar System
Single Object & Time Series Spectroscopy with JWST NIRCam
3677 Life in the Universe: Extra-solar planets
Pre-Cursor Data Needed for JWST Transit and Eclipse Observations
The Discovery In July 2015, NASA announced the discovery of the closest “cousin” to Earth yet discovered—in data collected by the Kepler spacecraft during.
NASA discovery (22th February 2017):
PHYS 2070 Tetyana Dyachyshyn
Strategies to detect Earth-like planets around nearby stars
SPHEREx LEGACY SCIENCE
Talking Points for Opener
Light Curves and Data Products from the Transiting Exoplanet
CHEOPS - CHaracterizing ExOPlanet Satellite
Presentation transcript:

1 Transiting Exoplanet Survey Satellite Daryl Swade Archive Team Meeting June 16, 2014

Agenda  Science goals  Mission concept  Organization  MAST 2

SCIENCE GOALS 3

TESS Science Goals and Drivers  Primary Goal: Discover Transiting Earths and Super- Earths Orbiting Bright, Nearby Stars  Rocky Planets & Water Worlds  Habitable Planets  Discover the “Best” ~1000 Small Exoplanets  “Best” Means “Readily Characterizable” Bright Host Stars Measurable Mass & Atmospheric Properties  Present: Only 2 small transiting exoplanets orbiting bright hosts are known  Large Area Surveys of Bright Stars  F, G, K dwarfs: +4 to +12 magnitude  M dwarfs known within ~60 parsecs  >200,000 target stars in two years 4

TESS Science Objectives 5  OBJECTIVE 1: Locate a diverse sample of transiting small exoplanets orbiting the brightest stars in the solar neighborhood.  OBJECTIVE 2: Locate a sample of transiting small exoplanets orbiting bright stars situated near the ecliptic poles, locations that are optimal for JWST follow-up.  OBJECTIVE 3: Establish the masses of a sample of TESS- located small transiting planets by means of precise radial velocity measurements.

TESS and Kepler Address Different Questions  TESS: Where are the nearest transiting rocky planets?  Kepler: How common are true Earth Analogs?  Solid angle coverage  Ω TESS ≃ 400 Ω Kepler  Number of accessible bright stars increased by same factor  Catalog star distances  TESS: ~10 2 light-yr  Kepler: ~10 3 light-yr  1/R 2 dependence means TESS stars are ~100x brighter than Kepler on average 6

Comparison of Host Star Brightness 7

Small Planets and Bright Stars 8

Predicted Science Yield from TESS Mission 9

TESS and the Habitable Zone 10

MISSION CONCEPT 11

TESS Wide FOV CCD Camera 12

TESS Prototype Focal Plane Assembly 13

Instrument Overview 14

Launch to Science Orbit Timeline 15

Operations Concept: Orbit 16

Operations Concept: Survey 17

ORGANIZATION 18

TESS Partnerships 19

TESS Project Organization 20

SOC 21

MAST 22

TESS Ground Segment Architecture 23

TESS Raw Data  Data types  Kepler: long cadence target – 150,000 targets, 32 pixels/target, 30 minutes cadence short cadence target – 300 targets, 85 pixels/target, 1 minute cadence full frame image – one per month  TESS: Target – targets/month, 100 pixels/target, 1 minute cadence Full Frame Image – 30 minute cadence  TESS raw data volume: 6600 GB/ year  Target data: 3500 GB/year  Full Frame Image data: 3100 GB/year  Kepler raw data volume: 380 GB/year  Long cadence: 293 GB/year  Short cadence: 84 GB/year  FFI: 2.3 GB/year 24

MAST Interfaces 25

TESS Archive Data Products from SPOC  Full Frame Image  Target Pixel Files  All pixels for a single target  Raw and calibrated values  Light Curves  Output of photometric analysis and cotrending  Collateral Pixel Files  Calibration data collected on-board  Ground calibration data  Cotrending Basis Vectors Systematic trends present in the ensemble of flux data for each CCD  Pixel Response Function Point spread function and pointing and electronic systematics  Flat Field Pixel response non-uniformity map 26

TESS Data Products from TSO  TESS Input Catalog (TIC)  Threshold Crossing Events (TCE) summary report  Identified from light curves  Data Validation (DV) results  Characterize and validate TCEs  TESS Objects of Interest (TOI) Catalog  Follow-up observations 27

Archive Operations  TESS monthly processing (Kepler quarterly)  Transferred from SPOC via hard drive  TESS archive data volume – 50 TB/year (to be refined)  Total Kepler archive data volume – 19 TB (Q0- Q17) Does not consider reprocessed data  No proprietary period on data  Availability depends primarily on SPOC processing time (<1 month)  Primary TESS web site hosted by MIT  Links to MAST web site 28

Archive Distribution Performance 29

Archive System Enhancements for TESS 30

Archive Development Effort 31 Phase B: April 1, 2014 – October 1, 2014 Phase C: October 2, 2014 – November 29, 2016 Phase D: November 30, 2016 – July 17, 2017

MAST Deliverables 32 DeliverableResponsibilityPhaseDate of Delivery TESS Archive Operations ConceptSystems EngineerBPDR TESS-Archive ICD SPOC-Archive TSO-Archive Systems EngineerB/CPDR/CDR Archive Catalog Design SpecificationSystems EngineerB/CPDR/CDR Archive ArchitectureSystems EngineerB/CPDR/CDR Archive Software DesignSystems EngineerCCDR TESS Archive User InterfaceSoftware EngineersC/DGS Test Archive Test ProceduresSystems EngineerDGS Test Archive Operations ProceduresArchive OperatorDLaunch TESS Archive User’s GuideArchive ScientistELaunch

TESS: A Bridge to the Future 33