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Present and Future Optical Space Missions: TESS & PLATO

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Present and Future Optical Space Missions: TESS & PLATO Present and future optical space missions: TESS & PLATO Angela^ R. G. Santos [email protected] Solar Focus { Solar-Stellar Connections: Present and Future Missions Boulder, May 8th, 2020 Previous missions CoRoT Angela^ Convection, Rotation et Transits Kepler & K2 Santos plan´etaires (CEA-France & ESA) (NASA) CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary Credits:ESA Credits:NASA 2/24 Angela^ Santos TESS & PLATO optical space missions TESS: Transiting Exoplanet Survey Satellite Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary Credits:MIT ∗ two-year all-sky survey ∗ main goal: discover hundreds of Earths & super-Earths ∗ bright stars in the solar neighborhood ∗ NASA's mission; PI: George R. Ricker (MIT) 3/24 Angela^ Santos TESS & PLATO optical space missions TESS Orbit Angela^ Santos CoRoT & Kepler TESS orbit observations science Porb ∼ 13.7 days extension Perigee: 17 REarth Apogee: 59 R PLATO Earth orbit observations science Summary Credits:NASA ∗ low radiation { prevent degradation ∗ facilitate data transfer { downlink every ∼ 13.7 days at perigee ∗ 2:1 resonance with the Moon's orbit ∗ inclined orbit { avoid eclipses by the Earth and Moon 4/24 Angela^ Santos TESS & PLATO optical space missions TESS Orbit AOP - Argument Of Perigee Angela^ GEO - Geosynchronous Earth Orbit Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary Ricker et al. (2014) ∗ Kozai cycles { three-body system: 10-month and 10-year cycles ∗ TESS orbital period varies between 12.8 to 14.6 days ∗ the orbit is stable on the time scale of decades or more 5/24 Angela^ Santos TESS & PLATO optical space missions TESS observations Angela^ Lund et al. (2017) Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary ∗ TESS band: 600-1000 nm ∗ interest in M dwarfs, which are cool and red 6/24 Angela^ Santos TESS & PLATO optical space missions TESS observations Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Ricker et al. (2015) Summary ∗ observation length from ∼ 27 days to ∼ 1 year ∗ 13 participially overlapping sectors ∗ 2-min cadence (main-sequence FGKM) ∗ Full Frame Images with cadence of 30 min 7/24 Angela^ Santos TESS & PLATO optical space missions TESS observations Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO Fausnaugh et al. (2018) orbit observations science Summary ∗ ∼ 1 day gaps during downlink (perigee) ∗ TESS momentum dump every 2.5 days (decrease in flux + modulation) ∗ times of large scatter in flux due \anomalously high pointing jitter" ∗ long-term systematics ∗ large pixels: photometric pollution 8/24 Angela^ Santos TESS & PLATO optical space missions Exoplanets with TESS Angela^ Barclay et al. (2018) Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary ∗ Expected exoplanet yield: more than 14,000 planets ∗ 280 planets smaller than 2REarth ∗ 500 planets around M dwarfs ∗ ground-based follow-up observations: masses and composition 9/24 Angela^ Santos TESS & PLATO optical space missions Exoplanets with TESS Angela^ Barclay et al. (2018) Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary ∗ Expected exoplanet yield: more than 14,000 planets ∗ 280 planets smaller than 2REarth ∗ 500 planets around M dwarfs ∗ ground-based follow-up observations: masses and composition 9/24 Angela^ Santos TESS & PLATO optical space missions Exoplanets with TESS Angela^ Santos Credits:NASA CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary 10/24 Angela^ Santos TESS & PLATO optical space missions Asteroseismology with TESS Schofield et al. (2019) Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary ∗ 2-min cadence from 2-yr TESS main-mission ∗ Expected p-mode detection for 5000 main-sequence and subgiant stars ∗ Asteroseismic Target List: 25,000 stars with p-mode detection probability > 5% 11/24 Angela^ Santos TESS & PLATO optical space missions Asteroseismology with TESS Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary Campante et al. (2016) ∗ 30-min cadence from 2-yr TESS main-mission ∗ expected p-mode detection for evolved planet hosts 12/24 Angela^ Santos TESS & PLATO optical space missions Asteroseismology with TESS Angela^ Santos Campante et al. (2019) CoRoT & Kepler HD 212771 TESS orbit observations science extension PLATO orbit observations science Summary 13/24 Angela^ Santos TESS & PLATO optical space missions Rotation and Activity with TESS Angela^ Santos Egeland et al. (in prep) Murphy et al. (in prep) 3.8 CoRoT & 4.0 Kepler 4.2 TESS K 4.4 H 0 R orbit g o l 4.6 observations science 4.8 extension 5.0 PLATO orbit 1.5 2.0 2.5 3.0 3.5 4.0 4.5 log Sph observations science Summary ∗ TESS targets are bright stars in the solar neighborhood (Kepler targets are typically faint) - Ground-based observations: independent constraints ∗ TESS main-mission provides short-term observations - inadequate for temporal variability (e.g. activity cyles) - biased Prot distribution; detection of the harmonics 14/24 Angela^ Santos TESS & PLATO optical space missions Rotation and Activity with TESS Angela^ Santos Egeland et al. (in prep) Murphy et al. (in prep) 3.8 CoRoT & 4.0 Kepler 4.2 TESS K 4.4 H 0 R orbit g o l 4.6 Santos observations et al. (2019) science 4.8 extension 5.0 PLATO orbit 1.5 2.0 2.5 3.0 3.5 4.0 4.5 log Sph observations science Summary ∗ TESS targets are bright stars in the solar neighborhood (Kepler targets are typically faint) - Ground-based observations: independent constraints ∗ TESS main-mission provides short-term observations - inadequate for temporal variability (e.g. activity cyles) - biased Prot distribution; detection of the harmonics 14/24 Angela^ Santos TESS & PLATO optical space missions Rotation and Activity with TESS Egeland et al. (in prep) Angela^ Santos Egeland et al. (in prep) 3.8 CoRoT & 4.0 Kepler 4.2 TESS K 4.4 H 0 R orbit g o l 4.6 observations science 4.8 extension 5.0 PLATO orbit 1.5 2.0 2.5 3.0 3.5 4.0 4.5 log Sph observations science Summary ∗ TESS targets are bright stars in the solar neighborhood (Kepler targets are typically faint) - Ground-based observations: independent constraints ∗ TESS main-mission provides short-term observations - inadequate for temporal variability (e.g. activity cyles) - biased Prot distribution; detection of the harmonics 14/24 Angela^ Santos TESS & PLATO optical space missions TESS publications Credits: NASA Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary 15/24 Angela^ Santos TESS & PLATO optical space missions TESS extension Angela^ Credits: NASA Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary ∗ NASA aproved 2-year extension ∗ short-cadence: from 1 min to 20 sec cadence ∗ FFI cadence: from 30 min to 10 min 16/24 Angela^ Santos TESS & PLATO optical space missions PLanetary Transits and Oscillations of stars Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary ∗ ultra-precision, long-term, continuous photometry ∗ main goal: Detect and characterize terrestrial exoplanets around bright solar-type stars ∗ under development; launch in 2026 ∗ ESA's mission; PI: DLR, Germany 17/24 Angela^ Santos TESS & PLATO optical space missions PLATO's orbit Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary Credits: ESA ∗ Lagrangian point L2 of the Sun-Earth system 18/24 Angela^ Santos TESS & PLATO optical space missions PLATO's observations first CCD { Credits: ESA Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary ∗ visible band with cadence of 25 seconds ∗ 26 cameras { largest digital combined camera flown in space ∗ extremely wide field of views: 2250 square degrees ∗ lifetime: 8.5 years (current plan for nominal mission: 4.5 years) 19/24 Angela^ Santos TESS & PLATO optical space missions PLATO's observations Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Summary Credits: ESA ∗ groups of cameras { point into different directions ∗ ultra-precision, long-term (up to 3-yr), continuous photometry ∗ short-term observations of different fields (2-3 months) 20/24 Angela^ Santos TESS & PLATO optical space missions PLATO's science Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations science Credits: ESA Summary ∗ bright stars in the solar neighborhood ∗ rocky planets (habitable zone), but also ice and giant planets ∗ ground-based follow-up observations: mass and composition ∗ understand the formation and evolution of planetary systems ∗ asteroseismology: probing stellar structure and evolution 21/24 Angela^ Santos TESS & PLATO optical space missions PLATO's science Angela^ Santos CoRoT & Kepler TESS orbit observations science extension PLATO orbit observations Credits: ESA science Summary ∗ planetary radii: ∼ 3% accuracy ∗ planetary masses (ground-based follow-up): ∼ 10% accuracy ∗ Asteroseismic stellar masses, radii, and ages: < 10% accuracy ∗ Identification of bright
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