Exploring the Universe: Synergies in the ESA Science Programme

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Exploring the Universe: Synergies in the ESA Science Programme Günther Hasinger, ESA Director of Science (D/SCI) 14 th Appleton Space Conference, RAL, 6.12.2018 Towards ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 1

BepiColombo Launch ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 2

ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 3 BepiColombo, Aeolus

ESA Solar System Missions Ice Giants? (e.g. M*) proba-3 Solar Coronograph smile Solar Wind Magnetosphere Ionosphere ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 4 Small Bodies? (e.g. MMX, F)

ESA Astrophysics Missions plato Exoplanets & stars xrism Formation of the elements Einstein probe Exploring the transient sky ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 5

ESA Missions of Opportunity Corot Exoplanets France Microscope Fundamental physics France Hinode Solar physics Japan Proba-2 Plasma physics TEC/Belgium Hitomi X-ray astronomy Japan ExoMars Planetary science HRE/Russia IRIS Solar physics NASA Proba-3 Solar physics TEC/Belgium XRISM X-ray astronomy Japan Einstein Probe X-ray astronomy China (June 18 SPC) MMX Planetary science Japan (November 18 SPC) extp X-ray Astronomy China LiteBIRD Cosmic Microwave Japan WFIRST NIR Astronomy NASA Taiji Gravitational Waves China HERA Asteroid deflection TEC/OPS/Safety L5 Space Weather OPS/TEC/Safety Lunar Gateway Planetary science HRE Einstein Probe MMX ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 6

Interstellar Visitor 1I Oumuamua is accelerating! Hubble observations show it is accelerating (by comet outgassing?) ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 7

Gaia Using the new trajectory, Gaia has just found four possible home stars for Oumuamua So far only a very small fraction of Gaia stars have all the necessary information. Looking forward to DR3 & DR4. But, every million years Oumuamua passes by several stars, thus hard to find its true home. ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 8

Gaia Exoplanet Studies Although exoplanets were not a primary topic foreseen for the Gaia mission, there are a substantial number of scientific Gaia publications referring to this field. Main results are about the properties of the host stars of exoplanets. More detailed distance determinations, in particular to the planets discovered by Kepler, came to the conclusion that the actual number of earth-like planets in the habitable zone around other stars is probably significantly smaller than originally estimated. ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 9

Trappist-1 and Proxima b system habitability HST transit spectroscopy has revealed that at least 4 of 7 the Trappist 1 planets are likely rocky. M-star habitable zone planets are subjected to X-ray and EUV radiation, limiting habitability. XMM-Newton has detected strong X-ray flares from Trappist-1, and shown that Proxima b receives 250x more X-ray radiation than Earth. Finally, the strong stellar magnetic field can induce currents which heat up the planets from inside. The surface may consist of liquid lava! ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 10

A frozen Super-Earth around Barnard s Star Gaia might be able to see the astrometric signal of this planet! I. Ribas et al., 2018, Nature ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 11

2019 CHEOPS / ESA, CH, et al. Bright future for ESA Exoplanet studies! 2026 PLATO / ESA 2021 ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 12 JWST / NASA, ESA, CSA 2028 ARIEL / ESA

ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 13

Exoplanets and the Solar System Formation Uranus/Neptune-size planets and Super-Earths are the most abundant classes of exoplanets. The only ground-truth we have on these types of objects thus far is from Voyager 2 flybys of Uranus (1986) and Neptune (1989). An exploration mission to our ice giants will play a critical role understanding our own planetary system and those beyond ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 14

Scientific Themes for a Mission to the Ice Giants INTERIORS ATMOSPHERES MAGNETOSPHERES MOONS RINGS ORIGINS From L2 and L3 Science Themes Meeting, Paris September 2013 C. Arridge 2013 ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 15

Multi-Messenger Quest for the first Black Holes Athena JWST JCMT Stray BH Euclid GRB GW: LIGO / LISA ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 16

Bringing sound to the cosmic movies Athena hot gas structures supermassive black holes LISA gravitational wave observation ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 17

Unique celestial opportunity to explore Ice Giants ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 18 Preparation of Cosmic Vision in the 2050 time frame

Intermediate Ministerial Meeting ESAC, 25.10.2018 Director General s proposal on A United Europe in Space 1. Resolution giving mandate to the Director General to establish appropriate relations between the European Space Agency and the European Union 2. Resolution providing strategic guidelines for the preparation of the Agency programmes and activities Approved unanimously at IMM18 ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 19

Strategic guidelines adopted at IMM18 Council recognizes the importance of the Agency s mandatory activities and underlines the objective to secure an adequate level of resources so that the scientific programme will continue to build on its remarkable success in past years while giving consideration to increasing the financial resources made available to it so as to allow it to conduct more science activities. ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 20

Level of Resources versus Member State GDP Evolution ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 21

17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 2020 Decadal Survey JWST HST? BepiColombo ExoMars Solar Orbiter CHEOPS JUICE Euclid at Mercury WFIRST? Plato GMT TMT 2030 Decadal Survey ARIEL & F1 at Jupiter Ice Giant Mission ATHENA Next Generation Observatory M5. & F2 LISA M7 Next Generation Observatory Next. Generation L Mission L4 ESA UNCLASSIFIED - For Official Use E_ELT Hasinger, Appleton Conference, RAL 6.12.2018 Slide 22 2040 Decadal Survey M8 & F3 M* Ice Giant Mission Uranus? Neptune? M9 47 48 49 Next. Generation L5 2050 Decadal Survey Cosmic Vision 2050 NASA Strategic ESA Large ESA Medium/F/S Groundbased

Towards Cosmic Vision 2050 Linda Tacconi Chris Arridge Plus Community Engagement Survey starting this year. Members of the ESA Advisory Structure will be involved in various roles. ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 23

Thank you very much! ESA UNCLASSIFIED - For Official Use Hasinger, Appleton Conference, RAL 6.12.2018 Slide 24