Looking to the Future: the rest of the planets
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1 AGU Chapman Conference June 2013 Annapolis, MD Crossing Boundaries in Planetary Atmospheres Looking to the Future: the rest of the planets Heidi B. Hammel AURA, Washington, DC
2 Looking to the future of Models, Laboratory Measurements, Archives Atmospheres in our Solar System Exoplanet atmospheres: space- based telescopes Exoplanet atmospheres: ground- based telescopes But FIRST community assessment poll
3 Community Assessment of Exoplanet Characterizaion Parameters Aki Roberge, Kunio Sayanagi, EvereT Schlawin, Jacqueline Radigan, Heidi Hammel
4 Assess on two 5- level raxng systems Difficulty of DeterminaEon 5 = Possible for most planets 4 = Possible for some planets 3 = Possible for few planets 2 = Not against the laws of physics 1 = Warp drive TheoreEcal Importance 5 = Crucial 4 = Important 3 = Useful 2 = Nice to have 1 = Irrelevant ImplementaEon: google poll will be established stand by
5 Parameter Categories Orbital Stellar Basic Physical Parameters (mass, radius, bulk composixon) Surface ProperXes Interior ProperXes External Factors
6 Orbital Parameters semi- major axis eccentricity obliquity inclinaxon rotaxon rate
7 Stellar Parameters stellar spectrum stellar age stellar variability stellar winds stellar metallicity
8 Basic Planet Parameters mass / gravity radius bulk composixon
9 Surface ProperXes planet reflected spectrum planet thermal spectrum planet transmission spectrum Bond albedo surface ocean fracxon atmospheric composixon clouds vs. hazes Wind Speed
10 Interior ProperXes magnexc field plate tectonics volcanic acxvity interior heat flux Xdal heaxng interior density structure
11 External Factors impact rate impact history rings moons interplanetary dust
12 Assess on two 5- level raxng systems Difficulty of DeterminaEon 5 = Possible for most planets 4 = Possible for some planets 3 = Possible for few planets 2 = Not against the laws of physics 1 = Warp drive TheoreEcal Importance 5 = Crucial 4 = Important 3 = Useful 2 = Nice to have 1 = Irrelevant ImplementaEon: google poll will be established stand by
13 Models, Laboratory Measurements, Archives
14 Atmospheres in our solar system
15
16 Atmospheres in our solar system Start with the outer solar system (because I just happen to have this slide already handy) ((been showing it for the past decade, in fact))
17 Solar System Exploration: Giant Planets Past Present Future " " Voyager 2 Ice Gian Missio Voyager 2 Pioneer 11 Voyager 1 Voyager 2 Pioneer 10 Voyager 1 Pioneer 11 Voyager 2 Cassini Orbiter Galileo Orbiter & Probe Saturn Probe?! New Frontiers Juno" Cassini New Horizons Orbiter Juice" Orbiter? H. B. Hammel 6/26/2013!
18 exploring atmospheres in our solar system with spacecrae
19 Mars Atmosphere NOTIONAL 6/28/ US Flagship Mars2020 Trace Gas Orbiter ExoMars Rover US Discovery InSight more Mars? MAVEN India s Mars Orbiter Mission Current Mars Missions FuncXoning and/or selected Selected but some uncertainxes NoXonal or much uncertainty Ground- and space- based telescopic observaxons
20 Other SS Atmospheres NOTIONAL 6/28/ US Flagship Cassini Ice Gia US New FronXers Juno NH Pluto Venus Express Akatsuki JUICE Saturn Probe? Titan? Venus In Situ Explorer? FuncXoning and/or selected Selected but some uncertainxes NoXonal or much uncertainty US Discovery Venus? Titan? Ice Giant (using warp drive)? Ground- and space- based telescopic observaxons
21 exploring atmospheres of exoplanets with spacecrae
22 exoplanet atmospheres from space NOTIONAL 6/28/ Kepler RIP Hubble Spitzer GAIA astrometry TESS transit photom CHEOPS PLATO transit photom JWST ECHO transit spectros JWST WFIRST AFTA/NRO + C super- duper (UVOIR?) mega- telescope to characterize exo- earths with: coronograph? occulter? interferometry? TBD? EXCEDE disks FINESSE
23 exploring atmospheres of exoplanets with ground- based telescopes
24 exoplanet atmospheres from the ground NOTIONAL 6/28/ Precision Radial Velocity machines such as: HARPS (La Silla), HARPS- N (TNG), ESPRESSO (VLT), YOUR FAVE HERE Radial Velocity such as: SpEX (IRTF), FIRE (Magellan), NESSI (Magdalena Ridge), YOUR FAVE HERE Imaging and/or spectra on 5- to 10- m telescopes such as: GPI (Gemini), Spheres (VLT), Palm1640 (Palomar 5- m), HiCIAO (Subaru), YOUR FAVE HERE Transits: Next GeneraXon Transit Survey, NESSI (Magdalena Ridge)small- telescope transit observaxons; YOUR FAVE HERE super- duper extremely large telescopes (ELTs) with: E- ELT + EPICS (imaging)? GMT + SuperHARPS (RV)? TMT + IRIS (IFU = spectra)? OMG SO MUCH OTHER STUFF: microlensing, polarizaxon with PlanetPol, zodi and disks with ALMA and LBTI, YOUR FAVE HERE
25 Looking to the future for Solar System planets
26 Looking to the future for exoplanets, the future s so bright you gota wear shades
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