Exoplanet Characterization by Proxy for Kepler-61B How a Nearby Star Bumped a Planet out of the Habitable Zone!

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Exoplanet Characterization by Proxy for Kepler-61b How a Nearby Star Bumped a Planet Out of the Habitable Zone! Sarah Ballard" University of Washington! Sagan Symposium, 9 November 2012! Outline" Validation: without radial velocities, when do we call a planet a planet? ! Characterization: measuring! the temperatures and radii of the Kepler planets orbiting the coolest stars! ! Kepler-61: an ideal! test bed! ! ! ! Spitzer" Kepler" Earth" Ruling Out False Positives with Color Dependence" Transiting planet" Target star! Achromatic" Ruling Out False Positives with Color Dependence" Eclipsing binary (Star + Star or )" Planet Target star! Color-dependent" Introduction to KOI 1361.01" KOI 1361" ! Ballard+ (2012, submitted)" KOI 1361.01: A super-Earth candidate (2.0 REarth) in a 59.8 day period ! around a 15th Kepler magnitude star! ! From published near-IR spectra (Muirhead et al. 2011): ! +66! Teff=3929-135 ! K , [Fe/H]=-0.02+/-0.11 dex! Spitzer Observations of KOI 1361.01" Gathered on 17 September 2011" (Part of 600-hour Warm Spitzer Campaign) " Ballard+ (2012, submitted)" 2 +482 ! Spitzer depth (Rp/R★) = 990 -387 ! ppm ! +73 ! Kepler depth : 1403 -65 ! ppm! A cache of cool, potentially rocky planets! transiting M dwarfs" Figure from Howard+ (2012)" A cache of cool, potentially rocky planets! transiting M dwarfs" All public KOIs (Borucki+ 2011, Batalha+ 2012) orbiting stars cooler than 4100 K" Stellar Characterization of M Dwarf KOIs" Muirhead+ 2012 4200 Mann+ 2012 Johnson+ 2012 4000 3800 3600 KIC Temperature (K) 3400 3500 3867 4233 4600 3200 Literature Temperature (K) 3161 3473 3785 4098 4410 4723 Revised Temperature (K) Figure from Dressing+ (in prep)" Stellar characterization: Bootstrapping from a nearby standard" Nearby standards KOI planet host Kepler Proxy Stars in Our Backyard?" As of a couple months ago, 75% of the stars in the solar neighborhood are M dwarfs Image: Riedel, Henry, & RECONS group Stellar characterization: Bootstrapping from a nearby standard" Stellar models from Dartmouth group (DoIer et al. 2008) HD 88230, direct measurement! (van Belle & von Braun 2009)! HD 88230, <direct measurement>! (Boyajian+ 2012)! KOI 1361, NIR spectrum ! (Muirhead+ 2012)! Ballard+ (2012, submitted)" A cache of cool, potentially rocky planets transiting M dwarfs" Ballard+ (2012, submitted)" Composition of Kepler-61b?" Doesn’t transit aer all! (Dragomir+ 2012) Looking ahead! •" Extended Spitzer and Kepler missions! •" Ongoing program with Apache Point Observatory 3.5 m telescope DIS and TripleSpec to observe KOIs + nearby standards ! !.

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