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Lisa Esteves: Varying Phase Curves of Kepler Exoplanets: Evidence for Clouds and Winds

  • physicssocietyyu
  • Oct 23, 2014
  • 1 min read

All members are invited to join us in another exhilarating talk hosted by PSYU. We are excited to welcome Lisa Esteves, a PhD student in the Department of Astronomy and Astrophysics at the University of Toronto researching the atmospheres of extrasolar planets. The talk will be held in PSE 317 at 5.30PM. Food, drink, great talk, and good company are always guaranteed! This event and its benefits are free to all attending members. Memberships can be purchased at the start of the event. The abstract of the talk is below: "The Kepler mission's long-term monitoring of stars through high-precision photometry has not only revealed a plethora of exoplanet transits but also provided valuable data for characterizing a subset of these planets. Using over four years of Kepler observations, we have derived phase curves for over a dozen planets, and use these measurements to constrain their mass, brightness/temperature and energy redistribution between the day and the night sides. In our new study, we also investigate possible offsets of the peak brightness of the phase curve, which could be indicative of inhomogeneous clouds and/or substantial winds in the planet's atmosphere. We find significant offsets for over a half-dozen planets. With this growing sample of measured phase curves, we are able to better examine the trends of hot Jupiter energy budgets and albedos, and for the first time relate these properties to the presence of clouds or winds on a planet." - Lisa Esteves

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