Colloquia Schedule Fall 2014
Colloquia are on Tuesdays (unless otherwise indicated) at 3:30 pm in RLM 15.216B
"Hot Chromospheres and Flares on Cool and Ultracool Dwarfs" Ohio State University host: Adam Kraus |
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"Let it Collide: An Epic Saga of Star Wars Planets, Planetesimals, and Super Planet Crashes" University of Texas at Austin host: Adam Kraus |
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"The Complex Interplay between Star Formation and Galaxy Evolution from z~0-6" Haverford College host: Steve Finkelstein |
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"Compact Galaxies and Super-Massive Black Holes" Max Planck Institute for Astronomy (MPIA), Heidelberg host: Karl Gebhardt |
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"The Architecture and Timing of Planetary Systems" University of Chicago host: TBD |
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"Who's Afraid of the Big Bad Supermassive Black Hole?" Pennsylvania State University host: Steve Finkelstein |
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"Puzzles in the Structure of Disk Galaxies" Queen's University, Kingston, Ontario, Canada host: Karl Gebhardt |
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"Galaxy Build-up in the First Gyr: Insights from ultra-deep HST and Spitzer Observations" Yale University host: Steve Finkelstein |
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"Forming Earths and Mercuries: Solids Less Volatile than Ice" Life requires a variety of chemicals and elements. The question of water, how it was delivered to Earth and how it would be delivered to exoplanets, has taken a central position. However, other chemicals and elements are also important. Earth is significantly (~80%) depleted in elements important for life like sodium and potassium, both much less volatile than water, but much more volatile than silicon, magnesium, or iron. I will show how part of the composition of rocky planets is set early during their formation process, when the solids are still in sub-cm dust grains. Thermal processing of these grains during accretion events will alter both their composition and geometries, promoting the rapid formation of planetesimals with compositions unexpected at their radial location. This can explain the Earth's puzzling depletion of moderately volatile elements. Relatedly, magnetically mediated interactions between small dust grains can explain why Mercury is extremely iron rich. Both processes should play major roles in exoplanet formation, with consequences for their composition and chemistry. American Museum of Natural History, New York host: Joel Green |
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"Shedding Lyman Alpha Light on Cosmological Reionization" Arizona State University host: Steve Finkelstein |
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"From Disks to Planets: Observational Insights" Rice University host: Adam Kraus |
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"The Giant Magellan Telescope Project: Science and Status" Giant Magellan Telescope (GMT) host: Taft Armandroff |
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"There's Government in Your Science" American Astronomical Society host: Jeff Silverman |
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DeVaucouleurs Medalist DeVaucouleurs Lecture: "The Growth of Supermassive Black Holes and Galaxy Evolution" Yale University dinner host: Shardha Jogee (Medal Awarded by Daniel Jaffe) |
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DeVaucouleurs Medalist Public Lecture: "Black Holes, Galaxies and the Evolution of the Universe: An Observer's View" Yale University dinner host: Daniel Jaffe |
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DeVaucouleurs Medalist UT CNS Women in Science Lecture: "Why So Few? The Dearth of Women in Science" Yale University dinner host: Dean Linda Hicke |
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"Brown Dwarfs as Exoplanet Analogs" Bucknell University, Lewisburg PA host: Adam Kraus |
Visitors to the Department of Astronomy can find detailed information and maps on our Visiting Austin Page.
Please report omissions/corrections to: G. Orris at argus@astro.as.utexas.edu.
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