Colloquia Schedule Fall 2013
Colloquia are on Tuesdays (unless otherwise indicated) at 3:30 pm in RLM 15.216B
See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker |
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See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker |
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See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker |
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See the handbills posted around the department for the details of the special colloquium that is being held today. Special Colloquium Speaker This presentation being held at 3:00 pm during the Cosmos Seminar time-slot. |
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"The Present and Future of Exoplanets with Precise Radial Velocities" Pennsylvania State University host: Adam Kraus |
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Frank N. Bash Symposium 2013: New Horizons in Astronomy: 6-8 October 2013. No Colloquium presentation scheduled on 8 October, to avoid conflict. |
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Tinsley Visiting Scholar/Planetary Group "Accessing the Atmospheres of Terrestrial Exoplanets" As our ability to detect smaller exoplanets continues to improve, it
becomes critical to develop techniques that are capable of measuring
the physical properties of the atmospheres of these planets. We have
had success in probing the atmospheres of giant exoplanets, but
atmospheres of terrestrial planets present a major challenge, not only
because of the reduction in size, but also because the physical
properties (and therefore the observational signatures) of terrestrial
planet atmospheres are dramatically different than those of giants.
Despite the difficulty, an elemental inventory of a terrestrial planet
atmospheres provides information about the planet's formation,
interior structure, geological evolution, and (as is the case for
Earth) biological evolution. While atmospheric characterization of a
true Earth analog is perhaps some time away, it is currently possible
to do so for exoplanets at the terrestrial planet boundary, the
so-called Super-Earths (M < 10 M-Earth). Currently, there are two
observational approaches for which the HET is particularly well suited
to make a significant impact and enable the achievement of important
milestones in the observations of terrestrial exoplanet atmospheres. I
will discuss the possibility of: (1) broadband observations of
Rayleigh scattering using multi-object or integral field
instruments. Rayleigh scattering is the dominant atmospheric signature
of terrestrial planets in the optical, and absolutely critical to
evaluating infrared observations. (2) high-resolution transmission
spectroscopy of H alpha which is sensitive to exoplanetary exospheres. The
expansive extent of a planetary exosphere can lead to much stronger
observational signature, and therefore makes such observations around
smaller exoplanets possible even if measurements of the bound
atmosphere are not. I will also discuss the prospects of future
observations of Super-Earth atmospheres from space using HST and/or
JWST. Wesleyan University host: Michael Endl |
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"Large-Scale Surveys of Star Formation in the Milky Way" University of Florida host: Neal Evans |
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"Supermassive Black Hole Binaries: The Search Continues" Georgia Institute of Technology host: Steve Finkelstein |
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"Observational Hallmarks of Evolution and Planet Formation in Circumstellar Disks" Harvard-Smithsonian Center for Astrophysics host: Neal Evans |
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"The Role of Large Herschel Surveys in the Fields of Galaxy Evolution and Cosmology" California Institute of Technology host: Karl Gebhardt |
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"Galaxy Evolution at High Redshifts: Lyman-alpha and Other Lines" Arizona State University host: Steve Finkelstein |
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"Revealing Cosmic Origins: from Exoplanet Atmospheres to the Intergalactic Medium with the HST Cosmic Origins Spectrograph" University of Texas at Austin host: Edward Robinson |
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"A CMB Perspective of the Epoch of Reionization" University of California, Berkeley host: Paul Shapiro |
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"Dark Matter in the Smallest Galaxies" Carnegie-Mellon University host: Andrew Mann |
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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