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Abstracts
(2/21)
The Age of Exometeorology: Observing the Atmospheres of Transiting Exoplanets
-Seth Redfield, University of Texas at Austin
High signal-to-noise ratio (S/N) and high spectral resolution
observations of transiting exoplanets provide an opportunity to
measure the properties of exoplanet atmospheres and exospheres through
transmission spectroscopy. I present the results of a large-scale
program which led to the first ground-based detection of absorption
due to an exoplanetary atmosphere. Observations were taken with the
Hobby-Eberly Telescope (HET), which is well suited for this type of
program given its large mirror, high resolution spectrograph, and
queue scheduling. We observe significant additional absorption in the
cores of the neutral sodium doublet relative to the continuum, when
in-transit observations are compared to out-of-transit observations.
Two tests are performed to confirm the detection: (1) analysis of a
strong control line that is predicted to show no absorption, and (2)
an empirical Monte Carlo analysis to quantify the impact of systematic
errors. Physical properties of the exoplanet atmosphere, such as
atomic and molecular composition, cloud altitudes, and wind speeds may
be derived from the transmission spectrum. I will discuss the
richness of the acquired datasets and describe several complimentary
research projects. Observations of several other bright transiting
systems are ongoing with the HET, while future large telescopes will
push research toward observations of smaller atmospheres (e.g.,
terrestrial exoplanets), weaker spectral features (e.g., biomarkers),
and temporal variability (e.g., weather). A growing sample of
transiting exoplanets coupled with continued observational
achievements and capabilities are just beginning to make direct
comparisons of physical characteristics of exoplanet atmospheres
possible, eventually leading to comparative exometeorology.
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