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DTSTART:20070311T020000
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DTSTART:20071104T020000
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UID:675dc585-8915-42c3-aecd-e3fe781c583e.179485@calendar.missouristate.edu
CREATED:20170316T164040Z
LAST-MODIFIED:20170316T164040Z
LOCATION:Kemper Hall 0206
SUMMARY:Guest Seminar Speaker Peter Gao: Understanding Exoplanet Clouds an
 d Hazes using Solar System Analogs 
DESCRIPTION:Clouds and hazes are ubiquitous in the atmospheres of planets 
 in our Solar System\, and have now been found in exoplanet atmospheres as
  well. Clouds made up of rocks and metals\, and hazes comprised of hydroc
 arbon soots and sulfurs block the spectral signatures of key atmospheric 
 molecules.  This impacts their brightness when seen in reflected and emit
 ted light. In other words\, not only do clouds and hazes prevent us from 
 gaining knowledge of exoplanets' atmospheric composition\, but they also 
 strongly affect the way we interpret current and future direct imaging ob
 servations. Understanding exoplanet atmospheres requires that we also und
 erstand the behavior of these clouds and hazes. In his talk\, Dr. Gao wil
 l discuss current efforts in modeling clouds and hazes in exoplanet atmos
 pheres\, with a focus towards the application of cloud physics in determi
 ning possible exoplanet cloud/haze distributions. \n\n\nDr. Gao holds a P
 hD in Planetary Sciences from the California Institute of Technology\, wh
 ere he did his thesis on Clouds and Hazes in Planetary Atmospheres.  He e
 arned an MS in Planetary Sciences\, also from CalTech. Currently\, Peter 
 Gao is a NASA Postdoctoral Program Fellow at the NASA Ames Research Cente
 r at Moffett Field\, CA. Here\, he performs research on modelling clouds 
 and hazes on exoplanets and Brown Dwarfs\, with applications to ongoing a
 nd future missions and observing campaigns.
X-ALT-DESC;FMTTYPE=text/html:&lt;html&gt;&lt;head&gt;&lt;title&gt;&lt;/title&gt;&lt;/head&gt;&lt;body&gt;&lt;p cl
 ass="MsoNormal"&gt;&lt;span&gt;Clouds and hazes are ubiquitous in the atmospheres 
 of planets in our Solar System\, and have now been found in exoplanet atm
 ospheres as well. Clouds made up of&amp;nbsp\;rocks and&amp;nbsp\;metals\, and ha
 zes comprised of hydrocarbon soots and sulfurs block the spectral signatu
 res of key atmospheric molecules. &amp;nbsp\;This impacts&amp;nbsp\;their brightn
 ess when seen in reflected and emitted light. In other words\, not only d
 o clouds and hazes&amp;nbsp\;prevent us from gaining knowledge of exoplanets'
  atmospheric composition\, but they also strongly affect the way we inter
 pret current and future direct imaging observations. U&lt;span&gt;nderstanding 
 exoplanet atmospheres requires that we also understand the behavior of th
 ese clouds and hazes.&amp;nbsp\;&lt;/span&gt;&lt;/span&gt;&lt;span&gt;In his talk\, Dr. Gao wil
 l discuss current efforts in modeling clouds and hazes in exoplanet atmos
 pheres\, with a focus towards the application of cloud physics in determi
 ning possible exoplanet cloud/haze distributions.&amp;nbsp\;&lt;/span&gt;&lt;/p&gt;\n&lt;p c
 lass="MsoNormal"&gt;&lt;span&gt;Dr. Gao holds a PhD in Planetary Sciences from the
  California Institute of Technology\, where he did his thesis on Clouds a
 nd Hazes in Planetary Atmospheres.&amp;nbsp\; He earned an MS in Planetary Sc
 iences\, also from CalTech. Currently\, Peter Gao is a NASA Postdoctoral 
 Program Fellow at the NASA Ames Research Center at Moffett Field\, CA. He
 re\, he performs research on modelling clouds and hazes on exoplanets and
  Brown Dwarfs\, with applications to ongoing and future missions and obse
 rving campaigns.&lt;o:p&gt;&lt;/o:p&gt;&lt;/span&gt;&lt;/p&gt;&lt;/body&gt;&lt;/html&gt;
DTSTART;TZID=America/Chicago:20170323T160000
DTEND;TZID=America/Chicago:20170323T170000
SEQUENCE:0
URL:https://www.facebook.com/MSUPAMS2/
CATEGORIES:Public,Alumni,Current Students,Faculty,Staff
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