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DTSTART:20070311T020000
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UID:7d0e7963-6463-4c69-bb7d-acd256907c9f.219241@calendar.missouristate.edu
CREATED:20211216T224846Z
LAST-MODIFIED:20211216T224846Z
LOCATION:Roy Blunt Hall 002 Lecture Hall
SUMMARY:GGP Seminar: Dr. Arya Udry - "How do we form granite on Mars witho
 ut plate tectonics?"
DESCRIPTION:Dr. Arya Udry\, MSA distinguished lecturer and associate profe
 ssor\, UNLV\, Department of Geoscience. The abstract for today's presenta
 tion:\n\n\nFor a long time\, the Martian crust has been considered to be 
 solely basaltic. These past six years\, with the analyses of surface rock
 s and additional meteorites\, it was shown that the Martian crust is more
  lithologically diverse than previously thought: Evolved rocks (i.e.\, hi
 gh in silica)\, including granitic rocks\, have been observed on the Mart
 ian surface by the Curiosity\, Mars Science Laboratory rover. In this tal
 k\, I present how we can better constrain the conditions of formation of 
 martian evolved rocks including magmatic processes (e.g.\, assimilation a
 nd fractional crystallization)\, using thermodynamical modeling.\n\n\nDr.
  Udry bio:\n\n\nHer research program seeks to better constrain the interi
 or composition\, magmatic processes and general evolution of the planet M
 ars through meteorite and rover data analyses. Her martian studies includ
 e comprehensive petrological analyses of martian samples to mimic the sca
 le of terrestrial geological studies. She also analyzes martian rover dat
 a to understand the formation of rare martian rocks with felsic compositi
 ons. Udry is a participating scientist on the Mars 2020 mission.
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&gt;Dr
 . Arya Udry\, MSA distinguished lecturer and associate professor\, UNLV\,
  Department of Geoscience. The abstract for today's presentation:&lt;/p&gt;\n&lt;p
 &gt;For a long time\, the Martian crust has been considered to be solely bas
 altic. These past six years\, with the analyses of surface rocks and addi
 tional meteorites\, it was shown that the Martian crust is more lithologi
 cally diverse than previously thought: Evolved rocks (i.e.\, high in sili
 ca)\, including granitic rocks\, have been observed on the Martian surfac
 e by the &lt;em&gt;Curiosity\,&lt;/em&gt; Mars Science Laboratory rover. In this talk
 \, I present how we can better constrain the conditions of formation of m
 artian evolved rocks including magmatic processes (e.g.\, assimilation an
 d fractional crystallization)\, using thermodynamical modeling.&lt;/p&gt;\n&lt;p&gt;D
 r. Udry bio:&lt;/p&gt;\n&lt;p&gt;Her research program seeks to better constrain the i
 nterior composition\, magmatic processes and general evolution of the pla
 net Mars through meteorite and rover data analyses. Her martian studies i
 nclude comprehensive petrological analyses of martian samples to mimic th
 e scale of terrestrial geological studies. She also analyzes martian rove
 r data to understand the formation of rare martian rocks with felsic comp
 ositions.&amp;nbsp\;Udry is a participating scientist on the Mars 2020 missio
 n.&lt;/p&gt;\n&lt;p&gt;&lt;/p&gt;&lt;/body&gt;&lt;/html&gt;
DTSTART;TZID=America/Chicago:20220218T143000
DTEND;TZID=America/Chicago:20220218T153000
SEQUENCE:0
URL:http://www.geosciences.MissouriState.edu
CATEGORIES:Public,Current Students,Faculty,Future Students
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