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DTSTART:20070311T020000
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UID:91eab9a5-523f-48ce-b0da-3d80beb4f30f.227964@calendar.missouristate.edu
CREATED:20230424T195012Z
LAST-MODIFIED:20230424T195012Z
LOCATION:Roy Blunt Hall 345
SUMMARY:GGP Seminar: Micah Mayle - "Potential lithosphere and asthenospher
 e melt sources of early syn-rift magmatism: Insights from 1D geodynamic m
 odels"
DESCRIPTION:Micah Mayle is currently a PhD candidate at Colorado State Uni
 versity. He is an alumnus of Missouri State University - Geology\, BS\, 2
 014.\n\n\nThis presentation will talk about geochemical and isotopic sign
 atures of magmatism from many continental rifts such as the East African 
 Rift System\, the Rio Grand Rift\, and West Antarctic Rift System. All su
 ggest that potential sources of syn-rift magmatism vary with time. The ea
 rliest magmas erupted during nascent rifting and are likely produced by t
 he melting of fertile lithologies in the lithosphere or asthenosphere. La
 ter magmatism\, occurring in mature rifts\, are the result of less fertil
 e asthenosphere-derived melts. Potential fertile sources in the mantle (p
 yroxenite-\, eclogite-\, and amphibole-bearing source rocks\, as well as 
 wet Iherzolite) responsible for the geochemical signatures\, have been pr
 oposed to result from previous metasomatization\, magmatism\, or subducti
 on.\n\n\nWe test the viability of a multi-lithology model consisting of f
 ertile sources (pyroxenite\, eclogite\, or wet Iherzolite) in the ambient
  mantle (dry Ihersolite) using a new 1D (one-dimensional) geodynamic mode
 l. This model can be run with or without latent heat of melting and calcu
 lates the pressure-temperature conditions for an extending lithosphere an
 d vertically ascending underlying asthenosphere through time. Results sho
 w that if a multi-lithology mantel is rifted\, there will be a distinct p
 attern of magmatism. Latent heat absorbed during early syn-rift melting o
 f the most fusible lithologies may reduce the temperature in the upper ma
 ntle sufficiently to inhibit a later melting of less fertile components t
 hat might be present. Thus\, early syn-rift magmatism may delay\, inhibit
 \, or prevent later syn-rift melt production from fertile components in t
 he mantle. Rift models that do not consider the latent heat of melting ov
 erestimate mantle temperatures and thus melt. They also underestimate the
  amount of extension required before melting begins and before peak melt 
 production rates are achieved. \n\n\nMicah obtained his master's degree i
 n geophysics from Oklahoma State University in 2018. His current research
  utilizes 1D and 2D geodynamic models to better understand the sources an
 d effects of syn-rift magmatism. Micah enjoys hiking and exploring Colora
 do in his spare time.
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;Mi
 cah Mayle is currently a PhD candidate at Colorado State University. He i
 s an alumnus of Missouri State University - Geology\, BS\, 2014.&lt;/p&gt;\n&lt;p&gt;
 This presentation will talk about geochemical and isotopic signatures of 
 magmatism from many continental rifts such as the East African Rift Syste
 m\, the Rio Grand Rift\, and West Antarctic Rift System. All suggest that
  potential sources of syn-rift magmatism vary with time. The earliest mag
 mas erupted during nascent rifting and are likely produced by the melting
  of fertile lithologies in the lithosphere or asthenosphere. Later magmat
 ism\, occurring in mature rifts\, are the result of less fertile asthenos
 phere-derived melts. Potential fertile sources in the mantle (pyroxenite-
 \, eclogite-\, and amphibole-bearing source rocks\, as well as wet Iherzo
 lite) responsible for the geochemical signatures\, have been proposed to 
 result from previous metasomatization\, magmatism\, or subduction.&lt;/p&gt;\n&lt;
 p&gt;We test the viability of a multi-lithology model consisting of fertile 
 sources (pyroxenite\, eclogite\, or wet Iherzolite) in the ambient mantle
  (dry Ihersolite) using a new 1D (one-dimensional) geodynamic model. This
  model can be run with or without latent heat of melting and calculates t
 he pressure-temperature conditions for an extending lithosphere and verti
 cally ascending underlying asthenosphere through time. Results show that 
 if a multi-lithology mantel is rifted\, there will be a distinct pattern 
 of magmatism. Latent heat absorbed during early syn-rift melting of the m
 ost fusible lithologies may reduce the temperature in the upper mantle su
 fficiently to inhibit a later melting of less fertile components that mig
 ht be present. Thus\, early syn-rift magmatism may delay\, inhibit\, or p
 revent later syn-rift melt production from fertile components in the mant
 le. Rift models that do not consider the latent heat of melting overestim
 ate mantle temperatures and thus melt. They also underestimate the amount
  of extension required before melting begins and before peak melt product
 ion rates are achieved.&amp;nbsp\;&lt;/p&gt;\n&lt;p&gt;Micah obtained his master's degree
  in geophysics from Oklahoma State University in 2018. His current resear
 ch utilizes 1D and 2D geodynamic models to better understand the sources 
 and effects of syn-rift magmatism. Micah enjoys hiking and exploring Colo
 rado in his spare time.&lt;/p&gt;&lt;/body&gt;&lt;/html&gt;
DTSTART;TZID=America/Chicago:20230428T153000
DTEND;TZID=America/Chicago:20230428T163000
SEQUENCE:1
URL:http://www.geosciences.MissouriState.edu
CATEGORIES:Public,Alumni,Current Students,Faculty,Future Students
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