DI51A:
From Core to Crust, the Evolution of Planetary Interiors I Posters

Friday, 19 December 2014: 8:00 AM-12:20 PM
Chairs:  Matt B Weller, Rice University, Houston, TX, United States and Julie C Castillo, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
Primary Conveners:  Matt B Weller, Rice University, Houston, TX, United States
Co-conveners:  Julie C Castillo, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Doris Breuer, Deutsches Zent Luft-Raumfahrt, Berlin, Germany and Nicolas Dauphas, University of Chicago, Chicago, IL, United States
OSPA Liaisons:  Nicolas Dauphas, University of Chicago, Chicago, IL, United States

Abstracts Submitted to this Session:

 
The influence of carbon, sulfur, and silicon on trace element partitioning in iron alloys
Jian Han, Case Western Reserve University, Cleveland, OH, United States, James A Van Orman, Case Western Reserve Univ, Cleveland, OH, United States, Katherine L Crispin, Geophysical Laboratory, Washington, DC, United States and Richard D Ash, University of Maryland, College Park, MD, United States
 
Fractionation of a Basal Magma Ocean
Matthieu Laneuville, Earth-Life Science Institute, Meguro-ku, Tokyo, Japan, John W Hernlund, Earth-Life Science Institute, Meguro, Japan and Stephane Labrosse, Ecole Normale Supérieure Lyon, Lyon, France
 
A High Core Heat Flow Solution to Earth’s Thermal and Magnetic Paradoxes
Peter E Driscoll, University of Washington Seattle Campus, Seattle, WA, United States
 
Extending the core paradox posed by an early dynamo
John Anthony Tarduno1,2 and Rory Danielle Cottrell2, (1)University of Rochester, Department of Physics & Astronomy, Rochester, NY, United States, (2)University of Rochester, Department of Earth & Environmental Sciences, Rochester, NY, United States
 
Combining Mantle Convection Modeling With Gravity and Topography Spectra to Constrain the Dynamic Evolution of the Terrestrial Planets
Tobias Rolf1, Stephanie C. Werner1 and Bernhard M Steinberger1,2, (1)University of Oslo, Centre for Earth Evolution and Dynamics (CEED), Oslo, Norway, (2)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany
 
Can We Approximate Non-Newtonian Rheology to Model Mantle Convection?
Doris Breuer1, Ana-Catalina Plesa1,2, Christian Hüttig1 and Nicola Tosi1,3, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)University of Münster, Münster, Germany, (3)Technical University Berlin, Berlin, Germany
 
Numerical Modeling of Mantle Convection with Heat-pipe Melt Transport
Sebastian Prinz1,2, Nicola Tosi2,3, Ana-Catalina Plesa2,4 and Doris Breuer2, (1)Freiberg University of Mining and Technology, Freiberg, Germany, (2)German Aerospace Center DLR Berlin, Berlin, Germany, (3)Technical University Berlin, Berlin, Germany, (4)University of Münster, Münster, Germany
 
Parameterized Thermal Evolution of the Earth with Continental Growth
Julie Menard, Washington State University, Pullman, WA, United States and Catherine M Cooper, WSU, Pullman, WA, United States
 
Mars Thermal History: Core, Atmosphere, Mantle, Phobos and Surface (MaTH CAMPS)
June K Wicks1, Matt B Weller2, Nathan J Towles3, Christopher Thissen4, Nicholas R Knezek5, Stephanie Johnston6, Sutatcha Hongsresawat7, Megan S Duncan2, Benjamin A Black8, Nicholas C Schmerr6, Mark P Panning9, Laurent Montesi10, Michael Manga11 and Philippe Henri Lognonne12, (1)Princeton University, Princeton, NJ, United States, (2)Rice University, Houston, TX, United States, (3)Johns Hopkins Univ, Baltimore, MD, United States, (4)Yale Univ-Geology & Geophysics, New Haven, CT, United States, (5)University of California, Berkeley, CA, United States, (6)University of Maryland College Park, College Park, MD, United States, (7)University of Florida, Gainesville, FL, United States, (8)University of California Berkeley, Berkeley, CA, United States, (9)Univ of FL-Geological Sciences, Gainesville, FL, United States, (10)University of Maryland, College Park, MD, United States, (11)Univ of California Berkeley, Berkeley, CA, United States, (12)Institut de Physique du Globe de Paris, Paris, France
 
Oscillatory Thermochemical Convection as a Cause for the Episodic Mare Basalt Volcanism in the PKT Region of the Moon
Chuan Qin and Shijie Zhong, University of Colorado at Boulder, Boulder, CO, United States
 
3D Spherical Convection Modeling of Venusian Resurfacing Mechanisms
Aaron C Prunty, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States and Scott D King, Virginia Tech, Blacksburg, VA, United States
 
Maximum-likelihood Estimation of Planetary Lithospheric Rigidity from Gravity and Topography
Kevin W Lewis1,2, Gabe L. Eggers1,3, Frederik J Simons1 and Sofia C Olhede4, (1)Princeton University, Princeton, NJ, United States, (2)Johns Hopkins University, Baltimore, MD, United States, (3)Georgia Institute of Technology Main Campus, Atlanta, GA, United States, (4)University College London, London, United Kingdom