DI43A:
What Lies Beneath: Multidisciplinary Approaches to Probing the Structure and Evolution of Planetary Interiors I Posters


Session ID#: 10244

Session Description:
While surface observations of planetary bodies in our solar system are plentiful, and new planets orbiting other stars are being detected with increasing regularity, planetary interiors remain difficult to access.  In this session, we focus on innovative techniques from a variety of disciplines to increase our understanding of the structure and evolution of planetary interiors, ranging from the terrestrial planets in our solar system (including Earth) to icy satellites, gas giants, and exoplanets. Topics in this session will bring together contributions from, but not limited to laboratory work, recent planetary missions along with their geophysical and geochemical observations, numerical modeling, and proposed future planetary data in a joint effort to illuminate the deep interiors of planets.
Primary Convener:  Mark P Panning, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Conveners:  Justin Filiberto, Southern Illinois University Carbondale, Carbondale, IL, United States, Kanani K M Lee, Yale University, Department of Geology & Geophysics, New Haven, CT, United States and Nicola Tosi, Technical University Berlin, Berlin, Germany
Chairs:  Justin Filiberto, Southern Illinois University Carbondale, Carbondale, IL, United States and Nicola Tosi, Technical University Berlin, Berlin, Germany
OSPA Liaison:  Justin Filiberto, Southern Illinois University Carbondale, Carbondale, IL, United States

Cross-Listed:
  • P - Planetary Sciences
  • V - Volcanology, Geochemistry and Petrology
Index Terms:

1060 Planetary geochemistry [GEOCHEMISTRY]
5430 Interiors [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
5724 Interiors [PLANETARY SCIENCES: FLUID PLANETS]
6296 Extra-solar planets [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

How Many Exoplanets Does it Take to Constrain the Origin of Mercury? (86385)
Leslie Rogers, University of California Berkeley, Berkeley, CA, United States; University of Chicago, Astronomy and Astrophysics, Chicago, United States
Inside a Diamond Planet: Experimental Investigation of High P-T SiC (62007)
Kierstin Daviau1, Zhixue Du1 and Kanani K M Lee2, (1)Yale University, New Haven, CT, United States, (2)Yale University, Department of Geology & Geophysics, New Haven, CT, United States
Effect of Silicon Alloying on the Structure of Exoplanetary Cores (84796)
June K Wicks1, Ray Smith2, Federica Coppari2, Richard G Kraus2, Matthew Newman3 and Thomas S Duffy4, (1)Princeton University, Princeton, NJ, United States, (2)Lawrence Livermore National Laboratory, Livermore, CA, United States, (3)California Institute of Technology, Pasadena, CA, United States, (4)Princeton University, Department of Geosciences, Princeton, NJ, United States
Thermal Evolution and Crystallisation Regimes of the Martian Core (77090)
Christopher J Davies, Scripps Institution of Oceanography, La Jolla, CA, United States and Anne Pommier, Carnegie Institution for Science, Earth and Planets Laboratory, Washington, United States
Investigation of 3-D lateral variations on seismic waveform modeling, in preparation for the InSight mission to Mars (78439)
Melanie Drilleau1, Dubois Alizee2, Jean-Francois Blanchette-Guertin3, Taichi Kawamura4 and Philippe Henri Lognonné4, (1)Institut Supérieur de l'Aéronautique et de l'Espace, Toulouse Cedex 04, France, (2)French Alternative Energies and Atomic Energy Commission, Gif sur Yvette, France, (3)Institut de Physique du Globe de Paris, Paris, France, (4)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France
Simultaneous Determination of Structure and Event Location Using Body and Surface Wave Measurements at a Single Station: Preparation for Mars Data from the InSight Mission (73713)
Mark P Panning1, William Bruce Banerdt2, Éric Beucler3, Jean-Francois Blanchette-Guertin4, Maren Boese5, John F Clinton6, Melanie Drilleau7, Stephanie R. James8, Taichi Kawamura9, Amir - Khan III10, Philippe Henri Lognonné9, Antoine Mocquet3 and Martin van Driel11, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)University of Nantes, Nantes, France, (4)Institut de Physique du Globe de Paris, Paris, France, (5)ETH Zurich, Zurich, Switzerland, (6)ETH Zurich, Swiss Seismological Service, Zurich, Switzerland, (7)Institut Supérieur de l'Aéronautique et de l'Espace, Toulouse Cedex 04, France, (8)Univ Florida, Gainesville, FL, United States, (9)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, (10)ETH, Zurich, Switzerland, (11)ETH Zurich, Institute of Geophysics, Zurich, Switzerland
Imaging Mars: Seeking Characteristic Signals in Models of the Martian Interior (69059)
Jessica C E Irving, University of Bristol, School of Earth Sciences, Bristol, BS8, United Kingdom and June K Wicks, Princeton University, Princeton, NJ, United States
Formation Conditions of Basalts at Gale Crater, Mars from ChemCam Analyses (79807)
Justin Filiberto1, John Bridges2, Rajdeep Dasgupta3, Peter Edwards2, Susanne P Schwenzer4 and Roger C Wiens5, (1)Southern Illinois University Carbondale, Carbondale, IL, United States, (2)University of Leicester, Leicester, United Kingdom, (3)Rice University, Department of Earth, Environmental and Planetary Sciences, Houston, TX, United States, (4)Open University, AstrobiologyOU, Milton Keynes, United Kingdom, (5)Space Science and Applications, Los Alamos, United States
Ellipticity and crustal corrections for seismic body wave paths: application to Mars and Moon (72734)
Stefanie Hempel, Institut Supérieur de l'Aéronautique et de l'Espace, DEOS / SSPA, Toulouse Cedex 04, France, Raphael Garcia, Institut Supérieur de l'Aéronautique et de l'Espace, SSPA/DEOS, Toulouse Cedex 04, France and Mark A Wieczorek, Institut de Physique du Globe de Paris, Paris, France
Origin and Constraints on Ilmenite-rich Partial Melt in the Lunar Lower Mantle (77644)
Ananya Mallik1, Heidi Haviland2, Paul M Bremner3, Sanja Panovska4, Matthew R Diamond5, Simon James Lock6, Yasuhiro Nishikawa7, Hugo Jiménez-Pérez7, Anat Shahar8, Wendy R Panero9, Philippe Henri Lognonné10 and Ulrich Faul11, (1)Bayerisches Geoinstitut, Universitaet Bayreuth, Bayreuth, Germany, (2)University of California Berkeley, Berkeley, CA, United States, (3)University of Florida, Ft Walton Beach, FL, United States, (4)Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Section 2.3 – Geomagnetism, Potsdam, Germany, (5)California Institute of Technology, Pasadena, United States, (6)Harvard University, Cambridge, MA, United States, (7)Institut de Physique du Globe de Paris, Paris, France, (8)Carnegie Institution for Science Washington, Washington, DC, United States, (9)Ohio State University Main Campus, School of Earth Sciences, Columbus, OH, United States, (10)Université Paris Cité, Institut de physique du globe de Paris, CNRS, Paris, France, (11)Massachusetts Institute of Technology, Earth Atmospheric and Planetary Sciences, Cambridge, MA, United States
Effect of Iron Content on the High-Pressure Plasticity of Olivine (73864)
Paul Raterron, Université de Lille, UMET - CNRS, Villeneuve d'Ascq, France, Caleb W Holyoke III, University of Akron, Geology and Geophysics, Akron, OH, United States, Nadege Hilairet, CNRS and Univ. Lille, Lille, France and Sebastien Merkel, Univ. Lille, Lille, France

See more of: Study of Earth's Deep Interior