V33A:
Chemical and Dynamical Constraints on the Formation and Evolution of the Terrestrial Planets II Posters


Session ID#: 10925

Session Description:
This session aims to bring together researchers studying the rates and processes that governed planetary accretion and differentiation. Such processes and timescales are still hotly debated. For example, how did chemical reservoirs evolve within the protoplanetary disk? What was the chemical composition of the material that accreted onto different bodies in the inner solar system? What was the nature and timing of volatile element depletion and addition to planets? What were the timescales planetary differentiation on Earth and other planets and planetesimals?

Topics of interest include efforts to determine the ages of early Solar System objects, the timing and sequence of volatile element depletion and addition to planets, as well as the chemical fingerprints left behind by crust, mantle, and core formation. We invite researchers that investigate these topics with both chemical and isotopic analysis of Earth and extraterrestrial materials as well as dynamical simulations of planetary formation processes.

Primary Convener:  Sune Nielsen, Woods Hole Oceanographic Institution, Department of Geology and Geophysics, Woods Hole, United States
Conveners:  Paul S Savage, University of Durham, Durham, United Kingdom, Maud Boyet, Laboratoire Magmas et Volcans, Clermont-Ferrand Cedex, France and Audrey Bouvier, University of Western Ontario, Earth Sciences, London, ON, Canada
Chairs:  Maud Boyet, CNRS, Clermont-Ferrand, France and Paul S Savage, Washington University, St. Louis, MO, United States
OSPA Liaison:  Sune Nielsen, Woods Hole Oceanographic Institute, Geology & Geophysics, Woods Hole, United States

Cross-Listed:
  • P - Planetary Sciences
Co-Sponsor(s):
  • EGU-GMPV: European Geosciences Union – Geochemistry, Mineralogy, Petrology, and Volcanology - European Geosciences Union – Geochemistry, Mineralogy, Petrology, and Volcanology
  • GS: Geochemical Society - Geochemical Society
  • MSA: Mineralogical Society of America - Mineralogical Society of America
Index Terms:

1027 Composition of the planets [GEOCHEMISTRY]
1060 Planetary geochemistry [GEOCHEMISTRY]
1160 Planetary and lunar geochronology [GEOCHRONOLOGY]
3672 Planetary mineralogy and petrology [MINERALOGY AND PETROLOGY]

Abstracts Submitted to this Session:

Testing Models for the Origin of the Earth-Moon System with 142Nd/144Nd Measurements (82135)
Eugenia Hyung1, Stein B Jacobsen1 and Li Zeng2, (1)Harvard University, Earth and Planetary Sciences, Cambridge, MA, United States, (2)Harvard University, Cambridge, MA, United States
A Partial Late Veneer for the Source of 3.8 Ga Isua Rocks: Evidence from Highly Siderophile Elements and 182W (61792)
Christopher Dale1, Thomas Kruijer2, Kevin W Burton1, Thorsten Kleine3 and Stephen Moorbath4, (1)Durham University, Durham, United Kingdom, (2)University of Münster, Münster, Germany, (3)University of Münster, Institut für Planetologie, Münster, Germany, (4)University of Oxford, Oxford, United Kingdom
The Metal-Silicate Partitioning of Tungsten at Magma Ocean Conditions Using a Laser-Heated Diamond Anvil Cell (68617)
Neil Bennett1, Colin Jackson1, Yingwei Fei1, Emma Bullock2 and John T Armstrong3, (1)Carnegie Institution for Science Washington, Washington, DC, United States, (2)Carnegie Science, Earth and Planets Laboratory, Washington, United States, (3)Carnegie Institution for Science, Washington, DC, United States
Redistribution of Argon by Lower Mantle Phases During Magma Ocean Crystallization (75400)
Colin Jackson1, Neil Bennett2, Yingwei Fei2, Curtis D Williams3 and Sujoy Mukhopadhyay4, (1)Carnegie Institution for Science Washington, Washington, DC, United States, (2)Carnegie Institution for Science, Geophysical Laboratory, Washington, DC, United States, (3)University of California Davis, Department of Earth and Planetary Sciences, Davis, CA, United States, (4)Arizona State University, Department of Earth and Planetary Sciences, Tempe, AZ, United States
Iron isotope composition of depleted MORB (75646)
Jabrane Labidi, Corliss Kin I Sio and Anat Shahar, Carnegie Institution for Science Washington, Washington, DC, United States
Core formation in the early solar system through percolation: 4-D in-situ visualization of melt migration (77972)
Geoff Bromiley1, Madeleine Berg1, Yann Le Godec2, Nohamed Mezouar3, Robert C. Atwood4 and Julien Phillipe5, (1)University of Edinburgh, School of GeoSciences, Edinburgh, United Kingdom, (2)Sorbonne Université, IMPMC, Paris, France, (3)ESRF European Synchrotron Radiation Facility, Grenoble, France, (4)Diamond Light Source, Didcot, United Kingdom, (5)IMPMC Institut de Minéralogie et de Physique des Milieux Condensés, Paris Cedex 05, France
A Multiple Impact Hypothesis for Moon Formation: Target Spin and Disk Properties (60361)
Raluca Rufu and Oded Aharonson, Weizmann Institute of Science, Earth and Planetary Sciences, Rehovot, Israel
Contrasting Effects of Carbon and Sulfur on Fe-Isotope Fractionation between Metal and Silicate Melt during Planetary Core Formation (79019)
Stephen M Elardo and Anat Shahar, Carnegie Institution for Science Washington, Washington, DC, United States
Early onset of magma ocean crystallization revealed by coupled 146,147Sm-142,143Nd systematics of Nulliak ultramafics (3.78 Ga, Labrador) (79587)
Précillia Morino1,2, Guillaume Caro2,3 and Laurie C. Reisberg1,2, (1)CRPG CNRS, Vandeuvre les Nancy, France, (2)CRPG Centre de Recherches Pétrographiques et Géochimiques, Vandoeuvre-Les-Nancy, France, (3)CNRS, Paris Cedex 16, France
Metal-Silicate Partitioning of Various Siderophile Elements at High Pressure and High Temperatures: a Diamond Anvil Cell Study (79699)
Ingrid Blanchard, Institut de Physique du Globe de Paris, Paris, France, James Badro, Institut de Physique du Globe de Paris, Université Paris Cité, Paris, France and Julien Siebert, Université de Paris & Institut de Physique du Globe de Paris, Paris, France
Origin of Hadean 146Sm-142Nd signatures in supracrustal enclaves of the Innuksuac complex (Quebec) (79904)
Guillaume Caro1, Précillia Morino1, Stephen J Mojzsis2, Nicole Cates3 and Wouter Bleeker4, (1)CNRS, Paris Cedex 16, France, (2)University of Colorado & Universite Lyon 1, Boulder, United States, (3)University of Colorado & Universite Lyon 1, Boulder, CO, United States, (4)Geological Survey of Canada, Ottawa, ON, Canada
Ophiolitic Chromitites from the Andriamena Greenstone Belt, Madagascar: Possible Evidence for mid-Archean Plate Tectonics (80743)
Laurie C. Reisberg1, Maryse Ohnenstetter2, Catherine Zimmermann1, Anick Ratefiarimino3 and Dan Levy1, (1)CRPG CNRS, Vandeuvre les Nancy, France, (2)GeoRessources, UMR 7359, Vandoeuvre-les-Nancy, France, (3)Université d'Antananarivo, Ecole Supérieure Polytechnique, Antananarivo, Madagascar
Hysteresis in melt network topology allows core formation by porous flow (67526)
Marc A Hesse1, Soheil Ghanbarzadeh1 and Masa Prodanovic2, (1)The University of Texas at Austin, Jackson School of Geosciences, Austin, United States, (2)University of Texas at Austin, Austin, TX, United States
Solubility and Partitioning of Carbon and Sulfur in Fe-rich Alloy and Silicate Melt Systems at High Pressures and Temperatures: Implications for Earth’s Heterogeneous Accretion (82430)
Yuan Li, Guangzhou Institute of Geochemistry, CAS, Guangzhou, China, Rajdeep Dasgupta, Rice University, Department of Earth, Environmental and Planetary Sciences, Houston, TX, United States, Kyusei Tsuno, Arizona State University, Eyring Materials Center, Tempe, AZ, United States, Brian Monteleone, Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, United States and Nobu Shimizu, WHOI, Department of Geology and Geophysics, Woods Hole, MA, United States

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