V33E:
Using Experimental Petrology to Place Geochemical, Mineralogical, and Petrological Constraints on Planetary Bodies II Posters

Submit an Abstract to this Session



Session ID#: 26894

Session Description:
Understanding the geochemistry, mineralogy, and petrology across the rocky planetary bodies in our Solar System is imperative to discerning the thermal and magmatic evolution of these rocky planetary bodies including Mercury, Venus, Earth, the Moon, and Mars as well as asteroid belt objects. The aim of this session is to bring together expertise from the various avenues of experimental petrology-centric research within the overarching field of planetary sciences in order to spark big picture and inter-disciplinary discussions. Therefore, we encourage submissions from all areas of experimental studies including surface conditions (1-bar), lower pressure/temperature conditions, and higher pressure/temperature conditions. We particularly welcome contributions which showcase new results/hypotheses/models that help to address the (1) accretion and differentiation of rocky planetary bodies, (2) thermal and magmatic evolution of rocky planetary bodies as well as secondary volcanic processes, and (3) surficial and/or resurfacing processes or rocky objects in our Solar System.
Primary Convener:  Kathleen E Vander Kaaden, NASA Headquarters, Washington, United States
Conveners:  Catherine A. Macris, Indiana University Indianapolis, Department of Earth and Environmental Sciences, Indianapolis, United States and Nicole Lunning, Rutgers University, Piscataway, United States
Chairs:  Catherine A. Macris, California Institute of Technology, Pasadena, United States and Kathleen E Vander Kaaden, Jacobs Technology, NASA Johnson Space Center, Houston, TX, United States
OSPA Liaison:  Catherine A. Macris, California Institute of Technology, Pasadena, United States

Cross-Listed:
  • DI - Study of the Earth's Deep Interior
  • EP - Earth and Planetary Surface Processes
  • MR - Mineral and Rock Physics
  • P - Planetary Sciences
Index Terms:

1060 Planetary geochemistry [GEOCHEMISTRY]
3630 Experimental mineralogy and petrology [MINERALOGY AND PETROLOGY]
5480 Volcanism [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
6299 General or miscellaneous [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

Exploring the Utilization of Low-Pressure, Piston-Cylinder Experiments to Determine the Bulk Compositions of Finite, Precious Materials (234821)
Kathleen E Vander Kaaden1, Francis McCubbin2 and Andrea Harrington2, (1)Jacobs Technology, NASA Johnson Space Center, Houston, TX, United States, (2)NASA Johnson Space Center, Houston, TX, United States
Assessing the Behavior of Typically Lithophile Elements Under Highly Reducing Conditions Relevant to the Planet Mercury (282916)
Richard Lee Rowland II1, Kathleen E Vander Kaaden2, Francis McCubbin3 and Lisa Renee Danielson1, (1)Jacobs Technology, NASA Johnson Space Center, Houston, TX, United States, (2)NASA Headquarters, Washington, United States, (3)NASA Johnson Space Center, Houston, TX, United States
A layer of neutrally buoyant olivine in the early stages of a deep lunar magma ocean and a possible consecutive overturn (271982)
Giuliano Krättli and Max W Schmidt, ETH Swiss Federal Institute of Technology Zurich, Zurich, Switzerland
Petrologic Modeling of Magmatic Evolution in The Elysium Volcanic Province (258370)
David Susko, 2Malin Space Science Systems, San Diego, United States, Suniti Karunatillake, Louisiana State University, Planetary Science Lab, Department of Geology & Geophysics, Baton Rouge, LA, United States and Don Hood, Baylor University, Geology and Geophysics, Waco, LA, United States
The Influence of Oxygen and Sulfur on Uranium Partitioning Into the Core (298017)
Robert Dean Moore Jr, James A Van Orman and Steven A. Hauck II, Case Western Reserve University, Cleveland, OH, United States
Recalescence during crystallization of stardust: Resolution of the amorphous interstellar medium paradox (226946)
Alan G Whittington, University of Texas at San Antonio, Heat And Mass Transfer & Experimental Rheology (HAMsTER) lab, Earth and Planetary Sciences, San Antonio, United States, Alexander Sehlke, NASA Ames Research Center, Moffett Field, CA, United States and Angela K Speck, University of Missouri Columbia, Physics & Astronomy, Columbia, MO, United States
The origin of pallasites. A combined experimental and numerical approach. (223170)
Giulio Francesco Damiano Solferino, Royal Holloway University of London, Egham, TW20, United Kingdom and Gregor Golabek, Universität Bayreuth, Bayerisches Geoinstitut, Bayreuth, Germany

See more of: Volcanology, Geochemistry and Petrology