U, Th, and K in planetary cores: Implications for volatile elements and heat production
Asmaa Boujibar1, Mya Habermann2,3, Kevin Righter4, Daniel Kent Ross5, Minako Righter6, Chidester Bethany7, Jennifer F Rapp8, Lisa Renee Danielson8, Kellye Pando9 and Rasmus Andreasen10, (1)NASA Johnson Space Center, Houston, TX, United States, (2)University of New Mexico Main Campus, Albuquerque, NM, United States, (3)Lunar and Planetary Institute, Houston, TX, United States, (4)NASA Johnson Space Center, Astromaterials Acquisition and Curation Office, Houston, United States, (5)UTEP, Jacobs Technology, NASA Johnson Space Center, Houston, TX, United States, (6)University of Houston, Houston, TX, United States, (7)University of Chicago, Chicago, United States, (8)Jacobs Technology, NASA Johnson Space Center, Houston, TX, United States, (9)Jacobs Technology, NASA Johnson Space Center, Houston, United States, (10)Aarhus University, Centre of Earth System Petrology, Department of Geoscience, Aarhus, Denmark
