Session 13 Geochemistry
Lin Wang (BGI, U. Bayreuth), Zhaodong Liu, Sanae Koizumi, Tiziana Boffa Ballaran, Dan Frost, Taekohiko Hiraga & Tomoo Katsura
Aluminum components in bridgmanite coexisting with corundum and CF-phase with temperature
No video is available.
Francesca Miozzi (Dep. Earth Scien., U. Milan), Simone Tumiati, Patrizia Fumagalli, Jing Yang, Paolo Nimis, Dimitri A. Sverjenski & Stefano Poli
Application of the double capsule technique in multi anvil apparatuses for the synthesis of COH fluids in equilibrium with diamonds
Dongyuan Zhou (Earth & Environm. Scien., U. Michigan), Junjie Dong, Yanhan Si, Feng Zhu & Jie Li
Melting Curve of Potassium Chloride from in situ Ionic Conduction Measurements
Rajdeep Dasgupta (Earth, Environm. & Planet. Scien., Rice U.), Damanveer S. Grewal, Kyusei Tsuno, Gelu Costin
The Fate of Nitrogen during Accretion and Differentiation of Rocky Planets
Video unavailable
Kevin Righter (Astromat. Res. & Expl. Scien., NASA John. Space Center), Lisa Danielson and Rick Rowland
Multi-anvil experimentation applied to planetary differentiation
Rajdeep Dasgupta (Saturday, 09 October 2021)
Hi Dr. Sokol, yes in our model we assumed that the early planetesimals underwent complete metal-silicate differentiation owing to heating by 26Al decay. This is perhaps an end-member, but the support for this comes from iron meteorites, which suggest that the earliest formed protoplanets underwent metal-silicate differentiation.
Alex Sokol (Monday, 27 September 2021 07:22)
Thanks for the great presentation.
According to your model, nitrogen differentiation between the silicate mantle and the core was carried out already in the planetisimals. But did planetisimals have magma oceans?