2026-08-06T13:33:15Z
https://icatplus.esrf.fr/oaipmh/request
oai:icatplus.esrf.fr:inv/2438147472
2026-07-20T06:00:38.577Z
4.2
EI
10.15151/ESRF-ES-2438147472
Maria Del Carmen SANCHEZ
Maria Del Carmen
Sanchez
Marisa WOOD
Marisa
Wood
Yining WU
Yining
Wu
MARTIN DEMOUCRON
Martin
Demoucron
Jean-Philippe PERRILLAT
Jean-Philippe
Perrillat
Yining WU
Yining
Wu
Marisa WOOD
Marisa
Wood
Kazi Ahnaf Abdullah SAAD
Kazi Ahnaf Abdullah
Saad
Maria Del Carmen SANCHEZ
Maria Del Carmen
Sanchez
Jean-Philippe PERRILLAT
Jean-Philippe
Perrillat
Max GERIN
Max
Gerin
Kazi Ahnaf Abdullah SAAD
Kazi Ahnaf Abdullah
Saad
Density of Titanium-rich Silicate Liquids: Implications for the Lunar Interior
Example Institute
2029
Data from large facility measurement
2026-07-16T06:00:00Z/2026-07-20T06:00:00Z
2026-07-20T06:00:00Z
I
CC-BY-4.0
The density of Ti-rich silicate liquids with respect to the lunar mantle determines their buoyancy within the lunar interior; however, the physical properties of such liquids are highly compositionally dependent due to the complex role of titanium within the melt structure. To address this, we will determine the density of Ti-rich silicate liquids using the X-ray absorption method (Beer-Lambert Law) at high pressure high temperature (PT) conditions up to 5 GPa, 2200 K, generated using the Paris-Edinburgh press. Furthermore, we will take X-ray diffraction for liquid structure analysis at select PT conditions which will be complemented by our ab initio molecular dynamics simulations.