Partial core vaporization during Giant Impacts inferred from the entropy and the critical point of iron

• Published in: Earth and planetary science letters 2020-10, Vol.547, p.116463, Article 116463
• Main Authors: Li, Zhi, Caracas, Razvan, Soubiran, François
• Format: Article
• Language: English
• Subjects: core vaporisation; critical point; Earth Sciences; entropy; Giant Impacts; iron; Planetology; Sciences of the Universe
• ISSN: 0012-821X; 1385-013X
• DOI: 10.1016/j.epsl.2020.116463

•The critical point of iron lies in 9000-9350 K temperature range, 1.85-2.40 g/cm3 density range, and 4-7 kbars pressure range.•The entropy gain during the giant impact was enough to partially vaporize Theia's core.•The core of late veneer impactors undergoes partial vaporization. Giant impacts are disruptive events occurring in the early stages of planetary evolution. They may result in the formation of a protolunar disk or of a synestia. A central planet and one or several moons condense upon cooling bearing the chemical signature of the silicate mantles of the initial bodies; the iron cores may partly vaporize, fragment and/or merge. Here we determine from ab initio simulations the critical point of iron in the temperature range of 9000-9350 K, and the density range of 1.85-2.40 g/cm3, corresponding to a pressure range of 4-7 kbars. This implies that the iron core of the proto-Earth may become supercritical after giant impacts and during the condensation and cooling of the protolunar disk. We show that the iron core of Theia partially vaporized during the Giant Impact. Part of this vapor may have remained in the disk, to eventually participate in the Moon's small core. Similarly, during the late veneer a large fraction of the planetesimals have their cores undergoing partial vaporization. This would help mixing the highly siderophile elements into magma ponds or oceans.