[S-SS32_1AM1] Fault Rheology and Earthquake Dynamics

[SSS32-P01_PG] Re-evaluation of frictional heat recorded in the dark gouge of a megasplay fault at the Nankai Trough

3-min talk in an oral session

*Hirokazu MASUMOTO¹, Tetsuro HIRONO¹, Tsuyoshi ISHIKAWA², Jun KAMEDA³, Hikaru YABUTA¹, Hideki MUKOYOSHI⁴ (1.Department of Earth and Space Science, Graduate School of Science, Osaka University, 2.Kochi Institute for Core Sample Research, Japan Agency for Marine-Earth Science and Technology, 3.Graduate School of Science, Hokkaido University, 4.Faculty of Education and Integrated Arts and Sciences, Waseda University)

Keywords:NanTroSEIZE, Tonankai earthquake, fluid-rock interactions, trace elements, X-ray diffraction, infrared spectroscopy

Because a megasplay fault branching from the deep subduction boundary megathrust in the Nankai Trough is thought to be the source of large tsunamis associated with past Tonankai earthquakes, investigation of the heat signal due to frictional slip recorded in the fault is important for estimating the earthquake slip parameters. We performed X-ray diffraction and infrared spectroscopic analyses of a megasplay fault-rock sample and re-examined previously reported trace-element and isotope compositions, but observed no specific change related to high temperature (≥250 ℃). In addition, although a qualitative increase of the illite content in illite/smectite mixed-layer minerals within the slip-zone sample was previously reported, our kinetic evaluation of illitization, taking into consideration the coseismic temperature change due to frictional heating and heat conduction, revealed that the illitization reaction hardly progresses at temperatures under 250 ℃. Alternatively, we suggest that the illite content in mixed-layer minerals might increase progressively via a comminution–dissolution–recrystallization process during multiple past slips. Accurate assessment of the slip behavior of the megasplay fault could be efficiently obtained by drilling to penetrate the fault zone at a deeper depth of approximately 1.5 km, where records of high temperatures would be detectable.