Abstract
After landing in the Utopia Planitia,Tianwen-1 formed the deepest landing crater on Mars,approximately 40 cm deep,exposing precious information about the mechanical properties of Martian soil.We estab-lished numerical models for the plume-surface interaction(PSI)and the crater formation based on Computational Fluid Dynamics(CFD)methods and the erosion model modified from Roberts'Theory.Comparative studies of cases were conducted with different nozzle heights and soil mechanical proper-ties.The increase in cohesion and internal friction angle leads to a decrease in erosion rate and maximum crater depth,with the cohesion having a greater impact.The influence of the nozzle height is not clear,as it interacts with the position of the Shock Diamond to jointly control the erosion process.Furthermore,we categorized the evolution of landing craters into the dispersive and the concentrated erosion modes based on the morphological characteristics.Finally,we estimated the upper limits of the Martian soil's mechanical properties near Tianwen-1 landing site,with the cohesion ranging from 2612 to 2042 Pa and internal friction angle from 25°to 41°.
基金项目
Key Research Program of the Institute of Geology and Geophysics,CAS(IGGCAS-202102)
Key Research Program of the Institute of Geology and Geophysics,CAS(IGGCAS-201904)
National Natural Science Foundation of China(42230111)
CAS Key Technology Talent Program()
维普
万方数据