The Proceedings of the Eighth International Conference on Creationism (2018)
Seely et al. ◀ Finite element analysis of a near impact event ▶ 2018 ICC 65 materials. Journal of Engineering Materials and Technology 139, 011010-011010–10. Horstemeyer, M.F., J. Lathrop, A.M. Gokhale, and M. Dighe. 2000. Modeling stress state dependent damage evolution in a cast Al–Si–Mg aluminum alloy. Theoretical and Applied Fracture Mechanics 33:31– 47. Horstemeyer, M.F., and J.R. Baumgardner. 2003. What initiated the Flood cataclysm? In Proceedings of the Fifth International Conference on Creationism , ed. R.E. Walsh., pp. 155-163. Pittsburgh, Pennsylvania: Creation Science Fellowship Hyodo, R., S. Charnoz, K. Ohtsuki, and H. Genda. 2017. Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object. Icarus 282: 195-213. Karato, S. 2012. Deformation of Earth materials. Cambridge University Press. Kavner, A. 2007. Garnet yield strength at high pressures and implications for upper mantle and transition zone rheology. Journal of Geophysical Research: Solid Earth 112, B12207. Mazarico, E., M.K. Barker, G.A. Neumann, M.T. Zuber, and D.E. Smith. 2014. Detection of the lunar body tide by the Lunar Orbiter Laser Altimeter. Geophysical Research Letters 41, no. 7: 2282–2288. NASA/JPL. Mars topographic map. Mars Global Surveyor. Mars Orbital Laser Altimeter. Nesvorný, D. 2011. Young solar system’s fifth giant planet? The Astrophysical Journal Letters 742: L22. Oard, M.J. 2012. An impact Flood submodel—dealing with issues. Journal of Creation 26, no 2: 73-81. Pires, P., S.M. Giuliatti Winter, and R.S. Gomes. 2015. The evolution of a Pluto-like system during the migration of the ice giants. Icarus 246: 330-338. Quintana, E.V., T. Barclay, W.J. Borucki, J.F. Rowe, and J.E. Chambers. 2016. The frequency of giant impacts on Earth-like worlds. The Astrophysical Journal 821, no. 2: 126-139. Rickman, H., T. Wisniowski, R. Gabryszewski, P. Wajer, K. Wojcikowski, S. Szutowicz, G.B. Valsecchi, andA. Morbidelli. 2017. Cometary impact Figure 14. Cross sectional view of the stationary body (model Earth) along the equatorial x-y plane showing the total displacement for both mantle and core material occurring during the fly-by of an Earth mass object. Counter clockwise from the upper left are shown displacements at time steps referenced to time of nearest passage. The position of the fly-by mass is shown as it passes above the stationary object from right to left (indicated by arrows). Note the largest residual displacements after passage follow nearly parallel to the surface, approximately 60 km lateral displacement.
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