The Proceedings of the Eighth International Conference on Creationism (2018)

Seely et al. ◀ Finite element analysis of a near impact event ▶ 2018 ICC 64 Bate, R.M., and A. Burkert. 1997. Resolution requirements for smoothed particle hydrodynamics calculations with self-gravity. Monthly Notices of the Royal Astronomical Society 288, no 4: 1060-1072. Baumgardner, J.R. 2003. Catastrophic plate tectonics: the physics behind the Genesis Flood. In Proceedings of the Fifth International Conference on Creationism , ed. R.L. Ivey, Jr., pp. 113–126. Pittsburgh, Pennsylvania: Creation Science Fellowship. Baumgardner, J.R. 2013. Explaining the continental fossil-bearing sediment record in terms of the Genesis Flood: insights from numerical modeling of erosion, sediment transport and deposition processes on a global scale. In Proceedings of the Seventh International Conference on Creationism , ed. M.F. Horstemeyer. Pittsburgh, Pennsylvania: Creation Science Fellowship. Baumgardner, J.R. 2016. Numerical modeling of the large-scale erosion, sediment transport, and deposition processes of the Genesis Flood. Answers Research Journal 9: 1-24. Canup, R., and E. Asphaug. 2001. Origin of the Moon in a giant impact near the end of the Earth’s formation. Nature 412: 708-712. Cho, H., M. Horstemeyer, J. Baumgardner, and J. Sherburn. 2018. Strength-reducing mechanisms in mantle rock during the Genesis Flood. In Proceedings of the Eighth International Conference on Creationism , ed. J.H. Whitmore, pp. 707-730. Pittsburgh, Pennsylvania: Creation Science Fellowship. Cuk, M. and, S.T. Stewart. 2012. Making the moon from a fast-spinning earth: a giant impact followed by resonant despinning. Science 338, no. 6110: 1047-1052. de Vries, J., A. van den Berg, and W. van Westrenen. 2010. Formation and evolution of a lunar core from ilmenite-rich magma ocean cumulates. Earth and Planetary Science Letters 292, no. 1: 139-147. Dziewonski, A.M., and D.L. Anderson. 1981. Preliminary reference Earth model. Physics of the Earth and Planetary Interiors 25: 297-356 Gomes, R., H.F. Levison, K. Tsiganis, and A. Morbidelli. 2005. Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets. Nature 435: 466–469. Hammi, Y., T.W. Stone, B. Paliwal, M.F. Horstemeyer, and P.G. Allison. 2016. Smooth yield surface constitutive modeling for granular Figure 13. Global map of permanent radial displacements for a two-layer Earth size model after near passage of a lunar mass object. The color coding indicates permanent topographical change after subsidence of the transient elastic displacements. Counter clockwise from the upper left are shown: (E) polar view, equatorial views of (C) near-side surface, (B) retreat-side surface, (D) far-side surface, and (B) approach-side surface. The value of the displacement is relative to the original surface as measured from the geometric center of the body. Note the global pattern of highlands (greens through red) and lowlands (blues), there are two elevated peaks and a band of lowlands stretching from pole to pole around the far-side.