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

Seely et al. ◀ Finite element analysis of a near impact event ▶ 2018 ICC 66 rates on the Moon and planets during the late heavy bombardment. Astronomy and Astrophysics 598: A67. Sherburn, J.A., J.R. Baumgardner, and M.F. Horstemeyer. 2013. New material model reveals inherent tendency in mantle minerals for runaway mantle dynamics. In Proceedings of the Seventh International Conference on Creationism , ed. M.F. Horstemeyer. Pittsburgh, Pennsylvania: Creation Science Fellowship. Sherburn, J.A., M.F. Horstemeyer, D.J. Bammann, and J.R. Baumgardner. 2011. Application of the Bammann inelasticity internal state variable constitutive model to geological materials. Geophysical Journal International 184:1023–1036. Spencer, W.R. 1998. Geophysical effects of Impacts during the Genesis Flood. In Proceedings of the Fifth International Conference on Creationism , ed. R.E. Walsh., pp. 567-579. Pittsburgh, PA: Creation Science Fellowship. Tsiganis, K., R. Gomes, A. Morbidelli, and H.F. Levison. 2005. Origin of the orbital architecture of the giant planets of the Solar System. Nature 435: 459–461. Wiechert, U., A.N. Halliday, D.C. Lee, G.A. Snyder, L.A. Taylor, and D. Rumble. 2001. Oxygen isotopes and the Moon-forming giant impact. Science 294, no. 5541: 345-348. Wise, K.P., S.A. Austin, J.R. Baumgardner, D.R. Humphreys, A.A. Snelling, and L. Vardiman. 1994. Catastrophic late tectonics: A global Flood model of earth history. In Proceedings of the Third International Conference on Creationism , ed. R.E. Walsh, pp. 609-621. Pittsburgh, Pennsylvania: Creation Science Fellowship. Zhang, J., N. Dauphas, A.M. Davis, I. Leya, and A. Fedkin. 2012. The proto-Earth as a significant source of lunar material. Nature Geoscience 5: 251-255. Figure 15. Von Mises stress contour for cross sections of the stationary body (model Earth) along the equatorial x-y plane for the near passage of an Earth mass object. Initial Von Mises stresses for simulation this step are carried forward from the preceding self-loading step. Counter clockwise from the upper left are shown Von Mises stress contours 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). The highest value of mantle stress at the core mantle interface in the quadrant between the near-side and retreat faces. The band of reduced stress begins on the opposite side from the passing object and sweeps around to the approach face.

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