Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes

Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes

Author: Keisuke Sugiura

Publisher: Springer Nature

Published: 2020-03-17

Total Pages: 143

ISBN-13: 9811537224

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This book describes numerical simulations of collisions between asteroids, based on a unique numerical code developed by the author. The code accurately solves the elastic dynamic equations and describes the effects of fracture and friction, which makes it possible to investigate the shapes of impact outcomes produced by asteroid collisions and subsequent gravitational accumulation of fragments. The author parallelizes the code with high parallelization efficiency; accordingly, it can be used to conduct high-resolution simulations with the aid of supercomputers and clarify the shapes of small remnants produced through the catastrophic destruction of asteroids. The author demonstrates that flat asteroids can only be produced by impacts involving objects with similar mass and low velocity, which suggests that the flat asteroids in our solar system were created in the planet formation era and have kept their shapes until today. The author also shows that asteroid collisions under certain conditions can produce the extremely elongated shape of an interstellar minor body, 1I/‘Oumuamua. In brief, the book offers a comprehensive investigation of asteroid impacts and shapes, making it a uniquely valuable resource.


Literature 1997, Part 1

Literature 1997, Part 1

Author: Astronomisches Rechen-InstitutARI

Publisher: Springer Science & Business Media

Published: 2013-11-11

Total Pages: 1746

ISBN-13: 3642517587

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Astronomy and Astrophysics Abstracts is devoted to the recording, summarizing and indexing of astronomical publications throughout the world. Two volumes are scheduled to appear per year. Volume 67 records 10,903 papers covering besides the classical fields of astronomy and astrophysics such matters as space flights related to astronomy, lunar and planetary probes and satellites, meteorites and interplanetary matter, X rays and cosmic rays, quasars and pulsars. The abstracts are classified under more than one hundred subject categories thus permitting quick surveying of the bulk of material published on the same topic within six months. For instance, this volume records 119 papers on minor planets, 155 papers on supernovae, and 554 papers on cosmology.


Application of Rigid Body Impact Mechanics and Discrete Element Modeling to Rockfall Simulation

Application of Rigid Body Impact Mechanics and Discrete Element Modeling to Rockfall Simulation

Author: Parham Ashayer

Publisher:

Published: 2007

Total Pages: 410

ISBN-13: 9780494393994

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Numerical modeling can assist in predicting falling rock trajectories and reducing the destruction caused by rockfalls. The majority of existing rockfall simulations are based on particle or lumped-mass models that consider the falling rock as an infinitesimal particle with a concentrated mass. Hybrid models usually find the rock-slope contact point using techniques similar to those used in particle models, while incorporating some aspects of the rigid body collisions for bouncing. There are also some rigid body models that employ simplified mathematical impact models. In the framework of this thesis, the applications of rigid body theory and discrete element modeling to rockfall simulation are investigated. A modified version of the discrete element model (MDEM), which can model impacts using methods similar to low-compliance impact models, is offered. In this model, the normal linear dashpot is replaced by a nonlinear dashpot which dissipates the impact velocity based on the contact normal velocity. A mono-direction sliding unit is added to model low-compliance impacts and the tangential dashpot is removed. Several numerical tests strongly indicate that if shape geometries can be sufficiently approximated by a group of particles, the proposed MDEM can replicate the rebound velocities that are predicted by the application of low compliance rigid body impact models. Application of rigid body impact mechanics (RBIM), originally developed by Stronge, in rockfall simulation is studied and compared with other classical rockfall impact models. The effects of several parameters on widely-used coefficients of restitution are investigated including: rock geometry and slenderness, angle of impact, rock orientation, and slope material properties. A new geometrical rockfall simulation program, GeoRFS, based on rigid body mechanics in two-dimensional space, is developed, where rock geometry can vary from prisms with a randomly generated polygonal cross section to superellipsoids. The trajectories of different rock geometries (e.g., roll-out distances, bounce heights, velocities, and energies) during multiple impacts on flat and inclined impact surfaces are studied. The results strongly suggest that the provided simulation program can satisfactorily replicate the roll-out distances obtained from the in-situ tests performed by the Oregon Department of Transportation using different rock geometries. It is expected that the geometrical simulation tools introduced in this work will replace the particle impact model currently used in rockfall programs.


Numerical N-body Approach to Binary Asteroid Formation and Evolution

Numerical N-body Approach to Binary Asteroid Formation and Evolution

Author: Carlo Comito

Publisher:

Published: 2012

Total Pages: 171

ISBN-13:

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Binary asteroids play a role of primary importance in determining some physical parameters difficult to measure from Earth, such as the mass. By studying the origin of binaries in the general frame of gravitational aggregates, we can use them as natural laboratories for granular system physics in microgravity conditions, thus obtaining valuable information for modelling asteroids in general. A large variety exists as for the range of parameters of the observed binary systems, and many possible origins have been suggested for them (catastrophic shattering of a parent object and reaccumulation as multiple bodies, planetary tidal perturbations, cratering, YORP ...). In this work we explore by numerical N-body simulations the dynamics of gravitational aggregates outside the limits of stability for a single body, looking for the most favourable configurations leading to binary systems formation. First we show how common the formation of binary systems in a catastrophic scenario is, well reproducing the variety in the observed population. As a second step we explore the possibility of a gradual shape deformation of an aggregate towards a binary system by the action of a slow perturbing force leading to a possible fission of the body. Our results provide new insights into the formation of asteroid binaries, as shown by a comparison to observations and existing literature.