Titlebook: Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste; Keisuke Sugiura Book 2020 The Editor

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https://doi.org/10.1007/978-3-662-29974-6 numerical simulations. We also analyzed shapes of actual asteroids and compare them with shapes of impact outcomes produced through our simulations. Finally we applied our simulations to the formation of the extremely elongated shape of 1I/‘Oumuamua. In this chapter, we summarize our study. We also

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Book 2020and 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 u

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2190-5053 er 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 u978-981-15-3724-0978-981-15-3722-6Series ISSN 2190-5053 Series E-ISSN 2190-5061

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Introduction,apter, we introduce the overview of the solar system, the properties of asteroids, the standard solar system formation scenario, and the collisional phenomena between rocky minor bodies as basic knowledge to extract information of the past solar system from asteroids’ shapes.

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

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Method,such numerical simulations, we need knowledge about not only hydrodynamics but also elastic dynamics for intact rocks, fracturing of rocky materials, and friction of completely damaged rocks. In this chapter, we introduce the detailed methods necessary for numerical simulations of asteroidal collisi

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Results: Shapes of Impact Outcomes, Database of Asteroid Models from Inversion Techniques provides almost all shapes of known asteroids with diameters larger than 100 km. Thus, in our impact simulations, we set radius of target asteroids to 50 km to allow us to directly compare the results of our simulations with the shapes of actual

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