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Summary and Future Prospects

  • Keisuke SugiuraEmail author
Chapter
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Part of the Springer Theses book series (Springer Theses)

Abstract

We firstly developed a numerical simulation code for rocky body collisions. Then we investigated shapes of asteroids formed by various impacts through 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 state future prospects of our study such as application to other phenomena.

Keywords

Summary Simulation method for rocky body impacts Asteroid shapes formed through collisions Application 

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Copyright information

© Springer Nature Singapore Pte Ltd. 2020

Authors and Affiliations

  1. 1.Earth-Life Science InstituteTokyo Institute of TechnologyMeguroJapan

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