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

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes/ by Keisuke Sugiura.
作者:	Sugiura, Keisuke.
面頁冊數:	XIII, 134 p. 57 illus., 55 illus. in color.online resource. :
Contained By:	Springer Nature eBook
標題:	Numerical and Computational Physics, Simulation. -
電子資源:	https://doi.org/10.1007/978-981-15-3722-6
ISBN:	9789811537226

Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes
Sugiura, Keisuke.

Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes[electronic resource] /by Keisuke Sugiura. - 1st ed. 2020. - XIII, 134 p. 57 illus., 55 illus. in color.online resource. - Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053. - Springer Theses, Recognizing Outstanding Ph.D. Research,.

Introduction -- Method -- Results: Shapes of Impact Outcomes -- Discussion: Collisional History of Asteroids -- Application: Extremely Elongated Shape of 1I/′Oumuamua -- Summary and Future Prospects -- Summary and Future Prospects -- Acknowledgement. .

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.

ISBN: 9789811537226

Standard No.: 10.1007/978-981-15-3722-6doiSubjects--Topical Terms:

1112293
Numerical and Computational Physics, Simulation.

LC Class. No.: QB600-701

Dewey Class. No.: 523.2

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