Name: Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes (Springer Theses) (en Inglés)
SKU: 52531202
Price: 2141.03 MXN
Availability: InStock
Author: Keisuke Sugiura
ISBN: 9789811537219

portada Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes (Springer Theses) (en Inglés)

Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes (Springer Theses) (en Inglés)

Formato

Libro Físico

Editorial

Springer

Autor

Keisuke Sugiura

Año

2020

Idioma

Inglés

N° páginas

147

Encuadernación

Tapa Dura

ISBN13

9789811537219

N° edición

Categorías

Astronomía, espacio y tiempo

Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes (Springer Theses) (en Inglés)

Keisuke Sugiura (Autor) · Springer · Tapa Dura

Libro Nuevo Importado

Envío: 14 a 19 días háb.

$ 4,757.86$ 2,141.03

-55%

Costos de importación incluídos en el precio ✅

Libro Nuevo

Quedan más de 100 unidades

$ 2,141.03

¡Envío Gratis! Llega entre el 24 Sep y el 02 Oct a CUAUHTÉMOC, Ciudad de México. Seleccionar ubicación

Agregar a lista de deseos

Reseña del libro "Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Asteroidal Shapes (Springer Theses) (en Inglés)"

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.