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Shapes and dynamics of granular mino...

Sharma, Ishan.

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Shapes and dynamics of granular minor planets = the dynamics of deformable bodies applied to granular objects in the solar system /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Shapes and dynamics of granular minor planets/ by Ishan Sharma.
Reminder of title:	the dynamics of deformable bodies applied to granular objects in the solar system /
Author:	Sharma, Ishan.
Published:	Cham :Springer International Publishing : : 2017.,
Description:	xx, 354 p. :ill., digital ;24 cm.
[NT 15003449]:	Preface -- Mathematical preliminaries -- Continuum mechanics -- Afﬁne dynamics -- Asteroids -- Satellites -- Binaries -- Granular materials.
Contained By:	Springer eBooks
Subject:	Asteroids. -
Online resource:	http://dx.doi.org/10.1007/978-3-319-40490-5
ISBN:	9783319404905

Shapes and dynamics of granular minor planets = the dynamics of deformable bodies applied to granular objects in the solar system /
Sharma, Ishan.

Shapes and dynamics of granular minor planetsthe dynamics of deformable bodies applied to granular objects in the solar system /[electronic resource] :by Ishan Sharma. - Cham :Springer International Publishing :2017. - xx, 354 p. :ill., digital ;24 cm. - Advances in geophysical and environmental mechanics and mathematics,1866-8348. - Advances in geophysical and environmental mechanics and mathematics..

Preface -- Mathematical preliminaries -- Continuum mechanics -- Afﬁne dynamics -- Asteroids -- Satellites -- Binaries -- Granular materials.

This book develops a general approach that can be systematically refined to investigate the statics and dynamics of deformable solid bodies. These methods are then employed to small bodies in the Solar System. With several space missions underway and more being planned, interest in our immediate neighbourhood is growing. In this spirit, this book investigates various phenomena encountered in planetary science, including disruptions during planetary fly-bys, equilibrium shapes and stability of small rubble bodies, and spin-driven shape changes. The flexible procedure proposed here will help readers gain valuable insights into the mechanics of solar system bodies, while at the same time complementing numerical investigations. The technique itself is built upon the virial method successfully employed by Chandrasekhar (1969) to study the equilibrium shapes of spinning fluid objects. However, here Chandrasekhar's approach is modified in order to study more complex dynamical situations and include objects of different rheologies, e.g., granular aggregates, or "rubble piles". The book is largely self-contained, though some basic familiarity with continuum mechanics will be beneficial.

ISBN: 9783319404905

Standard No.: 10.1007/978-3-319-40490-5doiSubjects--Topical Terms:

566765
Asteroids.

LC Class. No.: QB651

Dewey Class. No.: 523.44

Shapes and dynamics of granular minor planets = the dynamics of deformable bodies applied to granular objects in the solar system /
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490 1 $a Advances in geophysical and environmental mechanics and mathematics, $x 1866-8348
505 0 $a Preface -- Mathematical preliminaries -- Continuum mechanics -- Afﬁne dynamics -- Asteroids -- Satellites -- Binaries -- Granular materials.
520 $a This book develops a general approach that can be systematically refined to investigate the statics and dynamics of deformable solid bodies. These methods are then employed to small bodies in the Solar System. With several space missions underway and more being planned, interest in our immediate neighbourhood is growing. In this spirit, this book investigates various phenomena encountered in planetary science, including disruptions during planetary fly-bys, equilibrium shapes and stability of small rubble bodies, and spin-driven shape changes. The flexible procedure proposed here will help readers gain valuable insights into the mechanics of solar system bodies, while at the same time complementing numerical investigations. The technique itself is built upon the virial method successfully employed by Chandrasekhar (1969) to study the equilibrium shapes of spinning fluid objects. However, here Chandrasekhar's approach is modified in order to study more complex dynamical situations and include objects of different rheologies, e.g., granular aggregates, or "rubble piles". The book is largely self-contained, though some basic familiarity with continuum mechanics will be beneficial.
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