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Conservative and dissipative models ...

Celletti, A.

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Conservative and dissipative models of celestial mechanics

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Conservative and dissipative models of celestial mechanics/ by Alessandra Celletti.
作者:	Celletti, A.
出版者:	Cham :Springer Nature Switzerland : : 2025.,
面頁冊數:	xxi, 274 p. :ill. (chiefly col.), digital ;24 cm.
內容註:	Chapter 1. Conservative and dissipative dynamical systems -- Chapter 2. Perturbation theory -- Chapter 3. Kepler's problem -- Chapter 4. The 3-body problem. Chapter 5. Euler-Lagrange solutions -- Chapter 6. Halo orbits -- Chapter 7. Laplace resonance -- Chapter 8. The geopotential and the J2 problem -- Chapter 9. Earth's satellite and space debris dynamics -- Chapter 10. The spin-orbit problem -- Chapter 11. Rotational dynamics with obliquity -- Chapter 12. The spin-spin model -- Chapter 13. Dumbbell and tether models -- Chapter 14. Solar sails.
Contained By:	Springer Nature eBook
標題:	Celestial mechanics. -
電子資源:	https://doi.org/10.1007/978-3-032-01866-3
ISBN:	9783032018663

Conservative and dissipative models of celestial mechanics
Celletti, A.

Conservative and dissipative models of celestial mechanics[electronic resource] /by Alessandra Celletti. - Cham :Springer Nature Switzerland :2025. - xxi, 274 p. :ill. (chiefly col.), digital ;24 cm. - Springer monographs in mathematics,2196-9922. - Springer monographs in mathematics..

Chapter 1. Conservative and dissipative dynamical systems -- Chapter 2. Perturbation theory -- Chapter 3. Kepler's problem -- Chapter 4. The 3-body problem. Chapter 5. Euler-Lagrange solutions -- Chapter 6. Halo orbits -- Chapter 7. Laplace resonance -- Chapter 8. The geopotential and the J2 problem -- Chapter 9. Earth's satellite and space debris dynamics -- Chapter 10. The spin-orbit problem -- Chapter 11. Rotational dynamics with obliquity -- Chapter 12. The spin-spin model -- Chapter 13. Dumbbell and tether models -- Chapter 14. Solar sails.

This book is devoted to the presentation and discussion of some models of relevance in Celestial Mechanics and Astrodynamics. The motions of celestial bodies, either natural or artificial, are governed by conservative forces, like the gravitational attraction that preserve the total energy and by dissipative forces, like the tidal torque, Stokes drag, and the Poynting-Robertson effect. The basic idea of this book is to describe in each chapter a model in the conservative setting, providing its main features, and then to extend the model by including dissipative forces. In fact, the dynamics of many objects of the Solar system is well described, in a first approximation, by a conservative model; however, in the long term, dissipative effects may play a relevant role, for example, in shaping the dynamics and affecting the evolutionary history of the Solar system. Motivated by this observation, in this book, different models are presented and their main features are described in the conservative setting, but dissipative contributions, pertinent to the model, are added as well, which may lead to a completely different dynamics on long time scales. Conservative systems have a larger variety of motions, e.g., the dynamics can take place on rotational tori, librational motions, periodic orbits, and chaotic trajectories. On the contrary, dissipative systems admit a less rich dynamics, since the dissipation forces the motion to take place on a few attractors, e.g., rotational tori, periodic orbits or strange attractors. Besides, dissipative systems often need extra parameters to compensate for the loss of energy and to allow the dynamics to take place on non-trivial attractors. The book is addressed to graduate students and researchers interested in models of Celestial Mechanics and Astrodynamics.

ISBN: 9783032018663

Standard No.: 10.1007/978-3-032-01866-3doiSubjects--Topical Terms:

534193
Celestial mechanics.

LC Class. No.: QB351

Dewey Class. No.: 521

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505 0 $a Chapter 1. Conservative and dissipative dynamical systems -- Chapter 2. Perturbation theory -- Chapter 3. Kepler's problem -- Chapter 4. The 3-body problem. Chapter 5. Euler-Lagrange solutions -- Chapter 6. Halo orbits -- Chapter 7. Laplace resonance -- Chapter 8. The geopotential and the J2 problem -- Chapter 9. Earth's satellite and space debris dynamics -- Chapter 10. The spin-orbit problem -- Chapter 11. Rotational dynamics with obliquity -- Chapter 12. The spin-spin model -- Chapter 13. Dumbbell and tether models -- Chapter 14. Solar sails.
520 $a This book is devoted to the presentation and discussion of some models of relevance in Celestial Mechanics and Astrodynamics. The motions of celestial bodies, either natural or artificial, are governed by conservative forces, like the gravitational attraction that preserve the total energy and by dissipative forces, like the tidal torque, Stokes drag, and the Poynting-Robertson effect. The basic idea of this book is to describe in each chapter a model in the conservative setting, providing its main features, and then to extend the model by including dissipative forces. In fact, the dynamics of many objects of the Solar system is well described, in a first approximation, by a conservative model; however, in the long term, dissipative effects may play a relevant role, for example, in shaping the dynamics and affecting the evolutionary history of the Solar system. Motivated by this observation, in this book, different models are presented and their main features are described in the conservative setting, but dissipative contributions, pertinent to the model, are added as well, which may lead to a completely different dynamics on long time scales. Conservative systems have a larger variety of motions, e.g., the dynamics can take place on rotational tori, librational motions, periodic orbits, and chaotic trajectories. On the contrary, dissipative systems admit a less rich dynamics, since the dissipation forces the motion to take place on a few attractors, e.g., rotational tori, periodic orbits or strange attractors. Besides, dissipative systems often need extra parameters to compensate for the loss of energy and to allow the dynamics to take place on non-trivial attractors. The book is addressed to graduate students and researchers interested in models of Celestial Mechanics and Astrodynamics.
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