PDF Ebook Fundamentals of Astrodynamics (Dover Books on Aeronautical Engineering), by Roger R. Bate, Donald D. Mueller, Jerry E. White
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PDF Ebook Fundamentals of Astrodynamics (Dover Books on Aeronautical Engineering), by Roger R. Bate, Donald D. Mueller, Jerry E. White
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When the United States Air Force Academy began teaching astrodynamics to undergraduates majoring in astronautics or aerospace engineering, it found that the traditional approach to the subject was well over 100 years old. An entirely new text had to be evolved, geared to the use of high speed digital computers and actual current practice in the industry. Over the years the new approach was proven in the classrooms of the Academy; its students entering graduate engineering schools were found to possess a better understanding of astrodynamics than others. So pressing is the need for superior training in the aerospace sciences that the professor-authors of this text decided to publish it for other institutions' use. This Dover edition is the result.The text is structured for teaching. Central emphasis is on use of the universal variable formulation, although classical methods are discussed. Several original unpublished derivations are included. A foundation for all that follows is the development of the basic two-body and n-body equations of motion; orbit determination is then treated, and the classical orbital elements, coordinate transformations, and differential correction. Orbital transfer maneuvers are developed, followed by time-of-flight with emphasis on the universal variable solution. The Kepler and Gauss problems are treated in detail. Two-body mechanics are applied to the ballistic missile problem, including launch error analysis and targeting on a rotating earth. Some further specialized applications are made to lunar and interplanetary flight, followed by an introduction to perturbation, special perturbations, integration schemes and errors, and analytic formulation of several common perturbations.Example problems are used frequently, while exercises at the end of each chapter include derivations and quantitative and qualitative problems. The authors suggest how to use the text for a first course in astrodynamics or for a two-course sequence.This major instructional tool effectively communicates the subject to engineering students in a manner found in no other textbook. Its efficiency has been thoroughly demonstrated. Dover feels privileged in joining with the authors to make its concepts and text matter available to other faculties.
- Sales Rank: #24186 in Books
- Published on: 1971-06-01
- Released on: 1971-06-01
- Original language: English
- Number of items: 1
- Dimensions: 8.48" h x .92" w x 5.44" l, 1.06 pounds
- Binding: Paperback
- 480 pages
From the Back Cover
When the United States Air Force Academy began teaching astrodynamics to undergraduates majoring in astronautics or aerospace engineering, it found that the traditional approach to the subject was well over 100 years old. An entirely new text had to be evolved, geared to the use of high speed digital computers and actual current practice in the industry. Over the years the new approach was proven in the classrooms of the Academy; its students entering graduate engineering schools were found to possess a better understanding of astrodynamics than others. So pressing is the need for superior training in the aerospace sciences that the professor-authors of this text decided to publish it for other institutions' use. This Dover edition is the result.The text is structured for teaching. Central emphasis is on use of the universal variable formulation, although classical methods are discussed. Several original unpublished derivations are included. A foundation for all that follows is the development of the basic two-body and n-body equations of motion; orbit determination is then treated, and the classical orbital elements, coordinate transformations, and differential correction. Orbital transfer maneuvers are developed, followed by time-of-flight with emphasis on the universal variable solution. The Kepler and Gauss problems are treated in detail. Two-body mechanics are applied to the ballistic missile problem, including launch error analysis and targeting on a rotating earth. Some further specialized applications are made to lunar and interplanetary flight, followed by an introduction to perturbation, special perturbations, integration schemes and errors, and analytic formulation of several common perturbations.Example problems are used frequently, while exercises at the end of each chapter include derivations and quantitative and qualitative problems. The authors suggest how to use the text for a first course in astrodynamics or for a two-course sequence.This major instructional tool effectively communicates the subject to engineering students in a manner found in no other textbook. Its efficiency has been thoroughly demonstrated. Dover feels privileged in joining with the authors to make its concepts and text matter available to other faculties.
A new work, first published by Dover in 1971.
Most helpful customer reviews
55 of 58 people found the following review helpful.
Good Reference Source for Students, Engineers and Educators
By L. S. Fischer
While working for NASA/JPL back in the 1970's and 80's, I first used this book as a reference source while doing engineering support for radio astronomy experiments. I recall at the time wishing I'd know of the book a few years earlier while still at the Univ. of Arizona; while a student I would have found plenty of use for it.
Recently I have returned to academia, and find myself making use some of its material for by my lower-division astronomy students. I've come to depend on it for its clearly-written explanations of the various coordinate systems, reference frames and obital dynamics. And I especially like the way it introduces n-body problems and the how they are affected by perturbations. For myself I even make some use of it when doing calindrical calculations.
It is among a handful of reference sources that I find almost continuously useful in so many applications.
40 of 44 people found the following review helpful.
Some topics omitted, but still a good book
By Dr. Lee D. Carlson
This book is a fairly complete overview of planetary mechanics, at least from the standpoint of the Newtonian formulation of the problem, for the authors do not use Lagrangian or Hamiltonian methods. The use of Hamiltonian formulation, via phase space constructions, sheds considerable light on the two-body and the N-body problems, but the reader interested in Hamiltonian mechanics will have to look elsewhere. Also, the authors do not discuss the presence of chaotic dynamics in orbital mechanics, nor are integrability issues discussed. In addition, the current debate over modifications of Newtonian mechanics is not included in the book, due to its time of publication.
But if one wants a practical introduction to Newtonian orbital mechanics that also addresses numerical issues, this would be a good book to begin with. I would recommend the use of a symbolic programming language, such as Mathematica or Maple, to assist in the visualization of the orbits and in the routine computations if one were to use this book as an aid to teaching orbital mechanics. Another good feature of the book is the interjection of historical background and anecdotes at various places in the book. For example, one learns that it was Edmund Halley who was primarily responsible for bringing Newton's discoveries to the world. Newton's work remained idle for twenty years until Halley encouraged Newton to publish his explanation of planetary motion.
The mechanics as outlined in this book is timeless and will continue to be learned by future generations of students as they take up the reigns of human exploration beyond the Moon to the entire solar system.
16 of 16 people found the following review helpful.
An excellent introductory text to the subject
By A Customer
This work was written by three instructors at the USAF Academy for use as a textbook. It provides an excellent introduction to astrodynamics. A knowledge of calculus and linear algebra is required, but the derivations are quite reasonable. The diagrams are also very good, enabling the reader to visualize complex spatial orientations.
The book's only weakness is its age. Several real-world examples are out-of-date, and the numerical analysis techniques do not reflect the current state-of-the-art.
Nevertheless, this is the best book to start learning astrodynamics, and gives a solid foundation from which to study more advanced texts.
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