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An introduction to celestial mechanics, by Forest Ray Moulton
Fee Download An introduction to celestial mechanics, by Forest Ray Moulton
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This is a reproduction of a book published before 1923. This book may have occasional imperfections such as missing or blurred pages, poor pictures, errant marks, etc. that were either part of the original artifact, or were introduced by the scanning process. We believe this work is culturally important, and despite the imperfections, have elected to bring it back into print as part of our continuing commitment to the preservation of printed works worldwide. We appreciate your understanding of the imperfections in the preservation process, and hope you enjoy this valuable book.
- Sales Rank: #7855966 in Books
- Published on: 2010-09-07
- Original language: English
- Number of items: 1
- Dimensions: 9.69" h x .94" w x 7.44" l, 1.83 pounds
- Binding: Paperback
- 468 pages
Most helpful customer reviews
31 of 31 people found the following review helpful.
Great Reference for All
By Scott Lewis
If you happen to be unfortunate enough to be using Goldstein's, Classical Mechanics, you will find that Kepler's Laws are not fully explored. I found the Moulton book to fill in alot of gaps. I do mean....alot of gaps! The book gives great detail into series expansions. Not only does it address the series, but it addresses the exact origin and derivation of the series expansions. The only thing it lacks is the recursion formula! Moulton treats all of the equations like this. He shows you complete derivations of everything. And, he is good in showing you applications of what you've learned.
In itself, the book is a textbook, but it serves as a great companion to any modern text. This book is actually quite old, so it gives you alot of insight into "antequated knowledge." You know, the "stuff" teachers already assume you know.
So, I recommend this book to anyone. It is very readable. It explains concepts in a very simplistic manner. Unlike modern books that give you point "A" and expect you to fill in all the gaps to point "Z," Moulton uses the "old style of teaching" where he takes you from point "A" to point "Z" to fully prepare you, and then, he slams you with the impossible problems at the end. But, you find the problems are not nearly as difficult due to his preparations.
Great Book!!
23 of 23 people found the following review helpful.
Good historical background
By Robert Stellingwerf
This is an excellent textbook covering not only celestial mechanics, but a wide range of astrophysics topics. It was written in 1902 and updated in 1914. At that time nuclear processes were not known, and the composition of the sun was thought to be mainly iron. Given these limitations, however, the math is clear, the definitions are still used, and the historical background is interesting and informative. For a more up-to-date discussion of the subject, I recommend "Fundamentals of Astrodynamics", Bate, Mueller, White (1971), but get this one for the background.
2 of 2 people found the following review helpful.
Pinnacle Text on Newtonian Celestial Mechanics, 1962 MacMillan Co., Second Revision Ed.
By Directed Energy
This text by Moulton is perhaps the finest single treatment on Newtonian Celestial Mechanics available. The content is very methodically shared in detail and progresses in a logical, building block manner accentuated with brief discussions on the historical development of the theories.
Moulton covers the basics of linear motion as a short refresher in the begin of Chp 2 but does assume the reader is already familiar with linear algebra determinants, and Lagrangian mechanics when covering perturbation theory.
Not in the text are conversations on the Roche Limit, Lagrangian Points, and Relativistic Celestial Mechanics. The text does discus surface equipotentials in chapter VII The Problem of Three Bodies.
Some of my favorite sections of the text being:
Chp I Fundamental Principles and Definitions
I.16 pertaining to Kepler and discussion on Areal Velocity
Chp II Rectilinear Motion
II.33 Attractive Force Varying Inversely as the Square of the Distance
Chp III Central Force
III.55 Newton's Law of Gravitation
III.62 Force Varying as the Square of the Distance
Chp IV The Potential and Attractions of Bodies
IV.78 The Potential and Attraction of a Solid Homogeneous Oblate Spheroid upon a Distant Unit Particle
IV.81 The Attraction of Spheroids
Chp V The Problem of Two Bodies
V.97 Graphical Solution of Kepler's Equation
V.104 The Heliocentric Position in the Ecliptic System
Chp VIII The Problem of Three Bodies
VIII.163 Application to the Gegenschein
Chp IX Perturbations-Geometrical Considerations
IX.175 Disturbing Effects of the Orthogonal Components
IX.188 Perturbations of the Inclination
IX.189 Precession of the Equinoxes. Nutation
IX.197 The Motion of the Line of Apsides
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