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Excerpt from On the Stability of the Motion of Saturn's Rings There are some questions in Astronomy, to which we are attracted rather on account of their peculiarity, as the possible illustration of some unknown principle, than from any direct advantage which their solution would afford to mankind. The theory of the Moons inequalities, though in its first stages it presents theorems interesting to all students of mechanics, has been pursued into such intricacies of calculation as can be followed up only by those who make the improvement of the Lunar Tables the object of their lives. The value of the labours of these men is recognised by all who are aware of the importance of such tables in Practical Astronomy and Navigation. The methods by which the results are obtained are admitted to be sound, and we leave to professional astronomers the labour and the merit of developing them. The questions which are suggested by the appearance of Saturn's Rings cannot, in the present state of Astronomy, call forth so great an amount of labour among mathematicians. I am not aware that any practical use has been made of Saturn's Rings, either in Astronomy or in Navigation. They are too distant, and too insignificant in mass, to produce any appreciable effect on the motion of other parts of the Solar system; and for this very reason it is difficult to determine those elements of their motion which we obtain so accurately in the case of bodies of greater mechanical importance. But when we contemplate the Rings from a purely scientific point of view, they become the most remarkable bodies in the heavens, except, perhaps, those still less useful bodies - the spiral nebulae. When we have actually seen that great arch swung over the equator of the planet without any visible connexion, we cannot bring our minds to rest. We cannot simply admit that such is the case, and describe it as one of the observed facts in nature, not admitting or requiring explanation. We must either explain its motion on the principles of mechanics, or admit that, in the Saturnian realms, there can be motion regulated by laws which we are unable to explain. About the Publisher Forgotten Books publishes hundreds of thousands of rare and classic books. Find more at www.forgottenbooks.com This book is a reproduction of an important historical work. Forgotten Books uses state-of-the-art technology to digitally reconstruct the work, preserving the original format whilst repairing imperfections present in the aged copy. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in our edition. We do, however, repair the vast majority of imperfections successfully; any imperfections that remain are intentionally left to preserve the state of such historical works.
From the first time they were dimly sighted through Galileo's telescope to the recent spectacular pictures beamed back by Voyager, Saturn's rings have fascinated generations of observers. The scientific problems associated with them have also attracted the attention of successive generations of theoreticians. James Clerk Maxwell's 1856 Adams Prize Essay, "On the Stability of the Motion of Saturn's Rings," forms the central body of this book and is the work that first established his reputation as one of the greatest mathematical physicists of any generation. It is surrounded by previously unpublished materials written both before and after the essay was completed. The former group consists of sixteen letters - to William Thomson (later Lord Kelvin), George Gabriel Stokes, Peter Guthrie Tait, and other friends and colleagues - written while Maxwell was working out the problems and preparing the essay for publication, and they reveal both the sureness of his approach and false starts and errors. The post-essay documents include a review of the work by George Biddell Airy, the Astronomer Royal, and correspondence with the Harvard astronomer George Bond in 1863. Here Maxwell attempts to extend his analysis to include the effects of collisions among the particles of the ring, employing his own newly developed kinetic theory of gases. The editors' introduction provides a historical context for Maxwell's contribution.