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This book is not hagiography; Spencer P. Jones was not a saint, nor would he wish to be canonised as such. Spencer could be as flaky as he was trusting, as frustrating as he was loveable. In the course of researching this biography I witnessed first-hand the good and not-so-good of Spencer's personality: his intelligence and humour, his trust and generosity, his laissez-faire approach to time management, his well-meaning financial dissonance. Spencer was his own worst enemy, and at particular times in his life, his behaviour undermined both his career and some of his closest relationships. Spencer P. Jones did bad things, but he was never a bad person. He was just Spencer. And there will never be another like him.
In Home Is Where the Wind Blows, Sir Fred Hoyle, one of this century's most eminent scientists and author of dozens of successful books, both fiction and nonfiction, offers a revealing and charming account of his life and work. Mathematician, physicist, astronomer, cosmologist - Sir Fred is perhaps best known, in scientific circles, for his brilliant explanation of the origin of the elements from hydrogen nuclei in stars (a process known as nucleosynthesis) and for developing (with Sir Hermann Bondi and Thomas Gold) the elegant but controversial steady-state theory of the Universe (which assumes the continuous creation of matter). In 1950, in the last of a series of radio lectures on astrono...
Proceedings of Symposium No. 47 organized by the IAU held in Newcastle upon Tyne, England, March 22-26, 1971
The British Expeditionary Force at the start of World War I was tiny by the standards of the other belligerent powers. Yet, when deployed to France in 1914, it prevailed against the German army because of its professionalism and tactical skill, strengths developed through hard lessons learned a dozen years earlier. In October 1899, the British went to war against the South African Boer republics of Transvaal and Orange Free State, expecting little resistance. A string of early defeats in the Boer War shook the military’s confidence. Historian Spencer Jones focuses on this bitter combat experience in From Boer War to World War, showing how it crucially shaped the British Army’s tactical d...
This book is the latest volume of Spencer Jones's award-winning series which examines the British Army on the Western Front year-by-year.
The past decade has seen a considerable surge of interest in historical and philo sophical studies of gravitation and relativity, due not only to the tremendous amount of world-wide research in general relativity and its theoretical and observational consequences, but also to an increasing awareness that a collaboration between working scientists, historians and philosophers of science is, in this field, partic ularly promising for all participants. The expanding activity in this field is well documented by recent volumes in this Einstein Studies series on the History of General Relativity as well as by a series of international conferences on this topic at Osgood Hill (1986), Luminy (1988),...
As one of the oldest scientific institutions in the United States, the US Naval Observatory has a rich and colourful history. This volume is, first and foremost, a story of the relations between space, time and navigation, from the rise of the chronometer in the United States to the Global Positioning System of satellites, for which the Naval Observatory provides the time to a billionth of a second per day. It is a story of the history of technology, in the form of telescopes, lenses, detectors, calculators, clocks and computers over 170 years. It describes how one scientific institution under government and military patronage has contributed, through all the vagaries of history, to almost two centuries of unparalleled progress in astronomy. Sky and Ocean Joined will appeal to historians of science, technology, scientific institutions and American science, as well as astronomers, meteorologists and physicists.
This book, in three parts, describes three phases in the development of the modern theory and calculation of the Moon's motion. Part I explains the crisis in lunar theory in the 1870s that led G.W. Hill to lay a new foundation for an analytic solution, a preliminary orbit he called the "variational curve." Part II is devoted to E.W. Brown's completion of the new theory as a series of successive perturbations of Hill's variational curve. Part III describes the revolutionary developments in time-measurement and the determination of Earth-Moon and Earth-planet distances that led to the replacement of the Hill–Brown theory in 1984.