Presented for the first time in popular form is the fascinating true story of the search for the phantom planet Vulcan. As with legends of "the lost continent of Atlantis," scientists and dreamers alike have sought to prove that Vulcan is more than just a myth. Historians of astronomy Richard Baum and William Sheehan have combed the continents, digging through dusty letters and journals, to unravel this mysterious and captivating tale. The planet first assumed a shadowy reality against a backdrop of war and revolution early in the nineteenth century. Le Verrier, the autocratic Director of the Paris Observatory, had unveiled a problem with the motion of the planet Mercury. The indications were of a planet closer to the sun than Mercury. Incredibly, the prediction was immediately fulfilled by an obscure French country doctor using no more than a homemade telescope. The planet, named for the Roman god of fire, was no sooner discovered than it was lost. Still it reappeared often enough to tantalize even skeptics into considering its shadowy existence possible. This fast-paced tale follows the exploits of Le Verrier, and later of his followers, in a pursuit of his unbridled obsessions: to extend the universality of Newton's Laws, to prove Vulcan's existence, and to secure his place in history as one of the greatest astronomers of his time. Stranger than fiction, the story reaches an exciting climax in the final showdown in the unlikeliest of places: America's Wild West. Like gunslingers at high noon, determined astronomers of the opposing camps brave Indians and the elements in their attempt to prove once and for all whether the planet exists. They congregate with some of the most illustrious names of their time for the final test: a grand eclipse of the sun.

Expanding upon the ideas first proposed in his seminal book Cosmical Magnetic Fields, Eugene N. Parker here offers the first in-depth treatment of the magnetohydrodynamic theory of spontaneous magnetic discontinuities. In detailing his theory of the spontaneous formation of tangential discontinuities (current sheets) in a magnetic field embedded in highly conducting plasma, Parker shows how it can be used to explain the activity of the external magnetic fields of planets, stars, interstellar gas clouds, and galaxies, as well as the magnetic fields in laboratory plasmas. Provocative and fascinating, Spontaneous Current Sheets in Magnetic Fields presents a bold new theory that will excite interest and discussion throughout the space physics community.

'The first two editions of this textbook have received well-deserved high acclaims, and this - the third edition - deserves no less. Its explanations of the whole gamut of atomic and molecular spectroscopy provide a solid grasp of the theory as well as how to understand such spectra in practice. It thus makes an ideal companion to books that start from the observational aspect of spectroscopy, whether in the lab or at the telescope ... This new edition of TennysonaEURO (TM)s book ought to be in the library of every astronomical department.'The Observatory Magazine'It closely follows the course given to third year UCL undergraduates, and the worked examples have surely been tested on students ... The last two chapters serve as an effective appendix on more specialised topics in atomic and molecular theory.'Contemporary PhysicsThe third edition of Astronomical Spectroscopy examines the physics necessary to understand and interpret astronomical spectra. It offers a step-by-step guide to the atomic and molecular physics involved in providing astronomical spectra starting from the relatively simple hydrogen atom and working its way to the spectroscopy of small molecules.Based on UCL course material, this book uses actual astronomical spectra to illustrate the theoretical aspects of the book to give the reader a feel for such spectra as well as an awareness of what information can be retrieved from them. It also provides comprehensive exercises, with answers given, to aid understanding.

The search for life in the universe, once the stuff of science fiction, is now a robust worldwide research program with a well-defined roadmap probing both scientific and societal issues. This volume examines the humanistic aspects of astrobiology, systematically discussing the approaches, critical issues, and implications of discovering life beyond Earth. What do the concepts of life and intelligence, culture and civilization, technology and communication mean in a cosmic context? What are the theological and philosophical implications if we find life - and if we do not? Steven J. Dick argues that given recent scientific findings, the discovery of life in some form beyond Earth is likely and so we need to study the possible impacts of such a discovery and formulate policies to deal with them. The remarkable and often surprising results are presented here in a form accessible to disciplines across the sciences, social sciences, and humanities.

This concise textbook, the first volume in the Ohio State Astrophysics Series, covers all aspects of the interstellar and intergalactic medium for graduate students and advanced undergraduates. This series aims to impart the essential knowledge on a topic that every astrophysics graduate student should know, without going into encyclopedic depth. This text includes a full discussion of the circumgalactic medium, which bridges the space between the interstellar and intergalactic gas, and the hot intracluster gas that fills clusters of galaxies. Its breadth of coverage is innovative, as most current textbooks treat the interstellar medium in isolation. The authors emphasise an order-of-magnitude understanding of the physical processes that heat and cool the low-density gas in the universe, as well as the processes of ionization, recombination, and molecule formation. Problems at the end of each chapter are supplemented by online projects, data sets and other resources.

This textbook on the nature of space and time explains the new theory of Space Dynamics, which describes the dynamics of gravity as the evolution of conformal 3-dimensional geometry. Shape Dynamics is equivalent to Einstein's General Relativity in those situations in which the latter has been tested experimentally, but the theory is based on different first principles. It differs from General Relativity in certain extreme conditions. Shape Dynamics allows us to describe situations in which the spacetime picture is no longer adequate, such as in the presence of singularities, when the idealization of infinitesimal rods measuring scales and infinitesimal clocks measuring proper time fails. This tutorial book contains both a quick introduction for readers curious about Shape Dynamics, and a detailed walk-through of the historical and conceptual motivations for the theory, its logical development from first principles and a description of its present status. It includes an explanation of the origin of the theory, starting from problems posed first by Newton more than 300 years ago. The book will interest scientists from a large community including all foundational fields of physics, from quantum gravity to cosmology and quantum foundations, as well as researchers interested in foundations. The tutorial is sufficiently self-contained for students with some basic background in Lagrangian/Hamiltonian mechanics and General Relativity.

This is one of the most important studies in decades on Johannes Kepler, among the towering figures in the history of astronomy. Drawing extensively on Kepler's correspondence and manuscripts, James Voelkel reveals that the strikingly unusual style of Kepler's magnum opus, "Astronomia nova" (1609), has been traditionally misinterpreted. Kepler laid forth the first two of his three laws of planetary motion in this work. Instead of a straightforward presentation of his results, however, he led readers on a wild goose chase, recounting the many errors and false starts he had experienced. This had long been deemed a ''confessional'' mirror of the daunting technical obstacles Kepler faced. As Voelkel amply demonstrates, it is not.

Voelkel argues that Kepler's style can be understood only in the context of the circumstances in which the book was written. Starting with Kepler's earliest writings, he traces the development of the astronomer's ideas of how the planets were moved by a force from the sun and how this could be expressed mathematically. And he shows how Kepler's once broader research program was diverted to a detailed examination of the motion of Mars. Above all, Voelkel shows that Kepler was well aware of the harsh reception his work would receive--both from Tycho Brahe's heirs and from contemporary astronomers; and how this led him to an avowedly rhetorical pseudo-historical presentation of his results. In treating Kepler at last as a figure in time and not as independent of it, this work will be welcomed by historians of science, astronomers, and historians.

Discover how mathematics and science have propelled history

From Ancient Greece to the Enlightenment and then on to modern times, Shifting the Earth: The Mathematical Quest to Understand the Motion of the Universe takes readers on a journey motivated by the desire to understand the universe and the motion of the heavens. The author presents a thought-provoking depiction of the sociopolitical environment in which some of the most prominent scientists in history lived and then provides a mathematical account of their contributions.

From Eudoxus to Einstein, this fascinating book describes how, beginning in ancient times, pioneers in the sciences and mathematics have dramatically changed our vision of who we are as well as our place in the universe. Readers will discover how Ptolemy's geocentric model evolved into Kepler's heliocentric model, with Copernicus as the critical intermediary. The author explains how one scientific breakthrough set the stage for the next one, and he also places the scientists and their discoveries within the context of history, including:

Archimedes, Apollonius, and the Punic Wars

Ptolemy and the rise of Christianity

Copernicus and the Renaissance

Kepler and the Counter-Reformation

Newton and the Enlightenment

Einstein and the detonation of the atom bomb

Each chapter presents the work of a single scientist or mathematician, building on the previous chapters to demonstrate the evolutionary process of discovery. Chapters begin with a narrative section and conclude with a mathematical presentation of one of the scientist's original works. Most of these mathematical presentations, including the section on Einstein's special relativity, are accessible using only basic mathematics; however, readers can skip the mathematical sections and still follow the evolution of science and mathematics.

Shifting the Earth is an excellent book for anyone interested in the history of mathematics and how the quest to understand the motion of the heavens has influenced the broader history of humankind.

'The first two editions of this textbook have received well-deserved high acclaims, and this - the third edition - deserves no less. Its explanations of the whole gamut of atomic and molecular spectroscopy provide a solid grasp of the theory as well as how to understand such spectra in practice. It thus makes an ideal companion to books that start from the observational aspect of spectroscopy, whether in the lab or at the telescope ... This new edition of TennysonaEURO (TM)s book ought to be in the library of every astronomical department.'The Observatory Magazine'It closely follows the course given to third year UCL undergraduates, and the worked examples have surely been tested on students ... The last two chapters serve as an effective appendix on more specialised topics in atomic and molecular theory.'Contemporary PhysicsThe third edition of Astronomical Spectroscopy examines the physics necessary to understand and interpret astronomical spectra. It offers a step-by-step guide to the atomic and molecular physics involved in providing astronomical spectra starting from the relatively simple hydrogen atom and working its way to the spectroscopy of small molecules.Based on UCL course material, this book uses actual astronomical spectra to illustrate the theoretical aspects of the book to give the reader a feel for such spectra as well as an awareness of what information can be retrieved from them. It also provides comprehensive exercises, with answers given, to aid understanding.

Die Funktechnik ermoeglicht die Ausweitung der astronomischen Beobachtungen uber das Licht hinaus auf andere Frequenzbereiche. Dies fuhrte zur Entdeckung zahlreicher kosmischer Radioquellen, deren physikalische Ursachen erlautert werden, ebenso die Funktionsweise eines Radioteleskops. Schon mit kleinen Radioteleskopen kann die Strahlung der Sonne und anderer Radioquellen sowie die 21-cm-Strahlung aus der Milchstrasse beobachtet werden. Durch Interferometrie kann eine wesentlich hoehere Aufloesung als mit einzelnen Radioteleskopen erzielt werden. Dadurch kann die radioastronomische Forschung zu vielen aktuellen Fragen der Astronomie, Kosmologie und Physik beitragen.

This book provides an extensive survey of all the physics necessary to understand the current developments in the field of fundamental cosmology, as well as an overview of the observational data and methods. It will help students to get into research by providing definitions and main techniques and ideas discussed today. The book is divided into three parts. Part 1 summarises the fundamentals in theoretical physics needed in cosmology (general relativity, field theory, particle physics). Part 2 describes the standard model of cosmology and includes cosmological solutions of Einstein equations, the hot big bang model, cosmological perturbation theory, cosmic microwave background anisotropies, lensing and evidence for dark matter, and inflation. Part 3 describes extensions of this model and opens up current research in the field: scalar-tensor theories, supersymmetry, the cosmological constant problem and acceleration of the universe, topology of the universe, grand unification and baryogenesis, topological defects and phase transitions, string inspired cosmology including branes and the latest developments. The book provides details of all derivations and leads the student up to the level of research articles.

This book describes the basic concepts of supersymmetric theories. It is aimed at theorists, experimentalists and cosmologists interested in supersymmetry, and its content is correspondingly divided into three distinct tracks of study. The topics covered include a discussion of the motivation for supersymmetry in fundamental physics, a description of the minimal supersymmetric model as well as models of grand unification and string models, a presentation of the main scenarios for supersymmetry breaking, including the concepts and results of dynamical breaking. On the astrophysics/cosmology side, the book includes discussions of supersymmetric dark matter candidates, inflation, dark energy, and the cosmological constant problem. Some very basic knowledge of quantum field theory is needed and extensive appendices (in particular an introduction to the Standard Model of fundamental interactions) allow the reader to refresh and complete their notions.

The problem of motion of extended bodies in General Relativity is notorious for its analytical difficulty, but at the same time highly relevant for comparison of theoretical predictions with modern precision measurements in relativistic astrophysics and cosmology. Its one of the most important topics in General Relativity and its application to astrophysics.
Equations of Motion in General Relativity focuses attention on two aspects of equations of motion in general relativity: the motion of extended bodies (stars) and the motion of small black holes. The objective is to offer a guide to prospective researchers into these areas of general relativity and to point out open questions and topics that are ripe for further development. It is over forty years since a text on this subject was published and in that time the research area of equations of motion in general relativity has undergone extraordinary development, stimulated by the discovery of the binary neutron star PSR 1913+16 in 1974 (which was the first isolated gravitating system found in which general relativity plays a fundamental role in describing theoretically its evolution), and more recently by the advent of kilometre size interferometric gravitational wave detectors which are expected to detect gravitational waves produced by coalescing binary neutron stars.

The field of astrophysics is in the midst of a technologically driven renaissance, as fundamental discoveries are being made with astonishing frequency. In the last decade, new detectors in space, on earth, and deep underground have, when coupled with the computational power of modern computers, revolutionized our knowledge and understanding of the astronomical world. This is a great time for a student of any age to become acquainted with the remarkable universe in which we live. This volume is a collection of essays, originally presented orally to a diverse group of students and professionals, which reveal the most fertile areas for future study of astronomy and astrophysics. The emphasis of this work is on the clear description of the current state of our knowledge as a preparation for the future unraveling of the mysteries of the universe that appear today as most fundamental and most amenable to solution.

A stellar group of astronomers and astrophysicists describes the directions and styles of work that they think are most likely to lead to progress. Bibliographical notes at the end of each presentation provide guidance for the reader who wishes to go more deeply into a given subject. "Unsolved Problems in Astrophysics" is a uniquely stimulating introduction to some of the most important topics in modern astrophysics.

Take a trip to outer space with this weird and wonderful guide to our universe, the perfect gift for both young and old Vargic's beautifully innovative designs will help to explain all of the bizarre and fascinating aspects of the cosmos; from the history of the universe to what makes up our solar system and even how human life fits into the wider picture. Be taken on an unforgettable journey through space with chapters on . . . * Exploring the Cosmos * The Night Sky * Maps of the Inner Solar System * Timeline of the Universe * Cosmologies throughout History * Journey Into Outer Space * Scale of the Universe This is a book that celebrates the scale and spectacle of the universe on every page, and one which you'll treasure forever. _______ '5***** In more than one hundred pages filled with facts and illustrations he takes the reader on a journey through the history of the cosmos' BBC Sky at Night 'Packs in so much of our astronomical knowledge, so many tidbits about the history of astronomy and space exploration that I felt wonderfully enriched by it all. It is visually striking and beautifully illustrated' Dr. Alfredo Carpineti

"Almost fifty years after the beginning of space flight, Belbruno's work offers a realistic beginning for minimum--fuel and maximum--payload trajectories for interplanetary operations. It is a mark of sophistication in the evolution of space travel that simplified solutions to the vexing many-body problem are found to have practical applications. Belbruno's three-body solution for low-thrust minimum-fuel trajectories serves well not only the future of space flight but helps astronomy in understanding the sometimes erratic motions of celestial bodies."--Edgar D. Mitchell, Apollo 14 astronaut

""Fly Me to the Moon" is a fast, easy read that explains in simple nonscientific terms very complex matters of celestial mechanics, and it is delightful reading for students and professionals to update or learn very important new background materials. It is also a must-read for the lawyer-scientist."--Ambassador Edward R. Finch, Jr.

"This is an excellent book. The author succeeds in writing an exciting story about his research on low-fuel space travel, a subject that is not widely known but that will interest many readers. Moreover, the mathematical aspects of chaos in the context of space missions is well treated at the level of the nonexpert."--Florin Diacu, University of Victoria

"This is a good story. It is rare to see a nonpedantic book on celestial mechanics that gives some backroom stories about trajectory geeks. Belbruno ties very abstract concepts to real problems and situations."--Wendell W. Mendell, NASA Johnson Space Center, Astromaterials Research & Exploration Science Directorate

"This is an excellent book. It is an inside look at the important new field of chaotictrajectories by one of the masters and originators of the field. As we continue into space, I think we will be hearing more and more about these clever trajectories. Ed Belbruno has covered in a beautiful and interesting way the important applications of chaos to astrophysics and spacecraft trajectories. He also tells a very interesting personal story of his battles to get these trajectories used, and how he was able to save the Hiten spacecraft and get it to the moon. This is a great story, and he tells it very well."--Richard Gott, Princeton University

"The author's newly discovered interplanetary highways offer a romantic reflection of the pre-rocket, pre-airplane era, where balloons would transport us, with hardly any energy of our own, from one unexplored vista to another."--From the foreword by Neil deGrasse Tyson, astrophysicist and Director of the Hayden Planetarium, American Museum of Natural History, author of "Death by Black Hole: And Other Cosmic Quandaries"

Jonas Pohl liefert eine didaktisch aufbereitete Einfuhrung in die Gedankenwelt der Allgemeinen Relativitatstheorie. Er gibt einen Einblick in die Grundlagen von 100 Jahren Relativitatstheorie und spannt dabei den Bogen von der Speziellen Relativitatstheorie im Jahr 1905 bis hin zum aktuellsten Ereignis, der Entdeckung der Gravitationswellen im Fruhjahr 2015. Der Autor bietet damit besonders Studierenden des Lehramts die Moeglichkeit, die Essenz der Allgemeinen Relativitatstheorie in verstandlicher und nachvollziehbarer Weise zu erfassen.

This book is an introduction to the theory of supersymmetry, which is a cornerstone to understanding the physics of elementary particles beyond the so-called "Standard Model". Supersymmetry is the first introductory book on this modern and increasingly popular subject.

Jurgen Beetz zeigt zuerst den Ursprung der erdachten Geschichten der Physik aus der Steinzeit, denn vieles ist so einfach, dass es schon Steinzeitmenschen hatten verstehen koennen. Im Anschluss daran untersucht der Autor das Weltall auf seine Bestandteile: Monde, Planeten, Sterne, Galaxien usw. Daraus ergibt sich die Frage nach dessen Struktur und Dynamik: Ist das Universum ewig, endlos, konstant? Nichts davon: Es hat eine Entstehungsgeschichte, es expandiert und verandert sich - zum Teil aus noch ungeklarten Ursachen. Besonderes Augenmerk richtet er auf die Expansion des Weltalls und die sich daraus ergebenden Folgen.

Der neue Kosmos bietet in uberschaubarem Umfang eine zusammenhangende Einfuhrung in das Gesamtgebiet der Astronomie und Astrophysik. Der korrigierte und erweiterte Nachdruck tragt dem rasanten Fortschritt der astronomischen Forschung und Beobachtungsmoeglichkeiten in den zwei Jahren seit dem ersten Erscheinen der 7. Auflage Rechnung. Die wichtigsten neuen Ergebnisse, vor allem bei unserem Planetensystem, bei der Neutrinostrahlung der Sonne, bei den fernsten Galaxien und Quasaren sowie bei der Entwicklung des Universums werden berucksichtigt.

Astronomy and Astrophysics Abstracts, which has appeared in semi-annual volumes since 1969, is de- voted to the recording, summarizing and indexing of astronomical publications throughout the world. It is prepared under the auspices of the International Astronomical Union (according to a resolution adopted at the 14th General Assembly in 1970). Astronomy and Astrophysics Abstracts aims to present a comprehensive documentation of Iiterature in all fie1ds of astronomy and astrophysics. Every effort will be made to ensure that the average time interval between the date of receipt of the original Iiterature and publication of the abstracts will not exceed eight months. This time interval is near to that achieved by monthly abstracting journals, com- pared to which our system of accumulating abstracts for about six months offers the advantage of greater convenience for the user. Volume 10 contains Iiterature published in 1973 and received before March 15, 1974; some older Iiterature which was received late and which is not recorded in earlier vo1umes is also included. We acknowledge with thanks contributions to this volume by Dr. J. BouSka, who surveyed journals and publications in the Czech language and supplied us with abstracts in English, and by the Common- wealth Scientific and Industrial Research Organization (C.S.I.R.O.), Sydney, for providing titles and abstracts of papers on radio astronomy.

VII ubernommen habe. Mein eigenes Interesse fur Galaxien ist vor allem in Diskussionen mit Donald Lynden-Bell, Bernard Pagel und Martin Rees geweckt worden. Ich will meinen Dank gegenuber Douglas Meyer bekunden, der wiederum die Diagramme gezeichnet hat, und gegenuber Frau Peggy Nixon fur das sorgfaltige Schreiben des Manuskripts. Ebenso bin ich wiederum meinem Mitarbeiter Alan Everest zu Dank verpflichtet, der zahlreiche Vorschlage zum Text gemacht hat. Ich widme dieses Buch in Respekt und Bewunderung Herrn Professor Jan H. Oort, der nun schon seit uber 50 Jahren fundamentale Beitrage zur Aufklarung der galaktischen Struktur geliefert hat. Lewes, im Februar 1978 R. ]. Tayler Vorwort zur deutschen ubersetzung Obgleich zu den in diesem Buch behandelten Themen in den letzten 6 Jahren eine Fulle von Einzelarbeiten in der Literatur erschienen sind, wurde davon abgesehen, den Text im Rahmen der ubersetzung zu uber- arbeiten, weil die Diskussion einzelner hier behandelter Fragestellungen in vollem Gange ist und gesicherte Endergebnisse noch keineswegs vor- liegen. Es wurde aber der Absicht dieses Buches, das eine allgemein- verstandliche Einfuhrung in die Thematik geben will, widersprechen, wenn neuere, zum Teil kontroverse Einzelarbeiten besonders hervor- gehoben wurden. Der einzige groessere Eingriff in die Textgestaltung, der vorgenommen wurde, betrifft das Kapitel4 Stellardynamik, das geteilt wurde und sich jetzt teilweise im Anhang 2 befindet. Ferner wurde ein Teil der Abbildungen uberarbeitet bzw. neu gestaltet. Tubingen, im Mai 1985 M.

Described by one reviewer as 'one of the most perfect books ever written on theoretical astronomy', this work in Latin by the German mathematician Carl Friedrich Gauss (1777 1855), the 'Prince of Mathematicians', derived from his attempt to solve an astronomical puzzle: where in the heavens would the dwarf planet Ceres, first sighted in 1801, reappear? Gauss' predicted position was correct to within half a degree, and this led him to develop a streamlined and sophisticated method of calculating the effect of the larger planets and the sun on the orbits of planetoids, which he published in 1809. As well as providing a tool for astronomers, Gauss' method also offered a way of reducing inaccuracy of calculations arising from measurement error; the primacy of this discovery was however disputed between him and the French mathematician Legendre, whose Essai sur la th orie des nombres is also reissued in this series.