The genesis of modern searches for observable meteoritic phenomena on the Moon is the paper by Lincoln La Paz in Popular Astronomy magazine in 1938. In it he argued that the absence of observed fashes of meteoritic impacts on the Moon might be interpreted to mean that these bodies are destroyed as luminous meteors in an extremely rarefed lunar atmosphere. The paper suggested the possibility of systematic searches for such possible lunar meteors. With these concepts in mind, I was surprised to note a transient moving bright speck on the Moon on July 10, 1941. It appeared to behave very much as a lunar meteor would - except that the poorly estimated duration would lead to a strongly hyperbolic heliocentric velocity. Thus, the idea of systematic searches for both p- sible lunar meteors and meteoritic impact fashes was born. It was appreciated that much time might need to be expended to achieve any positive results. Systematic searches were carried out by others and myself chiefy in the years 1945-1965 and became a regular program at the newly founded Association of Lunar and Planetary Observers, or ALPO.

Including the abundance of information known prior to the return of Halley's comet, as well as the new information discovered since then, the science of comets is described here by order of its discovery. From tail phenomena to coma morphology, to the most recent findings from space missions, this comprehensive text provides complete and up-to-date coverage of the subject. It will be suitable for advanced undergraduates and graduate students of astronomy and planetary science. First Edition Hb (2001): 0-521-23906-0 First Edition Pb (2002): 0-521-27218-1

Discs occur in a wide variety of astronomical contexts, ranging in size from planetary ring systems to galaxies. Because the dynamical problems posed by each type of disc are remarkably similar, the Astronomy Department of the University of Manchester decided to bring together experts in each area for a conference in December 1988. This book is a collection of the papers presented at the conference. It contains mainly review papers covering recent developments in both theory and observations of planetary ring systems, discs in star-forming regions, protoplanetary discs, accretion discs and galaxy discs presented by an expert in each field. The book also gives brief summaries of contributed papers outlining current research by many of the participants.

Almost thirty years after the Apollo missions, "Tranquillity Base," "Hadley Rille," or "Taurus-Littrow" are names still resonant with the enormous achievements represented by the lunar landings. But how did these places get their names? Who named Copernicus crater? Where did all those names on lunar maps come from, and what stimulated their selection? Ewen Whitaker traces the origins and evolution of the present-day systems for naming lunar features such as craters, mountains, valleys and dark spots. The connections between the prehistoric and historic names, and today's gazetteer are clearly described. Beautiful lunar maps spanning four centuries of progress wonderfully illustrate the unfolding of our ability to map the Moon. Rare, early photographs add to the sense of history. Comprehensive appendices and the bibliography make this delightful book a work of lasting reference and scholarship.

Volume 2 of the four-volume catalog of comets observed throughout history provides a complete summary of every comet seen during the nineteenth century. It includes details of discovery, closest approaches to the Sun and Earth, path across the sky, physical descriptions, orbital information, and final observations. The catalog provides amateur and professional astronomers, and historians of science, with a definitive reference on comets through the ages. Also available: Volume 1: Ancient-1799 1999 0-521-58504-X $95.00 C

Instead of taking somebody's word for it about the basic size and distance statistics for the solar system, this book shows amateur astronomers how to measure these things for themselves. This is an enriching experience for any amateur astronomer - to understand and personally measure some fundamental astronomical quantities and distances.

A basic knowledge of geometry is required, but it is amazing how simple the geometry can be. Readers are led through the geometry as gently as possible - and in a light-hearted way - presuming that most non-academics will have half-forgotten most of their mathematics.

The practical astronomical equipment recommended is no more than a typical commercially-made amateur telescope and a camera of some sort - these days a webcam works very well. Apart from that all the reader will need is access to a computer, the know-how to download free software, and an enthusiasm to expand his knowledge of the basis of scientific astronomy.

Harold Hill's book is a unique collection of drawings published for the first time in this form. The illustrations are supplemented by text often taken from observing notes at the telescope. Astronomical drawing still has an important place alongside photography in the same way that photography has not supplanted the artist in the field of botany and ornithology. Indeed, because of movements in the Earth's atmosphere, astronomical images tend to shimmer even under the best possible conditions; drawings constructed by an artist who takes advantage of the fleeting moments of perfect vision are often more detailed than photographs. No one can fail to be impressed by the beauty and artistry of this work and, for the initiated, the accuracy and attention to detail is remarkable.

This is the ultimate, easy-to-read guide for "eclipse-chasers" which includes everything an eclipse chaser needs. There are some important eclipses coming up in the years ahead and the technology available to amateur astronomers is improving fast. The book provides "eclipse virgins" with a good feeling for what a trip abroad to an eclipse is like including a humorous look at all the things that can and have gone wrong. Travel details are included, essential in these days of high-security. And of course the first part of the book contains a wealth of information about solar eclipses and what can be observed only during a total eclipse.

Babylon to Voyager and Beyond describes the fascinating story of planetary research from the time of the Babylonians and Ancient Greeks to the modern age of space exploration. In it, David Leverington outlines the key astronomical discoveries in their historical context, covering not only the successes but also the main failures. Babylon to Voyager and Beyond is written to be accessible to both amateur and professional astronomers, and those interested in the history of science. Extensively illustrated, the book concludes with a description of the extensive planetary discoveries made by spacecraft, and the discoveries of planets around other stars.

David Levy has held a lifelong passion for comets, and is one of the most successful comet discoverers in history. In this book he describes the observing techniques that have been developed over the years--from visual observations and searching, to photography, through to electronic charge-coupled devices (CCDs). He combines the history of comet hunting with the latest techniques, showing how our understanding of comets has evolved over time. This practical handbook is suitable for amateur astronomers, from those who are casually interested in comets and how to observe them, to those who want to begin and expand an observing program of their own. Drawing widely from his own extensive experience, Levy describes how enthusiastic amateurs can observe comets and try to make new discoveries themselves. David H. Levy is one of the word's foremost amateur astronomers. He has discovered seventeen comets, seven using a telescope in his own backyard, and had a minor planet, Asteroid 3673 Levy named in his honor. He is best known as the co-discoverer of the famous 1994 Shoemaker-Levy 9 comet. Levy is frequently interviewed in the media and succeeded Carl Sagan as science columnist for Parade magazine. He has written and contributed to a number of books, most recently David Levy's Guide to the Night Sky (Cambridge, 2001).

Since the discovery of the first exoplanet orbiting a main sequence star in 1995, nearly 500 planets have been detected, with this number expected to increase dramatically as new ground-based planetary searches begin to report their results. Emerging techniques offer the tantalizing possibility of detecting an Earth-mass planet in the habitable zone of a solar-type star as well as the exciting prospect of studying exoplanetary atmospheres that could reveal the presence of biomarkers, such as water vapor, oxygen, and carbon dioxide. Can we find the "Holy Grail" of exoplanets? Cutting-edge research may reveal the answer Written by internationally renowned scientists at the forefront of the field, Extra-Solar Planets: The Detection, Formation, Evolution and Dynamics of Planetary Systems presents powerful analytical tools and methods for investigating extra-solar planetary systems. It discusses new theories on planetary migration and resonant capture that elucidate the existence of "hot Jupiters." It also examines the astrophysical mechanisms required to assemble gas giant planets close to their parent star. In addition, the expert contributors describe how mathematical tools involving periodicity, chaos, and resonance are used to study the diversity and stability of observed planetary systems. By presenting the fundamental analyses that underpin modern studies of extra-solar planetary systems, this graduate-level book enables readers to thoroughly understand important recent developments and offers a platform for future research. It also improves readers' understanding of our own solar system and its place in the diverse range of planetary systems discovered so far.

This book integrates astronomical observations and theories with geophysical studies, presenting a comprehensive overview of the extraterrestrial matter that falls to Earth from space. Meteoroids are the main topic of the book, although cosmic dust, interplanetary matter and meteorites are also discussed. This work is of great value to researchers involved in the study of meteor phenomena.

Jupiter’s magnetosphere (the region of space in which Jupiter’s magnetic field influences the motion of charged particles) is the largest object in the solar system; it exhibits new phenomena and behaves, in some respects, like a pulsar. It is a magnetosphere whose physics is dominated by internal sources of plasma and energy. This book consists of twelve carefully interwoven articles written by leading space scientists who summarize our state of knowledge of the physics of the magnetosphere surrounding the planet Jupiter. Ground-based data as well as information from the Pioneer and Voyager spacecraft are used in developing both physical descriptions and theoretical understanding. Physics of the Jovian Magnetosphere is a valuable reference work for those doing research in magnetospheric physics and in a number of related disciplines.

This introduction to the use of radar for remote sensing of natural surfaces provides the reader with a thorough grounding in practical applications, focusing particularly on terrestrial studies that may be extended to other planets. An historical overview of the subject is followed by an introduction to the nomenclature and methodology pertaining to radar data collection, image interpretation and surface roughness analysis. The author presents a summary (illustrated with examples from the natural environment) of theoretical explanations for the backscatter properties of continuous rough surfaces, collections of discrete objects, and layered terrain.

Canadian academic Martin Beech has written a text that attempts to cross the line between science fiction and science fact. Put simply, his book details a method that just might be able to stop the Sun from losing its power and, ultimately, save humanity and the Earth itself. It investigates the idea that the distant future evolution of our Sun might be controlled (or 'asteroengineered') so that it maintains its present-day energy output rather than becoming a bloated red giant star: a process that would destroy all life on Earth.

*Brings the story of the Cassini-Huygens mission and their joint exploration of the Saturnian system right up to date.

*Combines a review of previous knowledge of Saturn, its rings and moons, including Titan, with new spacecraft results in one handy volume.

*Provides the latest and most spectacular images, which will never have appeared before in book form.

*Gives a context to enable the reader to more easily appreciate the stream of discoveries that will be made by the Cassini-Huygens mission.

*Tells the exciting story of the Huygens spacecraft 's journey to the surface of Titan.

Our space age technology enables global communication, navigation, and power distribution that has given rise to our 'smart', interconnected and spacefaring world. Much of the infrastructure modern society depends on, to live on Earth and to explore space, is susceptible to space weather storms originating from the Sun. The Second Edition of this introductory textbook is expanded to reflect our increased understanding from more than a dozen scientific missions over the past decade. Updates include discussions of the rapidly expanding commercial space sector, orbital debris and collision hazards, our understanding of solar-terrestrial connections to climate, and the renewed emphasis of human exploration of the Moon and Mars. It provides new learning features to help students understand the science and solve meaningful problems, including some based on real-world data. Each chapter includes learning objectives and supplements that provide descriptions of the science and learning strategies to help students and instructors alike.

MARSWALK ONE: First Steps on a New Planet addresses the question of why we should embark on a journey to Mars, documenting what the first human crew will do when they place their feet in the red dust of the planet. The book also addresses why we need to carry out these tasks and, more importantly, what a human crew could achieve that an automated mission could not. Understanding the clear benefits of sending a human crew to the surface of Mars, and how these benefits can be seen back on Earth, is the key to sustained long-term public and political support for the programme in terms of cash and commitment.

The book accepts that the journey will be made, but does not specify precisely when. Flight time, and how to get to and from the planet are discussed briefly, to understand why the suggested duration spent at Mars is reasonable.

The main objective of the work is to look at what science will be done on the surface a" supported by orbital operations a" and what hardware and technology will be employed to achieve the mission objectives. This analysis is drawn from previous experiences in manned and unmanned space programmes, including Apollo, Skylab, Salyut/Mir, Shuttle and ISS, Viking, Luna/Lunokhod, and recent Mars missions such as Pathfinder and Global Surveyor.

In addition, new interviews with key personalities involved in planning Martian exploration, and discussions about current thoughts on what we need to accomplish on Mars when we get there, will provide a lively and thought provoking account that could generate fresh debate.

When the decision is finally made to go to Mars, it will be made in the knowledge that most of the world knows why we aregoing and what benefits mankind will see for the effort. The authorsa (TM) primary objective is to begin this understanding.

The force of gravity acting over eons has provided the solar system with an intricate dynamical structure, much of it revealed by recent space missions. This comprehensive introduction to the dynamical features of the solar system also provides all the mathematical tools and physical models needed for a complete understanding of the subject. Clearly written and well illustrated coverage shows how a basic knowledge of the two- and three-body problems and perturbation theory can be combined to understand features as diverse as the tidal heating of Jupiter's moon Io, the origin of the Kirkwood gaps in the asteroid belt, and the radial structure of Saturn's rings. Problems at the end of each chapter and a free Internet Mathematica® software package help students to fully develop their understanding of the subject. This volume provides an authoritative textbook for advanced undergraduate and graduate courses on planetary dynamics and celestial mechanics. It also equips students with the mathematical tools to tackle broader courses on dynamics, dynamical systems, applications of chaos theory and nonlinear dynamics. Written by two leading figures in planetary dynamics, it is a benchmark publication in the field and destined to become a classic.

Following the 'Big Bang', it took the universe billions of years to evolve into the unique system of stars and planets that we know of today. Scientists have studied the planets of our solar system for centuries, and are beginning to understand the billions of stars and other bodies that make up the Universe. Stars and Planets is an ideal reference book for anyone interested in astronomy, featuring 300 of the most well known stars, planets, moons, constellations and other cosmological phenomena, such as black holes and quasars. Each entry includes an image - either a photograph or an artist's impression or diagram - and a key information table including specifications such as the mass, radius, surface temperature, distance from sun, gravity and major elements of each object. Presented in a handy, pocket-size format, full of facts and engaging text, Stars and Planets is a valuable reference source as well as a fascinating read, revealing the spectacular world of the Cosmos.

Cometography is the most complete and comprehensive collection of data on comets available. It comes in four self-contained sequential volumes and this, the first, covers ancient times through to the end of the eighteenth century. Cometography uses the most reliable orbits known to determine all the key parameters of each well observed comet. Cometography also provides nontechnical details to help the reader understand how the comet may have influenced various cultures at the time of its appearance. All the information in Cometography has been sourced directly from the original documents, including European monastic histories, Roman, Greek and Muslim texts, Chinese, Japanese and Korean scripts. In many cases, dates of important historical events can be corrected based on the appearance of a comet and identified using this book. Cometography will be valuable to historians of science as well as providing amateur and professional astronomers with a definitive reference on comets through the ages.

Meteorites and Their Parent Planets provides an engrossing overview of a highly interdisciplinary field--the study of extraterrestrial materials. The second edition of this successful book has been thoroughly revised, and describes the nature of meteorites, where they come from, and how they get to Earth. Meteorites offer important insights into processes in stars and in interstellar regions, the birth of our solar system, the formation and evolution of planets and smaller bodies, and the origin of life. The first edition was immensely popular with meteorite collectors, scientists and science students in many fields, as well as amateur astronomers. In this second edition all of the illustrations have been updated and improved, many sections have been expanded and modified based on discoveries in the past decade, and a new final chapter on the importance of meteorites has been added. Everyone with an interest in meteorites will want a copy of this book.

What will be the next ‘giant leap’ in space exploration? Could it be a manned expedition to the Red Planet Mars? In this challenging and thought-provoking book, Martin Turner shows how modern technologies not only make such a journey possible, but that advances in those technologies will make it more probable, and that the first human mission to Mars will happen within our lifetime. The latest rocket propulsion, spacecraft technology and planned developments in nuclear and electric propulsion technologies are the key factors which will enable this journey to take place. Of particular importance is the necessity to transport cargo to Mars, and to provide essential life support for the crew food, water, air and fuel to enable the return journey. Expedition Mars challenges us to face the fact that, sooner or later, humans will have to make a choice: stay here on Earth or explore the Solar System beyond.

Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion.

This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties.

The discussion of plasma models is to a large extent limited to Magnetohydrodynamics (MHD) with its merits and limitations clearly explained. MHD provides the students on their first encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics.

From the reviews:

"Bulging with concise explanations and 142 clarifying diagrams and photos, the book probably represents some of the best pedagogy in the solar system on these topics. a ] just the right level for most undergraduates. a ] Open-minded scientists looking for an authoritative tour of astrobiology will enjoy the book a ] . The authora (TM)s summary of exoplanet detection techniques is excellent a ] . Jones keeps us interested with simple explanations a ] . His approach is quite an achievement a ] ." (Charley Lineweaver, Physics Today, February, 2005).

"This is a textbook suitable for university use. a ] this is one of the best. a ] includes excellent recent images of Mars, Europa and elsewhere, and is richly illustrated with explanatory diagrams. a ] There is a useful index, a glossary and a list of a ~resourcesa (TM) (websites and books)." (Malcolm Walter, Australian Physics, Vol. 42 (3) July/August 2005)

"What is required for life, and where might it have evolved? a ] These are the questions that are addressed in this wide ranging, well written and thought provoking book. a ] But for anyone wishing to follow a ] Jonesa (TM) book is an excellent start." (Dr. C.M.Linton, Contemporary Physics, Vol. 46 (3), 2005)

"This book centres on the search for life in the Solar System and beyond. It includes an overview of many of the disciplines involved in this field of research, which include astronomy, biology and geology. a ] It was good to see that the astronomy has been kept fairly descriptive and not too mathematical. This keeps the flow of the book. a ] As an overview of the key subjects involved in astrobiology for a university course, I think this book issuccessful." (James Silvester, Astronomy Now, March, 2005)

Although, at present there is no firm evidence for extraterrestrial life, enormous progress has been made in recent years, both in our understanding of life on Earth and of the potential for life existing elsewhere in the universe. Life in the Solar System and Beyond embaces aspects form all the osre related fields (astronomy, planetary science, chemistry, biology, and Physics). This excellent and thought-provoking introduction:

• Addresses the important question of what is life, and discusses the origins and evolution of life on Earth, as well as its probable fate
• Looks at places within our Solar System, beyond Earth, especially where life might exist, such as Mars and Europa
• Includes the very latest data on searches for planets around other stars, the results of these searches, and discusses what conditions might be like
• Speculates on possible life elsewhere in the Universe beyond our Solar system, and assesses our chances of making contact, if there is intelligent life out there
• Includes end of chapter summaries to help the reader grasp the main concepts to carry forward
• Provides a list of resources, including useful websites at the end of the book which will enable the reader to keep up to date in this rapidly moving field