The Sun is our nearest star; it is a dynamic star, which changes with time. Solar variations have significant influence on Earth's space environment and climate through the Sun's magnetic field, irradiation and energetic particles. Long-term and reliable historical datasets of solar and stellar activity indices are crucial for understanding the variations and predicting the future solar cycle. IAU Symposium 340 brings together scientists from diverse, interdisciplinary areas to address the latest discoveries from these long-term datasets for the understanding of solar and stellar magnetic cycles. They make comparisons between different datasets and discuss how to make uniform databases. The proceedings of IAU S340 contain a selection of presentations and reviews from internationally renowned experts. They provide an up-to-date account of this field of importance to researchers and advanced students in solar, stellar, space and heliospheric physics.

Discovering Pluto is an authoritative account of the exploration of Pluto and its moons, from the first inklings of tentative knowledge through the exciting discoveries made during the flyby of the NASA research spacecraft New Horizons in July 2015. Co-author Dale P. Cruikshank was co-investigator on the New Horizons mission, while co-author William Sheehan is a noted historian of the solar system. Telling the tale of Pluto's discovery, the authors recount the grand story of our unfolding knowledge of the outer solar system, from William Herschel's serendipitous discovery of Uranus in 1781, to the mathematical prediction in 1846 of Neptune's existence, to Percival Lowell's studies of the wayward motions of those giant planets leading to his prediction of another world farther out. Lowell's efforts led to Clyde Tombaugh's heroic search and discovery of Pluto-then a mere speck in the telescope-at Lowell Observatory in 1930. Pluto was finally recognized as the premier body in the Kuiper Belt, the so-called third zone of our solar system. The first zone contains the terrestrial planets (Mercury through Mars) and the asteroid belt; the second, the gas-giant planets Jupiter through Neptune. The third zone, holding Pluto and the rest of the Kuiper Belt, is the largest and most populous region of the solar system. Now well beyond Pluto, New Horizons will continue to wend its lonely way through the galaxy, but it is still transmitting data, even today. Its ultimate legacy may be to inspire future generations to uncover more secrets of Pluto, the solar system, and the universe.

Dawn-Dusk Asymmetries in Planetary Plasma Environments Dawn-dusk asymmetries are ubiquitous features of the plasma environment of many of the planets in our solar system. They occur when a particular process or feature is more pronounced at one side of a planet than the other. For example, recent observations indicate that Earth's magnetopause is thicker at dawn than at dusk. Likewise, auroral breakups at Earth are more likely to occur in the pre-midnight than post-midnight sectors. Increasing availability of remotely sensed and in situ measurements of planetary ionospheres, magnetospheres and their interfaces to the solar wind have revealed significant and persistent dawn-dusk asymmetries. As yet there is no consensus regarding the source of many of these asymmetries, nor the physical mechanisms by which they are produced and maintained. Volume highlights include: * A comprehensive and updated overview of current knowledge about dawn-dusk asymmetries in the plasma environments of planets in our solar system and the mechanisms behind them * Valuable contributions from internationally recognized experts, covering both observations, simulations and theories discussing all important aspects of dawn-dusk asymmetries * Space weather effects are caused by processes in space, mainly the magnetotail, and can be highly localized on ground. Knowing where the source, i.e., where dawn-dusk location is will allow for a better prediction of where the effects on ground will be most pronounced Covering both observational and theoretical aspects of dawn dusk asymmetries, Dawn--Dusk Asymmetries in Planetary Plasma Environments will be a valuable resource for academic researchers in space physics, planetary science, astrophysics, physics, geophysics and earth science.

Join Bonnie J. Buratti, a leading planetary astronomer, on this personal tour of NASA's latest discoveries. Moving through the Solar System from Mercury, Venus, Mars, past comets and asteroids and the moons of the giant planets, to Pluto, and on to exoplanets, she gives vivid descriptions of landforms that are similar to those found on Earth but that are more fantastic. Sulfur-rich volcanoes and lakes on Io, active gullies on Mars, huge ice plumes and tar-like deposits on the moons of Saturn, hydrocarbon rivers and lakes on Titan, and nitrogen glaciers on Pluto are just some of the marvels that await readers. Discover what it is like to be involved in a major scientific enterprise, with all its pitfalls and excitement, from the perspective of a female scientist. This engaging account of modern space exploration is written for non-specialist readers, from students in high school to enthusiasts of all ages.

From the authors of Sketching the Moon comes a comprehensive guide filled with richly illustrated, detailed drawing tutorials that cover a variety of solar phenomena. Explanations of what to expect visually from white light, Hydrogen-alpha and Calcium K filters are provided for those new to solar observing, along with essential tips on equipment, observing techniques and the practicalities of drawing at the eyepiece. Time-honored, traditional methods and media are described in tandem with innovative techniques developed and shared by contemporary astronomical sketchers. For the technically minded, detailed descriptions are given on how to use image manipulation software to bring your sketches to life through animation. The Sun is the most visually dynamic object in our solar system and offers compelling, spectacular views. Knotted magnetic field lines give rise to powerful eruptions and form the intricate sunspots and arching prominences that make our nearest star one of the most exciting, yet challenging, astronomical objects to sketch. Facilitated by the availability of affordable dedicated solar telescopes and filters, the Sun has become an increasingly popular target amongst astronomical sketchers. The use of narrowband solar filters provides a wonderful opportunity to capture views of the Sun that have, until recently, been largely inaccessible. You'll discover easy to follow, step-by-step instructions geared toward your specific interests, be it technical sketching and contributing to science, personal study, or even fun solar outreach activities that help children learn through art. By using Solar Sketching as a reference, drawing the Sun has never been easier.

The far side of the Moon, also called the "dark side of the Moon" was unknown to humanity until the Luna and Lunar Orbiter pictures were returned to Earth. This wonderful book contains beautiful photographs and newly-assembled mosaic images of the far side of the Moon, cleaned of transmission, imaging stripes and processing artifacts by today's computer technology. Byrne's superb analysis documents the appearance of the features of the far side with beautiful pictures from Lunar Orbiter. Until now, the far side Lunar Orbiter photos have only been available with strong reconstruction lines, but appear here for the first time as complete photographs, unmarred by imaging and processing artifacts.

Compiled by a team of experts, this textbook introduces the properties and evolution of the most immediately visible objects in the Universe - stars. Designed for elementary university courses in astronomy and astrophysics, it starts with a detailed discussion of our nearest star, the Sun, and describes how solar physicists have come to understand its internal workings. It then considers how we study the basic physical properties and life-cycles of more distant stars, culminating with a discussion of more 'exotic' objects, such as neutron stars and black holes. This second edition has a greater emphasis on the physical and spectral properties of stars, introducing stellar atmospheres, spectral line formation and the role of binary stars in the formation of compact objects. Avoiding complex mathematics, and generously illustrated in colour throughout, this accessible text is ideal for self-study and will appeal to both amateur astronomers and undergraduate students.

This fully-updated second edition remains the only truly detailed exploration of the origins of our Solar System, written by an authority in the field. Unlike other authors, Michael Woolfson focuses on the formation of the solar system, engaging the reader in an intelligent yet accessible discussion of the development of ideas about how the Solar System formed from ancient times to the present.Within the last five decades new observations and new theoretical advances have transformed the way scientists think about the problem of finding a plausible theory. Spacecraft and landers have explored the planets of the Solar System, observations have been made of Solar-System bodies outside the region of the planets and planets have been detected and observed around many solar-type stars. This new edition brings in the most recent discoveries, including the establishment of dwarf planets and challenges to the 'standard model' of planet formation - the Solar Nebula Theory.While presenting the most up-to-date material and the underlying science of the theories described, the book avoids technical jargon and terminology. It thus remains a digestible read for the non-expert interested reader, whilst being detailed and comprehensive enough to be used as an undergraduate physics and astronomy textbook, where the formation of the solar system is a key part of the course.Michael Woolfson is Emeritus Professor of Theoretical Physics at University of York and is an award-winning crystallographer and astronomer.

The Encyclopedia of the Solar System, third edition provides a framework for understanding the origin and evolution of the solar system, historical discoveries, and details about planetary bodies and how they interact-with an astounding breadth of content and breathtaking visual impact. The encyclopedia includes the latest explorations and observations, hundreds of color digital images and illustrations, and over 1,000 pages. It stands alone as the definitive work in this field, and will serve as a modern messenger of scientific discovery and provide a look into the future of our solar system.

New additions to the third edition will reflect the latest progress and growth in the field, including past and present space missions to the terrestrial planets, the outer solar systems and space telescopes used to detect extrasolar planets.

Presents 700 full-color digital images and diagrams from current space missions and observatories, bringing to life the content and aiding in the understanding and retention of key concepts.
Includes a substantial appendix containing data on planetary missions, fundamental data of relevance for planets and satellites, and a glossary, providing immediately accessible mission data for ease of use in conducting further research or for use in presentations and instruction.
Contains an extensive bibliography, providing a guide for deeper studies into broader aspects of the field and serving as an excellent entry point for graduate students aiming to broaden their study of planetary science.

Recent discoveries of planet-like objects circling other sun-like stars have stirred enormous interest in what other planets may exist in the universe, and whether they could support intelligent life. This book takes us into the midst of this search for extrasolar planets. Unlike other books, it focuses on the people behind the searches -- many known personally by the author -- and the extraordinary technology that is currently on the drawing boards. The author is an experienced, award-winning science journalist who was previously technology correspondent for the Financial Times of London. He has written on many topics in astronomy and astrobiology in over 35 different newspapers and magazines worldwide.

The Red Planet has been a subject of fascination for humanity for thousands of years, becoming part of our folklore and popular culture. The most Earthlike of the planets in our solar system, Mars may have harbored some form of life in the past and may still possess an ecosystem in some underground refuge. The mysteries of this fourth planet from our Sun make it of central importance to NASA and its science goals for the twenty-first century. In the wake of the very public failures of the Mars Polar Lander and the Mars Climate Orbiter in 1999, NASA embarked on a complete reassessment of the Mars Program. Scott Hubbard was asked to lead this restructuring in 2000, becoming known as the 'Mars Czar.' His team's efforts resulted in a very successful decade-long series of missions--each building on the accomplishments of those before it--that adhered to the science adage 'follow the water' when debating how to proceed. Hubbard's work created the Mars Odyssey mission, the twin rovers Spirit and Opportunity, the Mars Reconnaissance Orbiter, the Phoenix mission, and most recently the planned launch of the Mars Science Laboratory. Now for the first time Scott Hubbard tells the complete story of how he fashioned this program, describing both the technical and political forces involved and bringing to life the national and international cast of characters engaged in this monumental endeavor. Blending the exciting stories of the missions with the thrills of scientific discovery, Exploring Mars will intrigue anyone interested in the science, the engineering, or the policy of investigating other worlds.

The Sun is so powerful, so much bigger than us, that it is a terrifying subject. Yet though we depend on it, we take it for granted. Amazingly the first book of its kind, CHASING THE SUNis a cultural and scientific history of our relationship with the star that gives us life. Richard Cohen, applying the same mix of wide-ranging reference and intimate detail that won outstanding reviews for By the Sword, travels from the ancient Greek astronomers to modern-day solar scientists, from Stonehenge to Antarctica (site of the solar eclipse of 2003, when penguins were said to sing), Mexico's Aztecs to the Norwegian city of Tromso, where for two months of the year there is no Sun at all. He introduces us to the crucial 'sunspot cycle' in modern economics, the religious dances of Indian tribesmen, the histories of sundials and calendars, the plight of migrating birds, the latest theories of global warming, and Galileo recording his discoveries in code, for fear of persecution. And throughout, there is the rich Sun literature -- from the writings of Homer through Dante and Nietzsche to Keats, Shelley and beyond. Blindingly impressive and hugely readable, this is a tour de force of narrative non-fiction.

"Habitable Planets for Man" examines and estimates the probabilities of finding planets habitable to human beings, where they might be found, and the number there may be in our own galaxy. The author presents in detail the characteristics of a planet that can provide an acceptable environment for humankind, itemizes the stars nearest the earth most likely to possess habitable planets, and discusses how to search for habitable planets. Interestingly for our time, he also gives an appraisal of the earth as a planet and describes how its habitability would be changed if some of its basic properties were altered."Habitable Planets for Man" was published at the height of the space race, a few years before the first moon landing, when it was assumed that in the not-too-distant future human beings "will be able to travel the vast distances to other stars." More than forty years after its initial publication, and to celebrate RAND's 60th Anniversary, RAND brings this classic work back into print in paperback and digital formats.

"Planets for Man" was written at the height of the space race, a few years before the first moon landing, when it was assumed that in the not-too-distant future human beings "will be able to travel the vast distances to other stars." The authors propose to determine - on the basis of then current biological and cosmological knowledge - whether there are other worlds where humans can survive or where human life may even now be flourishing. This volume, co-authored by "RAND" researcher Stephen Dole and science fiction master Isaac Asimov, certainly one of the more unusual co-authorships in "RAND's" long history of research and publishing, it was based on a more technical treatise authored by Dole, "Habitable Planets for Man". More than forty years after its initial publication, and to celebrate "RAND's" 60th Anniversary, "RAND" brings this classic work back into print in paperback and digital formats.

The Moon is accessible to everyone. Because it is easy to observe everywhere, even in big cities, it is a prime target for aspiring astronomers and for those who are merely curious about the night sky. This easy-to-use guide to discovering lunar sites takes the reader through fourteen observing sessions from New Moon to Full Moon. For each evening, the book shows which craters, mountains and other features can be seen, and how to find them. Each photograph shows what the observer actually sees through a telescope, solving the usual difficulties of orientation confronting beginners. Images are shown as they appear through both refracting and reflecting telescopes. Maps printed on the book's front and back flaps show the whole Moon with sites as seen through a refractor, through a Newtonian reflector, or, when turned upside-down, through binoculars. Jean Lacroux has been a columnist for the French astronomy magazine Ciel et Espace for 25 years. He has published four successful amateur astronomy books in French. Christian Legrand is an engineer and amateur astronomer, who has been a passionate lunar observer since the Apollo missions.

The Near Earth Asteroid Rendezvous (NEAR) was the first dission to orbit and eventually land on an asteroid. A phenomenal success, the mission returned with hundreds of thousands of images, spectra, and other measurements about the large near-Earth asteroid 433 Eros. Some of the scientists and engineers who made NEAR such a success describe the mission here in their own words, from the initial concept studies, through the development phase, launch, cruise operations, the flyby of asteroid Mathilde, the near-catastrophic main engine failure in 1998, the heroic rescue and recovery of the spacecraft, the amazing year-long up-close look at one of Earth's most primitive celestial neighbors, and, finally, the daring attempt to land the spacecraft on Eros at the end of the mission. The book is illustrated throughout with images from the mission and explanatory diagrams. Jim Bell is an Assistant Professor in the Cornell University Astronomy Department whose research focuses on the geology, chemistry, and mineralogy of planets, asteroids, and comets using data obtained from telescopes and spacecraft missions. He is a member of a number of space science teams, including the NASA Mars Pathfinder and NEAR. Author of some 70 first and co-authored journal publications, he is a frequent contributor to popular astronomy magazines and radio shows. The International Astronomical Union recently awarded him the honor of having asteroid 8146 Jimbell named after him. Jacqueline Mitton is the Press Officer and a fellow of the Royal Astronomical Society, a member of the International Astronomical Union, and a Member of the Division of Planetary Sciences of the American Astronomical Society. She is the author or co-author of 16 astronomy books; her most recent being The Cambridge Dictionary of Astronomy (2001).

ABOUT THIS BOOK.... The success of any plan depends not only on the availability of the necessary skills and resources, but also very decisively, on the timing. In former times people gathered knowledge of axioms such as this by direct observation. They discovered that numerous natural phenomena are directly related to the movements of the moon Johanna Paungger is one of ten children of a Tyrolean mountain farmer. She belongs to the select few in whose environment this wisdom was kept alive for centuries handed down from one generation to the next. For the first time this knowledge is now made generally available. This book has an abundance of tips and advice to do with all the important areas of our daily life, from health, the home and nutrition to farming, forestry and gardening. In Germany it has been a massive best-seller for several years. Patience is the only thing necessary to profit from this book. Working with the lunar cycles and natural harmonies can change your life.

David Levy brings these "ghostly apparitions" to life. With fascinating scenarios both real and imagined, he shows how comets have wreaked their special havoc on Earth and other planets. Beginning with ground zero as comets take form, we track the paths their icy, rocky masses take around our universe and investigate the enormous potential that future comets have to directly affect the way we live on this planet and what we might find as we travel to other planets.

In this extraordinary volume, David Levy shines his expert light on a subject that has long captivated our imaginations and fears, and demonstrates the need for our continued and rapt attention.

An account of the 1976 Viking expedition to Mars describes the spacecraft and its instruments, the journey itself, and the mission's results.

Explore Earth's closest neighbor, the Moon, in this fascinating and timely book and discover what we should expect from this seemingly familiar but strange, new frontier. What startling discoveries are being uncovered on the Moon? What will these tell us about our place in the Universe? How can exploring the Moon benefit development on Earth? Discover the role of the Moon in Earth's past and present; read about the lunar environment and how it could be made more habitable for humans; consider whether continued exploration of the Moon is justified; and view rare Apollo-era photos and film stills. This is a complete story of the human lunar experience, presenting many interesting but little-known and significant events in lunar science for the first time. It will appeal to anyone wanting to know more about the stunning discoveries being uncovered on the Moon.

The early development of life, a fundamental question for humankind, requires the presence of a suitable planetary climate. Our understanding of how habitable planets come to be begins with the worlds closest to home. Venus, Earth, and Mars differ only modestly in their mass and distance from the Sun, yet their current climates could scarcely be more divergent. Only Earth has abundant liquid water, Venus has a runaway greenhouse, and evidence for life-supporting conditions on Mars points to a bygone era. In addition, an Earth-like hydrologic cycle has been revealed in a surprising place: Saturn's cloud-covered satellite Titan has liquid hydrocarbon rain, lakes, and river networks.
Deducing the initial conditions for these diverse worlds and unraveling how and why they diverged to their current climates is a challenge at the forefront of planetary science. Through the contributions of more than sixty leading experts in the field, "Comparative Climatology of Terrestrial Planets" sets forth the foundations for this emerging new science and brings the reader to the forefront of our current understanding of atmospheric formation and climate evolution. Particular emphasis is given to surface-atmosphere interactions, evolving stellar flux, mantle processes, photochemistry, and interactions with the interplanetary environment, all of which influence the climatology of terrestrial planets. From this cornerstone, both current professionals and most especially new students are brought to the threshold, enabling the next generation of new advances in our own solar system and beyond.
Contents
Part I: Foundations
Jim Hansen
Mark Bullock
Scot Rafkin
Caitlin Griffith
Shawn Domagal-Goldman and Antigona Segura
Kevin Zahnle
Part II: The Greenhouse Effect and Atmospheric Dynamics
Curt Covey
G. Schubert and J. Mitchell
Tim Dowling
Francois Forget and Sebastien Lebonnois
Vladimir Krasnopolsky
Adam Showman
Part III: Clouds, Hazes, and Precipitation
Larry Esposito
A. Maattanen, K. Perot, F. Montmessin, and A. Hauchecorne
Nilton Renno
Zibi Turtle
Mark Marley
Part IV: Surface-Atmosphere Interactions
Colin Goldblatt
Teresa Segura et al.
John Grotzinger
Adrian Lenardic
D. A. Brain, F. Leblanc, J. G. Luhmann, T. E. Moore, and F. Tian
Part V: Solar Influences on Planetary Climate
Aaron Zent
Jerry Harder
F. Tian, E. Chassefiere, F. Leblanc, and D. Brain
David Des Marais

IAU Symposium 263 provides a state-of-the-art review of icy bodies in the Solar System, a topic crucial to understanding processes involved in the Solar System's formation, the consequences for water on planets, and ultimately, the habitable zones around other stars. Ice-rich planetesimals which form beyond the snow line are discussed, using an interdisciplinary approach. The main topics covered include: accretion of icy grains in the protoplanetary disk, the long-period comet flux and the Oort cloud population, transfer mechanisms of bodies from their source regions to the Sun's neighborhood, the physics and dynamics of trans-Neptunian objects, transition objects (comets and asteroids), cryovolcanism and modeling the interiors of icy bodies, and a review of past, present and future space missions. This volume gives a broad overview of the importance of these bodies, from comets up to liquid water on terrestrial planets, and the formation of ices in the Solar System.