This book offers a new concept of the possible genesis of primary forms of living matter in the processes that accompany a hypervelocity meteorite impact onto the surface of a planet. The concept is based on results obtained in direct impact experiments and in laboratory simulations of hypervelocity impact processes involving the generation of a plasma torch, on bona fide data on the physical processes occurring in nature, and on the available material evidence of impact consequences on Solar system bodies. The concept can explain the possibility of the emergence of extraterrestrial life in the interiors of celestial bodies with extreme surface temperatures and moderate temperatures in the inner layers provided water is present.

The two most fascinating questions about extraterrestrial life are where it is found and what it is like. In particular, from our Earth-based vantage point, we are keen to know where the closest life to us is, and how similar it might be to life on our home planet. This book deals with both of these key issues. It considers possible homes for life, with a focus on Earth-like exoplanets. And it examines the possibility that life elsewhere might be similar to life here, due to the existence of parallel environments, which may result in Darwinian selection producing parallel trees of life between one planet and another. Understanding Life in the Universe provides an engaging and myth-busting overview for any reader interested in the existence and nature of extraterrestrial life, and the realistic possibility of discovering credible evidence for it in the near future.

This book addresses the problems of Geocosmos and provides a snapshot of the current research in a broad area of Earth Sciences carried out in Russia and elsewhere. The themes covered include solar physics, physics of magnetosphere, ionosphere and atmosphere, solar-terrestrial coupling links, seismology, geoelectricity, paleomagnetism and rock magnetism, as well as cross-disciplinary studies. The proceedings are carefully edited, providing a panoramic outlook of a broad area of Earth Sciences. The readership includes colleague researchers, students and early career scientists. The proceedings will help the readers to look at their research fields from various points of view. Problems of Geocosmos conferences are held by Earth Physics Department, St. Petersburg University bi-annually since 1994. It is the largest forum of this kind in Russia/former Soviet Union attracting up to 200 researchers in Earth and magnetospheric physics.

A total eclipse of the Sun is the most awesome sight in the heavens. Totality takes you to eclipses of the past, present, and future, and lets you see--and feel--why people travel to the ends of the Earth to observe them.
An absolutely indispensable resource for anyone who plans to observe an eclipse, and a must read for all astronomy buffs, this superb new edition brims with the anecdotes, experiences, and advice of many veteran eclipse observers. Indeed, it is the best guide and reference book on solar eclipses ever written, packed with information on how to observe them; how to photograph and videotape them; why they occur; their history and mythology; how eclipses revealed the workings of the Sun and made Einstein famous; and when and where to see future eclipses. Totality once again features the spectacular photography of Fred Espenak, who runs the NASA Eclipse Home Page and is the best-known and respected of all eclipse calculators and information sources. His many stunning color photographs illuminate this unparalleled exploration of eclipses. The volume has been updated to include current information on upcoming eclipses, with new chapters on the total eclipses due in 2008, 2009, 2010, and 2017, plus all new chapters on how to photograph, video record, and process your eclipse images, with emphasis on the new generation of digital cameras.
Strikingly illustrated with stunning photographs and more than a hundred maps and diagrams, here is everything you need to know about eclipses of the sun, in an accurate, clearly written, and entertaining volume that can be read by lay people and astronomers with ease and enjoyment.

The solar wind is a stream of charged particles -- a plasma -- ejected from the upper atmosphere of the sun. It consists mostly of electrons and protons with energies of about 1 keV. These particles are able to escape the sun's gravity, in part because of the high temperature of the corona, but also because of high kinetic energy that particles gain through a process that is not well-understood at this time. The solar wind creates the Heliosphere, a vast bubble in the interstellar medium surrounding the solar system. Other phenomena include geomagnetic storms that can knock out power grids on Earth, the aurorae such as the Northern Lights, and the plasma tails of comets that always point away from the sun. This book presents the latest research in the world on this topic.

A total eclipse of the Sun is the most awesome sight in the heavens. Totality takes you to eclipses of the past, present, and future, and lets you see--and feel--why people travel to the ends of the Earth to observe them.
An absolutely indispensable resource for anyone who plans to observe an eclipse, and a must read for all astronomy buffs, this superb new edition brims with the anecdotes, experiences, and advice of many veteran eclipse observers. Indeed, it is the best guide and reference book on solar eclipses ever written, packed with information on how to observe them; how to photograph and videotape them; why they occur; their history and mythology; how eclipses revealed the workings of the Sun and made Einstein famous; and when and where to see future eclipses. Totality once again features the spectacular photography of Fred Espenak, who runs the NASA Eclipse Home Page and is the best-known and respected of all eclipse calculators and information sources. His many stunning color photographs illuminate this unparalleled exploration of eclipses. The volume has been updated to include current information on upcoming eclipses, with new chapters on the total eclipses due in 2008, 2009, 2010, and 2017, plus all new chapters on how to photograph, video record, and process your eclipse images, with emphasis on the new generation of digital cameras.
Strikingly illustrated with stunning photographs and more than a hundred maps and diagrams, here is everything you need to know about eclipses of the sun, in an accurate, clearly written, and entertaining volume that can be read by lay people and astronomers with ease and enjoyment.

This book is a comprehensive advancement about the understanding of the volcanology of Mars in all its aspects, from its primary formation to its evolution in time, from the smaller structures to the bigger structures. It discusses the implications of volcanism in the general environmental and geological context of Mars. The book is validating the Southern Giant Impact Hypothesis explaining the formation of Mars in an interdisciplinary approach, including mineralogical, geochemical, volcanological as well as geomorphological information. Implications for future explorations in terms of resources are provided. This book serves as a textbook for undergraduate and graduate level to foster new basic research in the field of planetary volcanology and is a new guide for future missions toward a volcanic world, including new detailed information for the general audience who is always keen to know more about the history of Mars and its large volcanoes. The book also presents an updated situation about the water resources of the planet.

From myth to Musk, astrology to astronomy, Dr Stuark Clark selects the very best writing about the Red Planet. From its very first sighting, Mars has been a source of fascination for humanity. Named for the Roman god of war, this red planet has been explored more than any other beyond Earth and continues to occupy a distinctive place in our imagination. It's an environment that may even foster life. In The Book of Mars, Dr Stuart Clark selects one hundred pieces of writing about the planet. It is a collection that brings together fact and fiction, dreams and fears, centuries of observation and more recent feats of interstellar exploration. From classic writers of science fiction – Stanley G. Weinbaum, Arthur C. Clarke, H.G. Wells, Ray Bradbury, Pamela Sargent, Roger Zelazny – to distinguished experts in astronomy, astrobiology and aerospace engineering; from Hugo and Nebula Award-winning authors – Kim Stanley Robinson, Mary Robinette Kowal – to trail-blazing journalists and science communicators; from Andy Weir's The Martian to Elon Musk's SpaceX programme, The Book of Mars is an extraordinary overview both of the Red Planet and of the way scientific investigation diffuses into culture.

Embark on an awe-inspiring and informative journey through our Solar System and beyond in this illuminating astronomy book! Discover how big the Universe is, why our view of the sky is constantly changing, what came before the Big Bang, and so much more. 3, 2, 1, blast off! Inside the pages of this comprehensive guide to astronomy for beginners, you'll discover: - Simple text and step-by-step graphics make astronomy easy to understand - Fun facts and tip-of-the-tongue questions are presented through bite-sized factoids and question-and-answer features - Clear explanations demystifying more advanced topics such as cosmic rays, dark matter, and black hole collisions An out-of-this-world reference book about space that introduces you to the weird and wonderful world of astronomy and space exploration. From the structure of the Milky Way to the Earth's nearest celestial body, the Moon, How Space Works takes you on an unforgettable tour through the stars and galaxies, and to the furthest reaches of space! Answering all your burning questions about space, from ancient white dwarf stars to the Mars Rover, this visual guide explains the basics of astronomy through bold graphics and step-by-step artworks. It's the ultimate book for armchair astronomers and space-technology enthusiasts looking for reliable and up-to-date facts and explanations. DK's How Things Work series uses dynamic graphics and jargon-free text to explain the modern world simply and clearly. Packed with fascinating facts and stats, these visual guides cover everything from science to philosophy, making complex topics more accessible than ever before!

In the summer of 1878 three ruthless and brilliant scientists raced to Wyoming and Colorado to observe a total solar eclipse. One sought to discover a new planet. Another fought to prove that science was not an anathema to femininity. And a young, megalomaniacal inventor sought to test his bona fides and light the world through his revelations. David Baron brings to life these three competitors-James Craig Watson, Maria Mitchell and Thomas Edison-re-creating the jockeying of nineteenth-century astronomy. With accounts of train robberies and Indian skirmishes, the last days of the Wild West come alive. A magnificent portrayal of America's dawn as a superpower, American Eclipse depicts a nation looking to the skies to reveal its ambition and expose its genius.

The range of phenomena that manifest at all different time and length scales and the wide range of sizes of space objects, from minor bodies in the Solar System to exoplanets, and from dust particles to Jupiter-size bodies, require the development of dynamical modeling and analysis tools that can handle these different scales. This volume collects contributions given by distinguished scientists at the hybrid IAU Symposium 364. The methods in dynamics modeling of space objects have already reached a state of maturity, and their implementation provided a large number of important results pertaining to both the theory and their applications. The contributions cover the recent advances in the multi-scale dynamics of natural and artificial space objects from various perspectives, which will benefit graduate students and researchers working in the fields of celestial mechanics, astrodynamics, planetary sciences, applied mathematics and dynamical systems.

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.

Complete color global maps and high-resolution mosaics of Jupiter's four large moons - Io, Europa, Ganymede and Callisto - are compiled for the first time in this important atlas. The satellites are revealed as four visually striking and geologically diverse planetary bodies: Io's volcanic lavas and plumes and towering mountains; Europa's fissured ice surface; the craters, fractures and polar caps of Ganymede; and the giant impact basins, desiccated plains and icy pinnacles of Callisto. Featuring images taken from the recent Galileo mission, this atlas is a comprehensive mapping reference guide for researchers. It contains 65 global and regional maps, nearly 250 high-resolution mosaics, and images taken at resolutions from 500 meters to as high as 6 meters.

An authoritative introduction for graduate students in the physical sciences, this award-winning textbook explains the wide variety of physical, chemical, and geological processes that govern the motions and properties of planets. This updated second edition has been revised and improved while maintaining its existing structure and organization. Many data tables and plots have been updated to account for the latest measurements. A new Appendix focuses on recent discoveries since the second edition was first published. These include results from Cassini, Kepler, MESSENGER, MRO, LRO, Dawn at Vesta, Curiosity, and others, as well as many ground-based observatories. With over 300 exercises to help students apply the concepts covered, this textbook is ideal for graduate courses in astronomy, planetary science and earth science, and well suited as a reference for researchers. Color versions of many figures, movie clips supplementing the text, and other resources are available at www.cambridge.org/depater.

Our Sun is the nearest star and thus an ideal laboratory to study dynamic processes which are related to solar terrestrial physics. The topics addressed in this book cover solar MHD and generation of acoustic waves, as well as physical parameters that are suited to describing solar activity and could serve as proxies for space weather forecasting. The influence of solar activity (radiation and solar wind) on telecommunication systems, satellite missions etc. is also discussed. In short, contribution reports are given on various topics in solar physics. The book covers solar physics from the photosphere to space weather influences. The intended level of readership is aimed at students working in this or related fields, professionals, and astronomers who wish to acquire some basic knowledge in the field of solar terrestrial relations, which is provided in the review articles.

Extensively revised and updated, this new edition of David A. Rothery's acclaimed geological guide to the outer solar system includes results and close-up color and black and white images from the 1995-1999 Galileo mission to Jupiter and from the Voyager space probe. Rothery, a noted planetary scientist, explains the geological aspects of the major satellites of the outer bodies, from Jupiter and Neptune to the Pluto-Charon system. Rothery discusses their similarities and differences, and reveals how they resemble Earth-like planets. This fascinating book is written in an introductory style ideal for first or second year degree courses. Amateur geologists and astronomers will also find its insights rewarding.

Reviews of the First Edition: 'The depth and authority of the treatment of physical geological processes makes this a good introduction to the outer satellites for undergraduate students, while the clarity of the text ensures that things do not become too complicated for less expert readers.' Lionel Wilson, Times Higher Education Supplement

'Rothery brings these satellites to life.' David Hughes, New Scientist

Over the last decade the physics of black holes has been revolutionized by developments that grew out of Jacob Bekenstein's realization that black holes have entropy. Stephen Hawking raised profound issues concerning the loss of information in black hole evaporation and the consistency of quantum mechanics in a world with gravity. For two decades these questions puzzled theoretical physicists and eventually led to a revolution in the way we think about space, time, matter and information. This revolution has culminated in a remarkable principle called "The Holographic Principle", which is now a major focus of attention in gravitational research, quantum field theory and elementary particle physics. Leonard Susskind, one of the co-inventors of the Holographic Principle as well as one of the founders of String theory, develops and explains these concepts.

The Mars Curiosity Rover is the most sophisticated mobile laboratory ever deployed on a planet. For over seven years, scores of investigators have planned its daily route and activities, poring over the overwhelming images and data and revising our understanding of planetary surfaces, geology, and potential habitability. This book takes readers right down to the surface of Mars, chronicling Curiosity's physical and scientific journey across the planet's Earth-like, yet strikingly alien vistas. Through dozens of images and descriptive accounts of the surface, you will gain a deeper knowledge of the Martian landscape, from the floor of Gale Crater up to the cliffs of Mount Sharp. Presented at the end of each chapter are the results and revelations from the science team spearheading the mission. Like any cross-country road trip, the rover has hit some unexpected hitches along the way. The book describes the obstacles faced by the rover and its scientists over the years and the difficult decisions and careful experimentation it took to solve them.

This unique collaboration between a classicist and physicist at the University of Illinois at Chicago is the first work to combine the evidence from both China and Rome for the spectacular daylight comet of 44 BC, perhaps the most famous comet in antiquity. This investigation, which also examines allusions to this comet in astrological literature from later antiquity, sheds new light on the significance of the comet as a powerful symbol in the political propaganda that launched Augustus' career.

This book is devoted to the most relevant issues in crystal chemistry and mineral typomorphism; the structure, physico-chemical and technological properties of minerals; and the computational modeling of mineral structure and properties. Considerable attention is paid to the latest advances in and applications of physical methods of investigation for mineral structure and composition, in particular, X-Ray diffraction, spectroscopic (optical, vibrational, ESR, Moessbauer, etc.) and microscopic (SEM, TEM, AFM, etc.) studies, as well as chemical and isotopic analysis methods. The current research trends in space and planetary mineralogy (meteorites, regolites, tektites) are also discussed. Though specifically intended for the specialist earth and planetary science readership, the book will be of interest to a broad range of scientists. It gathers the proceedings of the Tenth All-Russian Youth Scientific Conference "Minerals: structure, properties, methods of investigation." Jointly organized by the Institute of Geology and Geochemistry, the Institute of Mineralogy (Urals Branch of the Russian Academy of Sciences) and Ural Federal University, the event was held in Ekaterinburg, Russia, on May 27-June 1, 2019.

Philosophers and poets in times past tried to figure out why the stainless moon "smoothly polished, like a diamond" in Dante's words, had stains. The agreed solution was that, like a mirror, it reflected the imperfect Earth. Today we smile, but it was a clever way to understand the Moon in a manner that was consistent with the beliefs of their age. The Moon is no longer the "in" thing. We see it as often as the Sun and give it little thought - we've become indifferent. However, the Moon does reflect more than just sunlight. The Moon, or more precisely the nomenclature of lunar craters, still holds up a mirror to an important aspect of human history. Of the 1586 craters that have been named honoring philosophers and scientists, only 28 honor a woman. These 28 women of the Moon present us with an opportunity to meditate on this gap, but perhaps more significantly, they offer us an opportunity to talk about their lives, mostly unknown today.

The chemical composition of any planetary atmosphere is of fundamental importance in determining its photochemistry and dynamics in addition to its thermal balance, climate, origin and evolution. Divided into two parts, this book begins with a set of introductory chapters, starting with a concise review of the Solar System and fundamental atmospheric physics. Chapters then describe the basic principles and methods of spectroscopy, the main tool for studying the chemical composition of planetary atmospheres, and of photochemical modeling and its use in the theoretical interpretation of observational data on chemical composition. The second part of the book provides a detailed review of the carbon dioxide atmospheres and ionospheres of Mars and Venus, and the nitrogen-methane atmospheres of Titan, Triton and Pluto. Written by an expert author, this comprehensive text will make a valuable reference for graduate students, researchers and professional scientists specializing in planetary atmospheres.

This book presents a global and synthetic vision of planetology - the study of objects in the Solar System. In the past several decades, planetology has undergone a real revolution, marked in particular by the discovery of the Kuiper belt beyond Neptune, the discovery of extrasolar planets, and also by the space exploration of ever more distant objects. Today, it is at the crossroads of many disciplines: astronomy, geophysics, geochemistry and biology. The Solar System 1 deals with the Solar System as a whole, offering a general presentation of the objects that compose it and its place in the galaxy. It also deals with planetary systems, exoplanets and the interaction of Solar System objects with interplanetary medium. Finally, it analyzes the telluric and giant planets.

This SpringerBrief explores the technological, economic, physiological, and psychological comparisons between a journey to the Moon versus a journey to Mars, taking into consideration the national and international perspectives at play. The author spent over six years interviewing leading space experts from around the world to learn why lunar habitats and the creation of a permanent presence on the Moon are an essential next step to human exploration and settlement in space. Practical reasons related to energy, telecommunications and networking, robotic systems, medical and scientific research, material processing, and more show why it must be the Moon First and Mars Second. These findings and recommendations have been adopted by current NASA Administrator Jim Bridenstine, as well as the current U. S. president. The research in this text reflects the author's experiences working internally within NASA Headquarters, the FAA Commercial Spaceflight Office, as well as the International Space University. It is partially based on Reneau's award-winning Harvard thesis in conjunction with her Master's in International Relations.