Compiled by a team of experts, this textbook has been designed for elementary university courses in astrobiology. It begins with an examination of how life may have arisen on Earth and then reviews the evidence for possible life on Mars, Europa and Titan. The potential for life in exoplanetary systems and the search for extraterrestrial intelligence are also discussed. The text contains numerous useful learning features such as boxed summaries, student exercises with full solutions, and a glossary of terms. It is also supported by a website hosting further teaching materials. Written in an accessible style that avoids complex mathematics, this book is suitable for self-study and will appeal to amateur enthusiasts as well as undergraduate students. It contains numerous helpful learning features such as boxed summaries, student exercises with full solutions, and a glossary of terms. The book is also supported by a webstite hosting further teaching materials.

It takes a certain amount of fortitude to confront your own doom. Ward and Brownlee, having acutely described life's beginnings in "Rare Earth", here portray the mechanisms of its end. With the course of life's evolution revealed in the work of many researchers, depicting the finale has rarely been attempted. Recent studies of the past have given the authors the tools for forecasting the future. They use the history of the planet to suggest the "tape of life" will be rerun - backwards. Changing conditions will reduce the options life has to continue surviving. As a swelling sun and dehydrating Earth limit choices, life will revert to simpler, hardier forms. At some point, although far in the future, life's opportunities will end. A bleak barren world will likely be consumed by Sol's energetic transformation into a red giant star. A lifeless planet will either skirt the circumference of that swollen star or be consumed in its fires.

Although a fiery conclusion is the ultimate finale, there are many intermediate steps along the path. Ice, which has covered our planet many times in the past, is shown here as one of the major signs of the impending finish. Seas withdraw from coastlines and habitat zones shrink dramatically. Weather patterns undergo massive changes from what we experience. The authors use "time transport" techniques to enable you to envision the impact of these drastic variations. You visit future scenarios where plant life's extinction has taken herbivores with it. Grasses exist for a bit, but it's too desolate for complex grazers to enjoy them. Harsh winds scream across those savannahs, dehydrating the soil until the grasses, too, finally expire. These conditions, Ward and Brownlee contend, have likely already begun. The peak of plant diversity may already be behind us. Animal extinctions, accelerated by our presence, must surely follow.

Energy, chemistry, solvents, and habitats - the basic elements of living systems - define the opportunities and limitations for life on other worlds. This study examines each of these parameters in crucial depth and makes the argument that life forms we would recognize may be more common in our solar system than many assume. It also considers, however, exotic forms of life that would not have to rely on carbon as the basic chemical element, solar energy as the main energy source, or water as the primary solvent. Finally the question of detecting bio- and geosignature of such life forms is discussed, ranging from earth environments to deep space. While speculative considerations in this emerging field of science cannot be avoided, the authors have tried to present their study with the breadth and seriousness that a scientific approach to this issue requires. They seek an operational definition of life and investigate the realm of possibilities that nature offers to realize this very special state of matter and avoid scientific jargon wherever possible to make this intrinsically interdisciplinary subject understandable to a broad range of readers.

This study investigates the major theories of the origins of life in the light of modern research with the aim of distinguishing between the necessary and the optional and between deterministic and random influences in the emergence of what we call ‘life.’ Life is treated as a cosmic phenomenon whose emergence and driving force should be viewed independently from its Earth-bound natural history. The author synthesizes all the fundamental life-related developments in a comprehensive scenario, and makes the argument that understanding life in its broadest context requires a material-independent perspective that identifies its essential fingerprints.

Astrobiology -- the study of the intimate relationship between life and the cosmos -- is a fast-growing field that touches on aspects of cosmology, astrophysics, and chemistry. In the first scholarly overview of this dynamic field, biochemists Kevin W. Plaxco and Michael Gross tell the story of life from the Big Bang to the present.

Emphasizing the biochemical nature of astrobiology, Plaxco and Gross examine the origin of the chemical elements, the events behind the developments that made the Universe habitable, and the ongoing sustenance of life. They discuss the formation of the first galaxies and stars, the diverse chemistry of the primordial planet, the origins of metabolism, the evolution of complex organisms, and the feedback regulation of Earth's climate. They also explore life in extreme habitats, potential extraterrestrial habitats, and the search for extraterrestrial life.

This broadly accessible introduction captures the excitement, controversy, and evolution of the dynamic young field of astrobiology. It shows clearly how scientists from different disciplines can combine their special knowledge to enhance our understanding of the Universe.

The dynamic field of astrochemistry brings together ideas of physics, astrophysics, biology and chemistry to the study of molecules between stars, around stars and on planets. Astrochemistry: from Astronomy to Astrobiology provides a clear and concise introduction to this rapidly evolving multidisciplinary subject. Starting with the Molecular Universe, the text covers the formation of the elements, simple models of stars and their classification. It then moves on to draw on the theme of the Origins of Life to study interstellar chemistry, meteorite and comet chemistry as well as the chemistry of planets. Prebiotic chemistry and astrobiology are explored by examining the extremes of the biosphere on Earth, seeing how this may be applied to life in other solar systems.

Astrochemsitry assumes a basic familiarity with principles of physical and organic chemistry but no prior knowledge of biology or astrophysics. This innovative text incorporates results from the latest research and ground and space missions, with key images enhanced by a colour plate section.

• includes latest research and results from ground and space missions
• colour plate section
• summary of concepts and calculations at the end of each chapter

"Do you feel lucky? Well do ya?" asked Dirty Harry. Paleontologist Peter Ward and astronomer Donald Brownlee think all of us should feel lucky. Their rare Earth hypothesis predicts that while simple, microbial life will be very widespread in the universe, complex animal or plant life will be extremely rare. Ward and Brownlee admit that "It is very difficult to do statistics with an N of 1. But in our defense, we have staked out a position rarely articulated but increasingly accepted by many astrobiologists."

Their new science

is the field of biology ratcheted up to encompass not just life on Earth but also life beyond Earth. It forces us to reconsider the life of our planet as but a single example of how life might work, rather than as the only example.

The revolution in astrobiology during the 1990s was twofold. First, scientists grew to appreciate how incredibly robust microbial life can be, found in the superheated water of deep-sea vents, pools of acid, or even within the crust of the Earth itself. The chance of finding such simple life on other bodies in our solar system has never seemed more realistic. But second, scientists have begun to appreciate how many unusual factors have cooperated to make Earth a congenial home for animal life: Jupiter's stable orbit, the presence of the Moon, plate tectonics, just the right amount of water, the right position in the right sort of galaxy. Ward and Brownlee make a convincing if depressing case for their hypothesis, undermining the principle of mediocrity (or, "Earth isn't all that special") that has ruled astronomy since Copernicus.

Origins: Genesis, Evolution and Biodiversity of Microbial Life in the Universe is the sixth unit of the book series Cellular Origins, Life in Extreme Habitats and Astrobiology (COLE) edited by Joseph Seckbach. In this book forty eminent scientists review their studies in the fields of Life from the beginning to the "Fact of Life". The history of Origin of Life and Astrobiology is well covered by these authors. Reviews cover the standard and alternative scenarios of the genesis of Life, while the chapters of "The First Cells" leading to the biodiversity and extremophiles of microbial Life. Among these extremophiles are the microbes living in the Life's limits, such as in high temperature, psychrophilic, UV radiation, and halophilic environments. The origin and history of Martian water is discussed followed by the possible biogeochemistry inside Titan. This new field of Astrobiology has been presented, from comets as a source of materials and Life on earth to the space for last Frontiers.

Growing evidence, based on observations from orbiters, landers and telescopes, indicates that Mars may still have numerous hidden water reservoirs. Moreover, from the point of view of habitability, Mars is a prime target for astrobiologists in search of extant or extinct microbial life because we know that life exists in earth’s permafrost regions, such as parts of Siberia and the Antarctic, which are the closest terrestrial analogues to Mars. Water on Mars and Life surveys recent advances made in research into water on Mars together with its astrobiological implications. This volume addresses not only scientists working in the field but also nonspecialists and students in search of a high-level but accessible introduction to this exciting field of research.

This is the second of a divided two-part softcover edition of  the "Lectures in Astrobiology Volume I" containing the sections "General Introduction", "From Prebiotic Chemistry to the Origin of Life on Earth" and "Appendices" including an extensive glossary on Astrobiology. "Lectures in Astrobiology" is the first comprehensive textbook at graduate level encompassing all aspects of the emerging field of astrobiology. Volume I of the Lectures in Astrobiology gathers a first set of extensive lectures that cover a broad range of topics, from the formation of solar systems to the quest for the most primitive life forms that  emerged on the Early Earth.

"This is a wonderful book by two of the best historians of biology in the business."—Michael Ruse, author of Darwin and Design: Does Evolution Have a Purpose?

"The detailed and thorough research underpinning this book is truly remarkable."—Frank Drake, senior scientist and director of the Center for the Study of Life in the Universe, SETI Institute

The Living Universe is a comprehensive, historically nuanced study of the formation of the new scientific discipline of exobiology and its transformation into astrobiology. Among many other themes, the authors analyze how research on the origin of life became wedded to the search for life on other planets and for extraterrestrial intelligence. Many scientific breakthroughs of the last forty years were either directly supported or indirectly spun off from NASA’s exobiology program, including cell symbiosis, the discovery of the Archaea, and the theories of Nuclear Winter and the asteroid extinction of the dinosaurs.

Exobiology and astrobiology have generated public fascination, enormous public relations benefits for NASA, and––on the flip side of the coin––some of the most heated political wrangling ever seen in government science funding. Dick and Strick provide a riveting overview of the search for life throughout the universe, with all of the Earthly complexities of a science-in-the-making and the imperfect humans called scientists. Their book will appeal to biologists, historians and philosophers of science, planetary scientists (including geologists), and an educated general readership interested in the investigation of life on other planets.

Are we alone? As the search for extraterrestrial intelligence comes more and more into the mainstream, scientists like David Darling step up to explain what we know and what's possible. His book Life Everywhere explores the history and current state of the field called, perhaps unfortunately, astrobiology. Devoted neither to organisms skimming the sun's surface nor to possible signs of intelligence among celebrities--though not explicitly rejecting these phenomena--astrobiology is concerned with the basic questions of life: What is a living organism? Is it common, or likely, elsewhere in the universe? Is it worth trying to communicate across light years? Darling, an astronomer and science journalist, has a knack for explaining complexities and fine details that carries his prose forward where other authors have foundered; the reader is swept up in the enthusiasm of the researchers Darling describes. Writing of the astronomical search for signs of life far off in the galaxy, he captures the thrill of this work:

Their efforts will revolutionize astrobiology, more so perhaps than spacecraft parachuting down out of the orange sky of Titan or roving the rock-strewn deserts of Mars. The world-shaking headlines of the next twenty years will likely come from giant instruments, on the ground and in Earth orbit, gazing with far sight at the planetary systems of other stars.

Since most research germane to the field has been done here on Earth, Darling explores such hot topics as heat vents and other geothermal mini-biomes, meteoritic dissection, and, of course, SETI's radio telescope arrays. Mars, Venus, and the moons of the outer planets are all major characters, and their stories will reinvigorate most readers' excitement about the prospects of having neighbors just down the cosmic street. Ending with a set of hypotheses and brief explorations of their ramifications if shown to be true, Life Everywhere is an outstanding and thought-provoking look at what could ultimately be the most world-shaking research ever conducted.

The year 2003 was the 50th anniversary of the seminal experiment of Stanley Miller. This was a unique opportunity for highlighting the current interest in this most interdisciplinary subject. The leading space agencies: the European Space Agency (ESA) as well as NASA, the American Space Agency, have planned missions that will elucidate some of the still unknown questions underlying research in the origin of life. New results are surpassing our ability to keep well informed: the reviews that we were presented at the Trieste meeting will bring the readers of this well-documented and timely book up to date in this fast-moving area. An important component of the conference was the review of the Cassini-Huygens mission due to arrive in the Saturn system just one year after the conference convened in Trieste. There was particular interest in the status of the experiments that will take place inside the atmosphere of Titan, the large satellite, which is a testing ground for the theories and experiments in the field of chemical evolution. The Jovian system is currently under study with the view of investigating the possibility of life underneath the frozen surface of the Galilean moon Europa; the ESA mission "Mars Express" and Mars Odyssey received special attention. Some of the world leaders in the field gathered in Trieste in September 2003 - that was a most timely date for reviewing recent data and discussing the prospects of future research. 

The Origin of Life: The Earth is an island, swirling in an ocean of space, and life has been washing ashore since the creation.

Cosmic collisions are commonplace, not only between meteors and planets, but entire galaxies, and life has been repeatedly tossed into the abyss... only to land on other planets.

The genetic seeds of life swarm throughout the cosmos, and these "genetic seeds," these living creatures, fell to Earth encased in stellar debris which pounded the planet for 700 million years after the creation. And these "seeds" contained the DNA instructions for the metamorphosis of all life, including woman and man.

DNA acts to purposefully modify the environment, which acts on gene selection, to fulfill specific genetic goals: the dispersal and activation of silent DNA, and the replication of life forms that long ago lived on other planets.

It is just over ten years since the first planet outside our solar system was detected. Since then, much work has focussed on understanding how extrasolar planets may form, and discovering the frequency of potentially habitable Earth-like planets. This volume addresses fundamental questions concerning the formation of planetary systems in general, and of our solar system in particular. Drawing from recent advances in observational, experimental, and theoretical research, it summarises our current understanding of the planet formation processes, and addresses major open questions and research issues. Chapters are written by leading experts in the field of planet formation and extrasolar planet studies. The book is based on a meeting held at Ringberg Castle in Bavaria, where experts gathered together to present and exchange their ideas and findings. It is a comprehensive resource for graduate students and researchers, and is written to be accessible to newcomers to the field.