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In the 12 years since the first discovery of an exoplanet around a main sequence star (51 Peg), more than 270 exoplanets have been detected. The proceedings of IAU Symposium 249 present the latest theoretical and observational advances in the field of exoplanet research, including the ongoing and future projects such as CoRoT and Kepler. The volume opens with a review of exoplanet detection and orbital determination techniques, before looking at the physics of gas giant atmospheres and close-in stars. The topics of planet formation, migration and the dynamical evolution of protoplanetary disks and multi-planet systems are also covered in detail. IAU S249 is a useful reference for the graduate students and researchers working in the exciting field of exoplanet study.
This latest, up-to-date resource for research on extrasolar planets covers formation, dynamics, atmospheres and detection. After a look at the formation of giant planets, the book goes on to discuss the formation and dynamics of planets in resonances, planets in double stars, atmospheres and habitable zones, detection via spectra and transits, and the history and prospects of ESPs as well as satellite projects. Edited by a renowned expert in solar system dynamics with chapters written by the leading experts in the method described -- from the US and Europe -- this is an ideal textbook for graduates, students in astronomy, and astronomers.
This is the first collection of review articles in one volume covering the very latest developments in exoplanet research. This edited, multi-author volume will be an invaluable introduction and reference to all key aspects in the field this field. The reviews cover topics such as the properties of known exoplanets and searching for exoplanets in the stellar graveyard. The book provides an easily accessible point of reference in a fast moving and exciting field.
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 zon
Science and Faith in Dialogue presents a cogent, compelling case for concordance between science and theism. The term theism refers, in this book, to the belief in God's existence. Within theology, the term theism is often used to convey a range of presuppositions about the nature and attributes of God. Based on scientific and natural theological perspectives, two pillars of natural theology are revisited: the Cosmological Argument and the Argument from Design. The book argues that modern science provides undeniable evidence and a scientific basis for these classical arguments to infer a rationally justifiable endorsement of theism as being concordant with reason and science – nature is seen as operating orderly on comprehensible, rational, consistent laws, in line with the conviction that God is Creator.
A complete record of the formal organisational and administrative proceedings of the XXVII General Assembly of the International Astronomical Union.
This discovery of several Earth-like planets within the habitable zones of their host stars has triggered extensive research on the formation, dynamical evolution, interior dynamics, and atmospheric characteristics of extrasolar habitable planets. IAU Symposium 293 presents a collection of articles on the state-of-the-art research on these topics, including new discoveries of habitable exoplanets. The volume starts by reviewing the current state of the detection of habitable planets, and after guiding the reader through the most recent theoretical and observational achievements on the discovery and understanding of potential life-harboring bodies, concludes by presenting the reader with a review of the upcoming missions that search for Earth-like planets around other stars, and the likely signatures of extraterrestrial life. This comprehensive, up-to-date and technical volume targets those seeking to understand the origin of life and the possibility and detection of life elsewhere in the Universe.
Over the past ten years, the discovery of extrasolar planets has opened a new field of astronomy, and this area of research is rapidly growing, from both the observational and theoretical point of view. The presence of many giant exoplanets in the close vicinity of their star shows that these newly discovered planetary systems are very different from the solar system. New theoretical models are being developed in order to understand their formation scenarios, and new observational methods are being implemented to increase the sensitivity of exoplanet detections. In the present book, the authors address the question of planetary systems from all aspects. Starting from the facts (the detection of more than 300 extraterrestrial planets), they first describe the various methods used for these discoveries and propose a synthetic analysis of their global properties. They then consider the observations of young stars and circumstellar disks and address the case of the solar system as a specific example, different from the newly discovered systems. Then the study of planetary systems and of exoplanets is presented from a more theoretical point of view. The book ends with an outlook to future astronomical projects, and a description of the search for life on exoplanets. This book addresses students and researchers who wish to better understand this newly expanding field of research.
Recent years have seen a dramatic increase in our understanding of planetary systems. Initially, new exoplanets were discovered through the effects they have on their parent stars - whether through radial velocity, transits or microlensing methods - but now the technology and the techniques have been developed to image light from exoplanets directly. Vast improvements have also been made in our ability to resolve circumstellar matter from protoplanetary disks, through transition disks to debris disks. These dramatic new observations have led to new advances in our theoretical understanding of the formation and evolution of planetary systems. The proceedings of IAU Symposium 299 report on recent results of this field covering the range from the detailed imaging of protoplanetary disks to the modeling of planetary atmospheres. The volume benefits both active researchers and graduate students entering this dynamic and rapidly progressing field.