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This second edition is a great enhancement of literature which will help the reader get deeper into the specific topics. There are new sections included such as space weather data sources and examples, new satellite missions, and the latest results. At the end a comprehensive index is given which will allow the reader to quickly find his topics of interest. The Sun and Space weather are two rapidly evolving topics. The importance of the Sun for the Earth, life on Earth, climate and weather processes was recognized long ago by the ancients. Now, for the first time there is a continuous surveillance of solar activity at nearly all wavelengths. These data can be used to improve our understanding of the complex Sun-Earth interaction. The first chapters of the book deal with the Sun as a star and its activity phenomena as well as its activity cycle in order to understand the complex physics of the Sun-Earth system. The reader will see that there are many phenomena but still no definite explanations and models exist for many of them. Other topics are the influences on the Earth’s atmosphere, long and short term climate variations. The last chapters discuss the protection against enhanced radiation environment in view of upcoming manned missions to the Moon and Mars, and the threat from space debris, asteroids and meteoroids. Since the field is quite interdisciplinary, the book will be of interest to scientists working in different fields such as solar physics, geophysics, and space physics.
Space environment. --- Meteorology. --- Solar radiation. --- Sun. --- Absorption, Atmospheric --- Atmospheric absorption of solar radiation --- Insolation --- Radiation, Solar --- Electromagnetic waves --- Aerology --- Earth sciences --- Atmosphere --- Environment, Space --- Extraterrestrial environment --- Space weather --- Extreme environments --- Solar system --- Atmospheric science
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The solar system has a rather well-known history. Looking at the present situation, one might get the impression that it was a rather stable and well-defined system: the orbits of the planets appear to be stable, climate and atmospheres on the planets have been determined, the risk of collision with other bodies (comets, asteroids, meteorites) seems to be small. However it is known today that the evolution of life on Earth was neither a steady progression nor uniform. There were several periods of mass extinction. These catastrophic events played a crucial role in the rise of new species. Events of astrophysical origin include: • Asteroid impacts • Major solar variabilty (space weather) • Nearby supernovae • The passage of the solar system through dense interstellar clouds Catastrophic cosmic events of this type appear in the range of some 100 million years. The author discusses whether and how such events could have occurred in the solar system as well as in recently found extrasolar planetary systems. In this text, which addresses readers in the field of Astrophysics and Astrobiology but also Geophysics and Biology these cosmic catastrophic events are described at an intermediate student's level.
Astrophysics. --- Life on other planets. --- Natural disasters. --- Habitable planets --- Exobiology --- Natural disasters --- Catastrophes (Geology) --- Astrophysics --- Life on other planets --- Astronomy & Astrophysics --- Biology --- Physical Sciences & Mathematics --- Health & Biological Sciences --- Biology - General --- Habitable planets. --- Exobiology. --- Extraterrestrial life --- Astronomical physics --- Natural calamities --- Astrobiology --- Earth-like planets --- Earthlike planets --- Physics. --- Planetology. --- Space sciences. --- Astrobiology. --- Climate change. --- Radiation protection. --- Radiation --- Astrophysics and Astroparticles. --- Extraterrestrial Physics, Space Sciences. --- Climate Change. --- Effects of Radiation/Radiation Protection. --- Safety measures. --- Astronomy --- Cosmic physics --- Physics --- Planets --- Fermi's paradox --- Historical geology --- Disasters --- Life --- Extrasolar planets --- Origin --- Climatic changes. --- Environmental protection. --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Changes, Climatic --- Changes in climate --- Climate change --- Climate change science --- Climate changes --- Climate variations --- Climatic change --- Climatic changes --- Climatic fluctuations --- Climatic variations --- Global climate changes --- Global climatic changes --- Climatology --- Climate change mitigation --- Teleconnections (Climatology) --- Planetary sciences --- Planetology --- Environmental quality management --- Protection of environment --- Environmental sciences --- Applied ecology --- Environmental engineering --- Environmental policy --- Environmental quality --- Environmental aspects --- Radiation—Safety measures. --- Radiation monitoring --- Radiation protection --- Science and space --- Space research --- Cosmology --- Science --- Global environmental change
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Due to its specific chemical and physical properties, water is essential for life on Earth. And it is assumed that this would be the case for extraterrestrial life as well. Therefore it is important to investigate where water can be found in the Universe. Although there are places that are completely dry, places where the last rainfall happened probably several 100 million years ago, surprisingly this substance is quite omnipresent. In the outer solar system the large satellites of Jupiter and Saturn are covered by a thick layer of ice that could be hiding a liquid ocean below. This of course brings up the question of whether the recently detected extrasolar planets could have some water on their surfaces and how we can detect this. Water molecules are also found in interstellar gas and dust clouds. This book begins with an introductory chapter reviewing the physical and chemical properties of water. Then it illuminates the apparent connection between water and life. This is followed by chapters dealing with our current knowledge of water in the solar system, followed by a discussion concerning the potential presence and possible detection of water on exoplanets. The signature of water in interstellar space and stars are reviewed before the origin of water in the Universe is finally discussed. The book ends with an appendix on detection methods, satellite missions and astrophysical concepts touched upon in the main parts of the book. The search for water in the Universe is related to the search for extraterrestrial life and is of fundamental importance for astrophysics, astrobiology and other related topics. This book therefore addresses students and researchers in these fields.
Interstellar hydrogen. --- Cosmochemistry. --- Space environment. --- Planets. --- Solar system. --- Environment, Space --- Extraterrestrial environment --- Space weather --- Astrochemistry --- Cosmic chemistry --- Space chemistry --- Astronomy. --- Astrobiology. --- Astronomy, Astrophysics and Cosmology. --- Water, general. --- Milky Way --- Extreme environments --- Chemistry --- Space sciences --- Hydrogen --- Interstellar matter --- Astrobiology --- Biology --- Habitable planets --- Life --- Origin --- Astrophysics. --- Water. --- Hydrology --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Outer space.
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This book offers an overview of solar physics with a focus on solar activity, particularly the activity cycle. It is known that solar activity varies periodically, but there are also phases of intermittency, such as the Maunder minimum, during which solar activity is very low or high over several decades. The book provides a brief introduction to chaos theory and investigates solar activity in terms of its chaotic behavior. It also discusses how intermittent phases of solar activity have affected and can affect Earth’s climate and long-term space weather, and reviews the underlying theories relating to the solar dynamo mechanism. Furthermore, each chapter includes references to scientific literature (review articles and papers) so that readers can delve deeper into the subjects covered. This richly illustrated book will appeal to a wide readership, and is also useful as a textbook for courses in solar physics and astrophysics.
Solar system. --- Geophysics. --- Solar and Heliospheric Physics . --- Geophysics/Geodesy. --- Geological physics --- Terrestrial physics --- Earth sciences --- Physics --- Solar cycle. --- Cycle, Sunspot --- Sun-spot cycle --- Sun-spot period --- Sunspot cycle --- Sunspot period --- Cycles --- Solar activity
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Astrobiology refers to the study of the origin, evolution, distribution, and future of life in the universe. This encompasses extraterrestrial life and life on Earth. Astrobiology is an interdisciplinary field that is gaining a rapidly growing interest among both the general public and the astronomical research community. This e-book explains the detection and evolution of exoplanets and discusses the question of habitability on such objects. Chapters in this text include cited references enabling the reader to acquire more information on specific aspects of astrobiology. It is also a suitable
Exobiology. --- Life on other planets. --- Astrobiology --- Biology --- Habitable planets --- Life --- Extraterrestrial life --- Planets --- Fermi's paradox --- Origin
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In this work, Prof. Arnold Hanslmeier provides modern and fascinating astronomical knowledge. The book begins with a description of the origin of the universe and goes on to dark matter, black holes and the formation of the solar system. Finally, it is rounded off at the end by the exciting question: Are we alone in the universe? In this book, which originated from a lecture given at the University of Graz for students of all faculties, the author explains the interrelationships clearly and in a generally understandable way with the help of many colorful pictures, without demanding too much basic knowledge of mathematics and physics. Somewhat deeper formulas and text passages are separated from the rest of the text and can be skipped without losing the context. This third edition incorporates new findings such as the spectacular direct discovery of gravitational waves, fascinating images and data from Pluto, and the first landing on a comet. Numerous new photographs and illustrations have been added to aid understanding. The latest data in the field of exoplanet research has also been incorporated. The book is intended not only for students, but also for interested laymen as well as for all those who deal with modern findings of natural science. "Physics, especially astrophysics, can be extremely exciting, I hope my readers gain just that impression by reading this book!" A. Hanslmeier The author Professor Arnold Hanslmeier is an astrophysicist at the Institute of Physics at the University of Graz. In addition to more than 400 scientific publications and several reference books, he also devotes himself very much to the comprehensible dissemination of the fascinating findings of modern astrophysics. He lectures at the University of Graz and is a visiting professor at the Universities of Vienna, Innsbruck, Toulouse, La Laguna, Tenerife and the Kiepenheuer Institute in Freiburg. Due to his special didactic abilities to present complicated things in a simple and clear way, he is an internationally sought-after speaker.
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This textbook provides the basic theoretical and practical knowledge of astronomy and astrophysics. It provides an overview from classical astronomy and observational methods to solar physics and astrophysics of stars and galaxies. It concludes with chapters on cosmology, astrobiology, and mathematical and numerical methods. Numerous color illustrations, examples of calculations, and exercises with solutions make this work a useful companion to undergraduate astronomy lectures. The book is suitable for students of physics and astronomy at teacher training level or in the Bachelor's degree - but also people interested in natural sciences with appropriate basic knowledge of mathematics and physics will find here an appealing introduction to the subject. This fourth edition has been updated and revised with respect to the latest developments in astronomy. The chapter on mathematical methods has been redesigned and the software used is now exclusively Python. Contents: Spherical Astronomy - History of Astronomy - Celestial Mechanics - Astronomical Instruments - Physics of Solar System Bodies - The Sun - State Variables of Stars - Stellar Atmospheres - Stellar Structure - Stellar Evolution - Interstellar Matter - The Galaxy - Extragalactic Systems - Cosmology - Astrobiology - Mathematical Methods This book is a translation of the original German 4th edition Einführung in Astronomie und Astrophysik by Arnold Hanslmeier, published by Springer-Verlag GmbH Germany, part of Springer Nature in 2020. The translation was done with the help of artificial intelligence (machine translation by the service DeepL.com). A subsequent human revision was done primarily in terms of content, so that the book will read stylistically differently from a conventional translation. Springer Nature works continuously to further the development of tools for the production of books and on the related technologies to support the authors.
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UV radiation is an important part in the electromagnetic spectrum since the energy of the photons is great enough to produce important chemical reactions in the atmospheres of planets and satellites of our Solar System, thereby affecting the transmission of this radiation to the ground and its physical properties. Scientists have used different techniques (balloons and rockets) to access to the information contained in this radiation, but the pioneering of this new frontier has not been free of dangers. The Sun is our main source of UV radiation and its description occupies the first two chapters of the book. The Earth is the only known location where life exists in a planetary system and therefore where the interaction of living organism with UV radiation can be tested through different epochs and on distinct species. The development of the human technology has affected the natural shield of ozone that protects complex lifeforms against damaging UV irradiation. The formation of the ozone hole and its consequences are described, together with the possible contribution of UV radiation to recent climate changes. Finally, we will discuss the potential role of ultraviolet light in the development of life on bodies such as Mars, Europa and Titan. The Solar System is not isolated; other external sources can contribute to the enhancement of the UV radiation in our environment. The influence of such events as nearby supernovae and gamma-ray bursts are described, together with the consequences to terrestrial life from such events.
Ultraviolet radiation. --- Solar radiation. --- Astrophysics. --- Solar system. --- Milky Way --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Absorption, Atmospheric --- Atmospheric absorption of solar radiation --- Insolation --- Radiation, Solar --- Electromagnetic waves --- Black light --- Light, Black --- Light, Ultraviolet --- Rays, Ultraviolet --- U-V light --- U-V radiation --- U-V rays --- Ultra-violet radiation --- Ultra-violet rays --- Ultraviolet light --- Ultraviolet rays --- UV light --- UV radiation --- UV rays --- Radiation --- Astrobiology. --- Oncology. --- Climatic changes. --- Environmental protection. --- Astrophysics and Astroparticles. --- Astronomy, Observations and Techniques. --- Cancer Research. --- Climate Change. --- Effects of Radiation/Radiation Protection. --- Environmental quality management --- Protection of environment --- Environmental sciences --- Applied ecology --- Environmental engineering --- Environmental policy --- Environmental quality --- Changes, Climatic --- Changes in climate --- Climate change --- Climate change science --- Climate changes --- Climate variations --- Climatic change --- Climatic changes --- Climatic fluctuations --- Climatic variations --- Global climate changes --- Global climatic changes --- Climatology --- Climate change mitigation --- Teleconnections (Climatology) --- Tumors --- Astrobiology --- Biology --- Habitable planets --- Life --- Environmental aspects --- Origin --- Observations, Astronomical. --- Astronomy—Observations. --- Cancer research. --- Climate change. --- Radiation protection. --- Radiation—Safety measures. --- Radiation monitoring --- Radiation protection --- Cancer research --- Astronomical observations --- Observations, Astronomical --- Global environmental change
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This volume covers aspects of life on Earth with all its diversity and the possibilities of extraterrestrial life. It presents contributions by experts from 20 countries who discuss astrobiology emphasizing life “as we know it” to extraterrestrial places. In the chapters on life in the Cosmos, the authors emphasized in particular certain planets and satellites within the Solar System. On Earth, life also exists at the edge with harsh limitations (such as extremophiles growing in severe environments). Some chapters address the extremophiles in niches of microbial life in terrestrial halo-environments, the local life without water, and the dormancy of polar cyanobacteria, while others focus on microorganisms dwelling in severe conditions such as lava caves. All those conditions of harsh environments, including the Antarctic biota, could serve as analogues for other planets. Special stress is given to the frozen worlds of Mars; Europa, the satellite of Jupiter; and life in the Saturn neighborhood with its moon Titan. The subsurface under the icy layers of these celestial bodies may contain large oceans that have extant or extinct microbial life. Other chapters discuss the habitability of exoplanets, Galacticpanspermia, molecules, and prokaryotes below the planetary surface, halophile life in the Universe, and the SETI search for extraterrestrial intelligence in the Cosmos.
Exobiology. --- Physics. --- Astronomy. --- Astrophysics. --- Cosmology. --- Astrobiology. --- Astrophysics and Astroparticles. --- Astronomy, Astrophysics and Cosmology. --- Astrobiology --- Biology --- Habitable planets --- Life --- Origin --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics
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The book contains lecture papers and contributed papers on different aspects of magnetic phenomena in the solar atmosphere. The main topics addressed are the physics of solar flares, prominences, coronal mass ejections, magnetic helicity, high-energy radiation from the Sun, observations of the photosphere and chromosphere as well as highlights from the SOHO mission. The lecture papers provide a very valuable introduction and overview on recent developments in these fields of solar physics. The comprehensive lists of references at the end of each review enable the interested reader to go into m
Solar magnetic fields --- Solar radiation --- Astronomy. --- Astrophysics. --- Astronomy, Astrophysics and Cosmology. --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Space sciences. --- Science and space --- Space research --- Cosmology --- Science
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