Presolar Grains in Extra-Terrestrial Materials: Probing Stars with Stardust presents the latest research on presolar grains and their stellar sources in a cohesive resource for bringing researchers in cosmochemistry, astrophysics, and astronomy up to speed on the state-of-the-art developments, analysis, and future implications. Beginning with a historical perspective on the study of presolar grains, the book then reviews the properties and features of a variety of presolar grains, including sililcon carbide, graphite, diamonds, oxides, and silicates. It also includes techniques for analyzing presolar grains in the lab, and covers the stars that are considered sources of presolar grains, such as asymptotic giant branch (AGB) stars, supernovae, novae, and born-again AGB stars. Condensation calculations in various types of stars and minerals observed and/or expected in the stellar atmospheres and presolar grains are also presented.By providing the latest state in the study of of presolar grains and relevant fields of astronomy and astrophysics, Presolar Grains in Extra-Terrestrial Materials serves as an up-to-date summary of data, analysis, and implications of the study of presolar grains and their stellar sources.
Optics of the Moon offers a modern approach to lunar remote sensing. It presents methods for interpreting optics of surfaces with complicated structures, in particular, the lunar regolith. For example, this book illustrates how phase-ratio techniques can lead to the detection of surface structure anomalies and describes polarimetric studies of the lunar surface and their use. This book addresses many questions related to the surfaces of the Moon, such as why the Moon looks like a ball at a large phase angle and like a disk in full moon, why the lunar surface has slight color variations, and why at large phase angles its polarization degree closely correlates with albedo.Including historical perspectives, case studies, maps, and figures to enhance the understanding of both theory and techniques, Optics of the Moon is a valuable resource for researchers and students in lunar and planetary science and remote sensing.
Titan After Cassini-Huygens is the most up-to-date and comprehensive coverage of our knowledge on Titan, including results and insights from the joint NASA/European Space Agency/Italian Space Agency mission Cassini-Huygens and the conclusions drawn by experts following detailed analysis of the mission data. Our knowledge of Titan has increased substantially due to observations from the Cassini-Huygens mission, which ended in 2017. Since then, observations from Earth, as well as laboratory and theoretical studies, have continued to add to our knowledge. These conclusions, combined with the latest ground-based and theoretical research, provide the most recent understanding of the science of Titan, covering the origin and evolution of Titan, its magnetic and plasma environment, surface, interior structure, geology, atmosphere, and the astrobiological potential for the oceans on the moon.The first book of the new COSPAR book series, Titan After Cassini-Huygens, is an integral reference for scientists, researchers, and academics working on Titan or ocean worlds. Part of the COSPAR Book SeriesEdited by Jean-Louis Fellous, former Executive Director of COSPAR (Committee on Space Research; 2008–2019)
Planetary Tectonism across the Solar System, Volume Two in the Comparative Planetology series, addresses key questions surrounding planetary tectonism, such our understanding of the global contraction of Mercury, the formation of giant rift zones on Saturn’s icy moons, or the tesserated terrain on Venus. The book makes connections to Earth, such as how deformation on Mercury is both similar and different, and how to apply theoretical considerations behind plate tectonics on Earth to other planets. The book offers up-to-date, accessible and comprehensive discussions on the major tectonic processes and landforms that shape and drive the evolution of planets, moons and smaller bodies. By placing a singular emphasis on comparing tectonic processes and landforms on all relevant Solar System bodies, with the explicit objective of providing a systems-level understanding of this widespread phenomenon, this book is ideal for anyone studying planetary tectonism.
Magnetohydrodynamic Processes in Solar Plasmas provides a comprehensive theory and practice of basic plasma processes in the Sun and heliosphere. It deals with the basic dynamics of the Sun from its interior up to its outer atmosphere in the framework of Magnetohydrodynamics. Topics covered include essential phenomena in the solar interior such as magnetism, dynamos and helioseismology and in the solar atmosphere such as waves, shocks, instabilities, reconnection and coronal heating. The book provides frontline research aspects of solar plasma processes. In addition, the content is relevant for astrophysical plasmas, laboratory plasmas, fluid dynamics and related basic fields. Magnetohydrodynamic Processes in Solar Plasmas not only focuses on the fundamentals of the processes under consideration but in addition it presents recent research developments. In this manner it forms an essential reference for researchers, academics and advanced students in solar physics, astrophysics and related disciplines.
Astrochemical Modelling: Practical Aspects of Microphysics in Numerical Simulations is a comprehensive and detailed guide to dealing with the standard problems that students and researchers face when they need to take into account astrochemistry in their models, including building chemical networks, determining the relevant processes, and understanding the theoretical challenges and the numerical limitations. The book provides chapters covering the theoretical background on the predominant areas of astrochemistry, with each chapter following theoretical background with information on existing databases, step-by-step computational examples with solutions to recurrent problems, and an overview of the different processes and their numerical implementation. Furthermore, a section on case studies provides concrete examples of computational modelling usage for real-world applications and cases where the techniques can be applied is also included.
Ices in the Solar System: A Volatile-Driven Journey from the Inner Solar System to Its FarReaches explores the origins, evolution and distribution of various ice species throughout thesolar system.Geographically, the book’s focus on ice(s) migrates outwardly from Mercury, the Earth and theMoon, Mars, then Ceres and other volatile-rich small bodies; it carries on with the moons ofJupiter, Saturn, and Uranus, followed by Pluto and other Kuiper Belt/Trans-Neptunian objects.Conceptually and empirically, the book depicts the often-enigmatic narratives of the differentice species (H2O, CO2, CH4, etc.) in the solar system and examines their interaction with a widerange of surface, near-subsurface, interior and atmospheric processes.
The International Astronomical Union formalized the naming of meteor showers in 2006. Each newly discovered shower now is assigned a unique and officially recognized name, number, and 3-letter code. Close to a thousand possible meteor showers have since been reported, over a hundred in the cause of writing this book.Atlas of Earth's Meteor Showers takes stock of all reported detections by going back to the combined video and radar data in hand at the end of 2021, in order to weed out duplicates and false detections. Maps were created that show the direction of motion of meteors (their radiant) during 5-day and 10-day intervals throughout the year. All 500+ showers recognized are briefly described from their radiant, speed, and orbital elements, and the meteoroid mass distribution index was calculated. Physical properties of the meteoroids were derived from their beginning, peak and end height, from their deceleration in Earth's atmosphere, and from spectroscopic information. Candidate parent bodies are mentioned and the age of the stream was calculated from the dispersions in orbital elements and from the meteor magnitude distribution index. A brief history is given of the shower's discovery, of when features were first recognized, and of results from dynamical modeling, all with references to the literature.
Water Worlds in the Solar System: In Search of Habitable Environments and Life is a comprehensive reference on the formation, availability, habitability potential, and astrobiological implications of water in the Solar System. The book provides understanding of the importance of water on Earth to elucidate potential water and biosignature sources on other bodies in the Solar System. It covers processes involved in the formation of Earth and its Moon, genesis of water on those bodies, events on early Earth, and other processes that are applicable to celestial bodies in the Solar System, directly correlating data available on water on other bodies to over 15 Earth analogue sites. This book forms a comprehensive overview on water in the Solar System, from formation to biosignature and habitability considerations. It is ideal for academics, researchers and students working in the field of planetary science, extraterrestrial water research and habitability potential.
Planetary Exploration Horizon 2061: A Long-Term Perspective for Planetary Exploration synthesizes all the material elaborated and discussed during three workshops devoted to the Horizon 2061 foresight exercise. Sections cover the science of planetary systems, space missions to solar system objects, technologies for exploration, and infrastructures and services to support the missions and to maximize their science return. The editors follow the path of the implementation of a planetary mission, from the needed support in terms of navigation and communication, through the handling of samples returned to Earth, to the development of more permanent infrastructures for scientific human outposts on the Moon and Mars. This book also includes a special chapter entirely devoted to contributions from students and early-career scientists: the “Horizon 2061 generation” and a final chapter on important avenues for the actual implementation of the planetary missions coming out of our “Dreams for Horizon 2061”: International cooperation, and the growing role and initiatives of private enterprise in planetary exploration.