An Introduction to the Chemistry of the Atmospheres of Earth, the Planets, and Their Satellites
Author: Richard Peer Wayne
Publisher: Oxford University Press on Demand
' This popular book introduces chemists to the chemistry of the atmospheres of the earth and other planets. In the new edition of the chapter on stratosphere chemistry has been update to reflect our improved understanding of the catalytic cycles that destroy ozone, and the importance of heterogeneous chemistry' Aslib
Chemistry is covered at just the right depth for students to develop a thorough understanding of natural processes.Chemical processes shape the world we live in; the air we breathe, the water we drink, the weather we experience. Guiding us through the chemical composition of the three key environmental systems; the atmosphere, hydrosphere, and terrestrial environment; the authors explain the chemical processeswhich occur within and between each system, allowing for better understanding of how they behave. We then see how human activity continues to affect the chemical behaviour of these environmental systems, and what the consequences of these natural processes being disturbed can be.
Planetary atmospheres is a relatively new, interdisciplinary subject that incorporates various areas of the physical and chemical sciences, including geophysics, geophysical fluid dynamics, atmospheric science, astronomy, and astrophysics. Providing a much-needed resource for this cross-disciplinary field, An Introduction to Planetary Atmospheres presents current knowledge on atmospheres and the fundamental mechanisms operating on them. The author treats the topics in a comparative manner among the different solar system bodies—what is known as comparative planetology. Based on an established course, this comprehensive text covers a panorama of solar system bodies and their relevant general properties. It explores the origin and evolution of atmospheres, along with their chemical composition and thermal structure. It also describes cloud formation and properties, mechanisms in thin and upper atmospheres, and meteorology and dynamics. Each chapter focuses on these atmospheric topics in the way classically done for the Earth’s atmosphere and summarizes the most important aspects in the field. The study of planetary atmospheres is fundamental to understanding the origin of the solar system, the formation mechanisms of planets and satellites, and the day-to-day behavior and evolution of Earth’s atmosphere. With many interesting real-world examples, this book offers a unified vision of the chemical and physical processes occurring in planetary atmospheres. Ancillaries are available at www.ajax.ehu.es/planetary_atmospheres/
Building on the first principles of environmental chemistry, engineering, and ecology, this volume fills the need for an advanced textbook introducing the modern, integrated environmental management approach, with a view towards long-term sustainability and within the framework of international regulations. As such, it presents the classic technologies alongside innovative ones that are just now coming into widespread use, such as photochemical technologies and carbon dioxide sequestration. Numerous case studies from the fields of air, water and soil engineering describe real-life solutions to problems in pollution prevention and remediation, as an aid to practicing professional skills. With its tabulated data, comprehensive list of further reading, and a glossary of terms, this book doubles as a reference for environmental engineers and consultants.
Physics and Chemistry of the Solar System focuses on planetary physics and chemistry. This book consists of 12 chapters. Chapters I to IV cover the general properties and environment of the planetary system. The solar system beyond Mars is elaborated in Chapters V to VIII, while the inner solar system is considered in Chapters XI to XII. In these chapters, this compilation specifically discusses the limitations on big bang nucleosynthesis; structure and classification of galaxies; and mass and angular momentum distribution. The radio wave propagation in space plasmas; interiors of Jupiter and Saturn; density and composition of icy satellites; and evaporation and non-gravitational forces are also deliberated. This text also explains the physical properties of meteorites; geology of the Moon; geophysical data on Mars; and search for extraterrestrial intelligence. This publication is a good reference for first-year graduate students who intend to take graduate courses in specialized areas of planetary sciences, as well as practicing Ph.D. scientists with training in physics, chemistry, geology, astronomy, meteorology, and biology.
Chemical Evolution of the Giant Planets is a compilation of papers on the chemical evolution of giant planets, presented at a colloquium sponsored by the Laboratory of Chemical Evolution in October, 1974. The compendium focuses on the interpretation of data provided by the Pioneer 10 and 11 missions, which conducted explorations of the outer planets. Scientists from various disciplines tackle the various aspects of the study of the chemical environment of the giant planets and their satellites. Subjects such as the atmosphere of Jupiter and Saturn; chemical abundances in the atmospheres of the giant planets and their satellites; possibility of growth of airborne microbes in outer planetary atmospheres; and the biology on the outer planets are covered in the book. Astronomers, chemists, geologists, and biologists will find the book interesting.