Rosaly M.C. Lopes – författare

Planetary Volcanism across the Solar System compares and contrasts the vast array of planetary bodies in the Solar System, including Earth. The wealth of spacecraft data for almost all major solid-surface bodies in the Solar System indicate that volcanism has been a dominant mechanism in shaping the landscapes of these bodies. The book addresses key questions surrounding our understanding of planetary volcanism, such as how to integrate the data into a coherent view of how volcanic activity arises, how this mechanism shapes planets, which volcanic landforms are ubiquitous throughout the Solar System, and which are unique.

By placing a singular emphasis on comparing volcanic processes and landforms on all relevant Solar System bodies, and with the explicit objective of providing a systems-level understanding of this widespread phenomenon, users will find an up-to-date, accessible and comprehensive discussion of the major volcanic processes and landforms that shape and drive the evolution of planets, moons and smaller bodies.

Includes an introduction placing the book in the context of the larger Comparative Planetology series Compares volcanic processes and landforms on all relevant Solar System bodies, providing a systems-level understanding of this widespread phenomenon Offers a thorough examination of the major volcanic processes and landforms that shape and drive the evolution of planets, moons and smaller bodies Includes information from new mission data and discoveries in recent years Features over 100 color illustrations and charts to more clearly convey concepts Offers additional online content, including figures, animations, video, and other multimedia content such as interviews with contributing authors

Planetary Volcanism across the Solar System compares and contrasts the vast array of planetary bodies in the Solar System, including Earth. The wealth of spacecraft data for almost all major solid-surface bodies in the Solar System indicate that volcanism has been a dominant mechanism in shaping the landscapes of these bodies. The book addresses key questions surrounding our understanding of planetary volcanism, such as how to integrate the data into a coherent view of how volcanic activity arises, how this mechanism shapes planets, which volcanic landforms are ubiquitous throughout the Solar System, and which are unique.By placing a singular emphasis on comparing volcanic processes and landforms on all relevant Solar System bodies, and with the explicit objective of providing a systems-level understanding of this widespread phenomenon, users will find an up-to-date, accessible and comprehensive discussion of the major volcanic processes and landforms that shape and drive the evolution of planets, moons and smaller bodies.- Includes an introduction placing the book in the context of the larger Comparative Planetology series- Compares volcanic processes and landforms on all relevant Solar System bodies, providing a systems-level understanding of this widespread phenomenon- Offers a thorough examination of the major volcanic processes and landforms that shape and drive the evolution of planets, moons and smaller bodies- Includes information from new mission data and discoveries in recent years- Features over 100 color illustrations and charts to more clearly convey concepts- Offers additional online content, including figures, animations, video, and other multimedia content such as interviews with contributing authors

**2026 PROSE Award Finalist in Chemistry, Physics, Astronomy, and Cosmology**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)

Details the total knowledge of Titan from Cassini-Huygens and subsequent observations from Earth, as well as laboratory and theoretical studies from the last decadeCovers all aspects of Titan, including origin and evolution, magnetic and plasma environment, surface, interior structure, geology, atmospheric science and astrobiological potentialProvides detailed, referenceable data from investigators of the Cassini spacecraft and Huygens probe, as well as the ALMA radio telescope observatory

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)- Details the total knowledge of Titan from Cassini-Huygens and subsequent observations from Earth, as well as laboratory and theoretical studies from the last decade- Covers all aspects of Titan, including origin and evolution, magnetic and plasma environment, surface, interior structure, geology, atmospheric science and astrobiological potential- Provides detailed, referenceable data from investigators of the Cassini spacecraft and Huygens probe, as well as the ALMA radio telescope observatory

Written by active research scientists who study the volcanism of Earth and of other planets, the contributions provide the first general review of volcanic activity throughout the Solar System. Successive chapters describe past and present volcanic activity as it is observed throughout the Solar System. These chapters relate to readers not only our present knowledge of volcanism throughout the Solar System but also how frontline scientists working in this field conduct their research.

Written by experts in the field, many of whom took part in the Galileo mission, the book reviews the basics about Io and its unique space environment. Coverage includes all subjects, where the Galilio mission has shed new light on, with some emphasis on Io''s most remarkable characteristics: its active volcanism. Written primarily for planetary scientists this book will also benefit volcanologists in general and newcomers wishing to specialize in this field of research.

Written by active research scientists who study the volcanism of Earth and of other planets, the contributions provide the first general review of volcanic activity throughout the Solar System. Successive chapters describe past and present volcanic activity as it is observed throughout the Solar System. These chapters relate to readers not only our present knowledge of volcanism throughout the Solar System but also how frontline scientists working in this field conduct their research.