Understanding The New Solar System

This volume reveals the latest knowledge of the composition and nature of our solar family. Here you'll discover what lies beyond the orbit of Pluto, which solar body is the most volcanically active, and which solar system bodies have atmospheres and may harbour primitive life.

The solar system - our sun and the planets and other bodies that orbit it - has remained essentially the same for hundreds of millions of years. What, then, is the New Solar System? Quite simply what's new is our understanding of what in fact makes up the solar system, and our deeper understanding of long-known objects such as the planets, their satellites, comets and asteroids. The ancient Romans observed and noted the motions of the known planets at that time but it wasn't until 1781 that Uranus was discovered. Neptune was discovered in 1846 and Pluto was discovered in 1930. Pluto's moon, CHARON, was only discovered in 1978, or about the time that robotic exploration of the solar system became a serious undertaking. UNDERSTANDING THE NEW SOLAR SYSTEM reveals the latest knowledge of the composition and nature of our solar family. Here you'll discover what lies beyond the orbit of Pluto, which solar body is the most volcanically active, and which solar system bodies have atmospheres and may harbour primitive life, and much, much more.

This volume reveals the latest knowledge of the composition and nature of our solar family. Here you'll discover what lies beyond the orbit of Pluto, which solar body is the most volcanically active, and which solar system bodies have atmospheres and may harbour primitive life.

This volume reveals the latest knowledge of the composition and nature of our solar family. Here you'll discover what lies beyond the orbit of Pluto, which solar body is the most volcanically active, and which solar system bodies have atmospheres and may harbour primitive life.

Exploration by space probes has revealed many fascinating details about Earth’s planetary neighbours. Today we stand on the threshold of the next phase of planetary exploration and knowledge, with several space probe missions currently underway and others being planned. Probing the New Solar System discusses the latest findings that have contributed to a changed understanding of the solar system – and how the revised definition of a planet in 2006 by the International Astronomical Union affected this understanding. Each chapter includes some historical information, ‘Did you know?’ items of particular interest to readers, and photographs of objects in the solar system showing newly discovered features of the planets, their moons and of dwarf planets. This is an up-to-date record of the many recent discoveries made about our solar system and other planetary systems using ground-based and space probe technology. It has been written for people interested in astronomy, both professional and amateur, as well as for students and educators.

A new frontier in our solar system opened with the discovery of the Kuiper Belt and the extensive population of icy bodies orbiting beyond Neptune. Today the study of all of these bodies, collectively referred to as trans-Neptunian objects, reveals them to be frozen time capsules from the earliest epochs of solar system formation. This new volume in the Space Science Series, with one hundred contributing authors, offers the most detailed and up-to-date picture of our solar systemÕs farthest frontier. Our understanding of trans-Neptunian objects is rapidly evolving and currently constitutes one of the most active research fields in planetary sciences. The Solar System Beyond Neptune brings the reader to the forefront of our current understanding and points the way to further advancement in the field, making it an indispensable resource for researchers and students in planetary science.

A modern introduction to the solar system incorporates the latest research and technology, providing beginner-level stargazers with a removable turn-the-wheel planisphere and coverage of the 2005 debate about planet definitions.

This book's interdisciplinary scope aims at bridging various communities: 1) cosmochemists, who study meteoritic samples from our own solar system, 2) (sub-) millimetre astronomers, who measure the distribution of dust and gas of star-forming regions and planet-forming discs, 3) disc modellers, who describe the complex photo-chemical structure of parametric discs to fit these to observation, 4) computational astrophysicists, who attempt to decipher the dynamical structure of magnetised gaseous discs, and the effects the resulting internal structure has on the aerodynamic re-distribution of embedded solids, 5) theoreticians in planet formation theory, who aim to piece it all together eventually arriving at a coherent holistic picture of the architectures of planetary systems discovered by 6) the exoplanet observers, who provide us with unprecedented samples of exoplanet worlds. Combining these diverse fields the book sheds light onto the riddles that research on planet formation is currently confronted with, and paves the way for a comprehensive understanding of the formation, evolution, and dynamics of young solar systems. The chapters ‘Chondrules – Ubiquitous Chondritic Solids Tracking the Evolution of the Solar Protoplanetary Disk’, ‘Dust Coagulation with Porosity Evolution’ and ‘The Emerging Paradigm of Pebble Accretion’ are published open access under a CC BY 4.0 license via link.springer.com.