Examines the clouds of dust and gas that recycle the remains of dead stars to form new stars

Amazing 3-D images take readers inside the birth and death of stars. This visually amazing volume, with text and 3-D images, takes readers inside the birthplace of stars—the cosmic clouds called nebulae. Nebulae (from the Latin for “cloud” or “fog”) are stellar nurseries, frequently intermingled with clusters of young stars. Seen in the night sky, they glow, energized by the new stars within and around them. Cosmic Clouds 3-D offers hundreds of magnificent images of nebulae captured by ground-based and space telescopes. Along with the high-resolution views of nebulae are unique stereo views that show the nebulae in three dimensions. As we observe the birth of stars in these great clouds of gas, we are peering into the world of infant suns, seeing a process that for our own Sun took place some 4.6 billion years ago. The story of elements in nature, of why we are here, of our cosmic roots, is strongly tied to the story of stars in our galaxy and universe. And that means exploring the lives of stars, how stars come to be, what happens during their lifetimes, and how they, too—like humans—eventually die. We may not all know it, but we are part of the biggest recycling program that exists—the birth, life, and death of stars. A 3-D viewer, designed by astrophysicist (and lead guitarist with the rock group Queen) Brian May, is included with the book.

A 1959 classic 'hard' science-fiction novel by renowned Cambridge astronomer and cosmologist Fred Hoyle. Tracks the progress of a giant black cloud that comes towards Earth and sits in front of the sun, causing widespread panic and death. A select group of scientists and astronomers - including the dignified Astronomer Royal, the pipe smoking Dr Marlowe and the maverick, eccentric Professor Kingsly - engage in a mad race to understand and communicate with the cloud, battling against trigger happy politicians. In the pacy, engaging style of John Wyndham and John Christopher, with plenty of hard science thrown in to add to the chillingly credible premise (he manages to foretell Artificial Intelligence, Optical Character Recognition and Text-to-Speech converters), Hoyle carries you breathlessly through to its thrilling end.

The general background of this monograph and the aim of it is described in detail in Chapter I. As stated in 1.7 it is written according to the principle that "when rigour appears to conflict with simplicity, simplicity is given preference", which means that it is intended for a rather broad public. Not only graduate students but also advanced undergraduates should be able to understand at least most of it. This monograph is the result of many years of inspiring discussions with a number of colleagues, for which I want to thank them very much. Especially I should mention the groups in Stockholm and La Jolla: in Stockholm, Dr Carl-Gunne Flilthammar and many of his collaborators, including Drs Lars Block, Per Carlqvist, Lennart lindberg, Michael Raadu, Staffan Torven, Miroslav Babic, and Itlgvar Axniis, and further, Drs Bo Lehnert and Bjorn Bonnevier, all at the Royal Institute of Technology. Of other col leagues in Sweden, I should mention Dr Bertel Laurent, Stockholm University, Dr Aina Elvius, The Stockholm Observatory, and Dr Bengt Hultqvist, Kiruna. In La Jolla my thanks go first of all to Dr Gustaf Arrhenius, who once invited me to La Jolla, which was the start of a most interesting collaboration; further, to Dr W.B.

Physics of the Inner Heliosphere gives for the first time a comprehensive and complete summary of our knowledge of the inner solar system. Using data collected over more than 11 years by the HELIOS twin solar probes, one of the most successful ventures in unmanned space exploration, the authors have compiled six extensive reviews of the physical processes of the inner heliosphere and their relation to the solar atmosphere. Researchers and advanced students in space and plasma physics, astronomy, and solar physics will be surprised to see just how closely the heliosphere is tied to, and how sensitively it depends on, the sun. Volume 2 deals with particles, waves, and turbulence, with chapters on: - magnetic clouds - interplanetary clouds - the solar wind plasma and MHD turbulence - waves and instabilities - energetic particles in the inner solar system

The most important popular science book since James Lovelock's Gaia.

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