the-chemical-cosmos

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If you have ever wondered how we get from the awesome impersonality of the Big Bang universe to the point where living creatures can start to form, and evolve into beings like you, your friends and your family, wonder no more. Steve Miller provides us with a tour through the chemical evolution of the universe, from the formation of the first molecules all the way to the chemicals required for life to evolve. Using a simple Hydrogen molecule – known as H-three-plus - as a guide, he takes us on a journey that starts with the birth of the first stars, and how, in dying, they pour their hearts out into enriching the universe in which we live. Our molecular guide makes its first appearance at the source of the Chemical Cosmos, at a time when only three elements and a total of 11 molecules existed. From those simple beginnings, H-three-plus guides us down river on the violent currents of exploding stars, through the streams of the Interstellar Medium, and into the delta where new stars and planets form. We are finally left on the shores of the sea of life. Along the way, we meet the key characters who have shaped our understanding of the chemistry of the universe, such as Cambridge physicist J.J. Thomson and the Chicago chemist Takeshi Oka. And we are given an insider’s view of just how astronomers, making use of telescopes and Earth-orbiting satellites, have put together our modern view of the Chemical Cosmos.

To accompany "Cosmos" by Carl Sagan.

Earth and Cosmos presents a comprehensive view of the many connections between the environment of Man on Earth and the environment of the Earth in the cosmos. Topics covered range from matter, radiation, and the basic forces of nature to Earth's relation to the universe, the galaxy, and the sun. The energy balance and global circulation of the atmosphere are also discussed, along with continents, oceans, and climate. This book is comprised of 13 chapters and begins with an overview of the environment of Man on Earth, with emphasis on the Earth's chemical composition and how it is related to both cosmic and terrestrial processes; the radiation environment at the Earth's surface and above; how the atmosphere interacts with both solar and terrestrial radiation; and climate. The following chapters explore matter, radiation, and the laws of nature in relation to the universe; how the terrestrial environment is related to the structure of the universe as a whole; how the composition of the solar system and the Earth reflects the history of the galaxy; and the stability of the Earth's environment. The origins of life on Earth and the impact of human activities on the planet are also considered. The last chapter speaks of the future of humanity, and notably of the problem of the population explosion and its consequences. This monograph will be of interest to students, astronomers, planetary scientists, astrophysicists, biologists, chemists, and geologists.

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