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Worlds in the making: The evolution of the universe

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About This Book

The text presents physical explanations for the origin and evolution of Earth and other celestial bodies, linking terrestrial phenomena to astronomical processes. It examines volcanoes, earthquakes, interior heat, atmospheric composition, and the factors that govern planetary habitability and climatic change. It develops solar physics, treating radiation, sunspots, prominences, and the role of radiation pressure in shaping cometary tails, dust, and exchanges of matter. The work addresses aurorae and magnetic disturbances, meteors and meteorites, and draws on observations of nebulae and stellar spectra to discuss nebular structures and collision-driven cosmogony. Physical laws and thermodynamics are applied throughout to account for large-scale cosmic evolution.

About the Author

Arrhenius, Svante portrait

Svante Arrhenius

Svante Arrhenius was a Swedish scientist and a pivotal figure in the field of physical chemistry. He is best known for his groundbreaking work on the theory of electrolytic dissociation, which laid the foundation for modern physical chemistry. Arrhenius also made significant contributions to our understanding of the greenhouse effect and climate change, positing that increased carbon dioxide levels could lead to global warming. His notable works include "The Destinies of the Stars" and "Worlds in the Making: The Evolution of the Universe," where he explores cosmic phenomena and the evolution of the universe. Arrhenius's insights continue to influence scientific thought and environmental discussions today.

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