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The Earth's Beginning

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About This Book

A concise survey of hypotheses for the solar system's origin, presenting the nebular theory and examining the difficulty of sustaining solar heat over geological time. The text contrasts contraction-based explanations with recently discovered internal energy sources, arguing that radioactive processes could supply long-term solar radiation. It marshals geological and chemical evidence, including estimates of ocean salinity accumulation, to support great antiquity, and reviews observational advances that elevate the importance of spiral nebulae. Astronomy, geology, and emerging experimental physics are woven together to explain planetary formation and the persistence of solar energy.

About the Author

Ball, Robert S. portrait

Robert S. Ball

Robert S. Ball was a prominent figure in the field of astronomy and mechanics, known for his engaging lectures and writings aimed at both scientific and general audiences. He delivered a series of influential lectures at the Royal College of Science for Ireland, which were later compiled into his book "Experimental Mechanics." Ball's works often explored the wonders of the universe, as seen in titles like "Great Astronomers" and "Star-land: Being Talks With Young People About the Wonders of the Heavens." His contributions to popular science literature helped to inspire a fascination with astronomy and the natural world.

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