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.
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