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An original theory or new hypothesis of the universe / cover

An original theory or new hypothesis of the universe /

Presented as nine letters, the work develops a mathematical hypothesis that interprets the Milky Way as a flattened, system-like arrangement of stars and extends that model to the sizes, motions, and distances of planets, stars, and nebulae. It assesses observational evidence and degrees of probability, offers estimates of cosmic scale, and argues that many faint nebulae are remote, galaxy-like systems. Throughout, the author connects these cosmological ideas to questions of order, final causes, and the theological and moral implications of a vast hierarchical universe.

About This Book

Presented as nine letters, the work develops a mathematical hypothesis that interprets the Milky Way as a flattened, system-like arrangement of stars and extends that model to the sizes, motions, and distances of planets, stars, and nebulae. It assesses observational evidence and degrees of probability, offers estimates of cosmic scale, and argues that many faint nebulae are remote, galaxy-like systems. Throughout, the author connects these cosmological ideas to questions of order, final causes, and the theological and moral implications of a vast hierarchical universe.

About the Author

Wright, Thomas portrait

Thomas Wright

Thomas Wright was a 19th-century English author and antiquarian known for his diverse contributions to literature and historical studies. His works often explore cultural and social themes, particularly in relation to English history. Notable among his writings is "A History of Caricature and Grotesque in Literature and Art," which examines the evolution of caricature and its impact on artistic expression. Wright also delved into domestic life in medieval England with his book "A History of Domestic Manners and Sentiments in England During the Middle Ages." His scholarly pursuits extended to the life of explorer Sir Richard Burton and the archaeological significance of Roman sites in Britain.

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