Tables of the Motion of the Moon PDF Download

Author: Ernest William Brown
Publisher:
ISBN:
Category : Moon
Languages : en
Pages : 740

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Author: Ernest William Brown
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 456

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Author: Ernest William Brown
Publisher:
ISBN:
Category : Moon
Languages : en
Pages : 0

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Book Description

Author: John M. Steele
Publisher: Springer Science & Business Media
ISBN: 1461421489
Category : Mathematics
Languages : en
Pages : 169

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Book Description
The discovery of a gradual acceleration in the moon’s mean motion by Edmond Halley in the last decade of the seventeenth century led to a revival of interest in reports of astronomical observations from antiquity. These observations provided the only means to study the moon’s ‘secular acceleration’, as this newly-discovered acceleration became known. This book contains the first detailed study of the use of ancient and medieval astronomical observations in order to investigate the moon’s secular acceleration from its discovery by Halley to the establishment of the magnitude of the acceleration by Richard Dunthorne, Tobias Mayer and Jérôme Lalande in the 1740s and 1750s. Making extensive use of previously unstudied manuscripts, this work shows how different astronomers used the same small body of preserved ancient observations in different ways in their work on the secular acceleration. In addition, this work looks at the wider context of the study of the moon’s secular acceleration, including its use in debates of biblical chronology, whether the heavens were made up of æther, and the use of astronomy in determining geographical longitude. It also discusses wider issues of the perceptions and knowledge of ancient and medieval astronomy in the early-modern period. This book will be of interest to historians of astronomy, astronomers and historians of the ancient world.

Author:
Publisher: University of Pennsylvania Press
ISBN:
Category :
Languages : en
Pages : 208

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Author: José Chabás
Publisher: BRILL
ISBN: 9047429591
Category : History
Languages : en
Pages : 149

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Book Description
The Alfonsine Tables became the main computing tool for astronomers for about 250 years, from their compilation in Toledo ca. 1272 to the edition in 1551 of new tables based on Copernicus’s astronomical models. It consisted of a set of astronomical tables which, over time, was presented in many different formats. Giovanni Bianchini (d. after 1469), an astronomer active in Ferrara, Italy, was among the few scholars of that extended period to compile a coherent and insightful set based on the Alfonsine Tables. His tables, described and analyzed here for the first time, played a remarkable role in the transmission of the Alfonsine Tables and in their transition from manuscript to print. Medieval and Early Modern Science, 10

Author: Edward Greswell
Publisher: Oxford : University Press
ISBN:
Category : Calendar
Languages : en
Pages : 420

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Author: Martin C. Gutzwiller
Publisher:
ISBN:
Category : Lunar theory
Languages : en
Pages : 284

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Book Description

Author: Ernest W. (Ernest William) Brown
Publisher: Hardpress Publishing
ISBN: 9781290272490
Category :
Languages : en
Pages : 242

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Unlike some other reproductions of classic texts (1) We have not used OCR(Optical Character Recognition), as this leads to bad quality books with introduced typos. (2) In books where there are images such as portraits, maps, sketches etc We have endeavoured to keep the quality of these images, so they represent accurately the original artefact. Although occasionally there may be certain imperfections with these old texts, we feel they deserve to be made available for future generations to enjoy.

Author: Curtis Wilson
Publisher: Springer Science & Business Media
ISBN: 1441959378
Category : Mathematics
Languages : en
Pages : 323

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Book Description
This book, in three parts, describes three phases in the development of the modern theory and calculation of the Moon's motion. Part I explains the crisis in lunar theory in the 1870s that led G.W. Hill to lay a new foundation for an analytic solution, a preliminary orbit he called the "variational curve." Part II is devoted to E.W. Brown's completion of the new theory as a series of successive perturbations of Hill's variational curve. Part III describes the revolutionary developments in time-measurement and the determination of Earth-Moon and Earth-planet distances that led to the replacement of the Hill–Brown theory in 1984.