株式会社極東書店トップ商品一覧Theoria motus lunae exhibens omnes eius inaequalitates: In additamento hoc idem argumentum aliter tractatur simulque ostenditur quemadmodum motus lunae cum omnibus inaequalitatibus innumeris aliis modis repraesentari atque ad calculum revocari possit.

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Theoria motus lunae exhibens omnes eius inaequalitates: In additamento hoc idem argumentum aliter tractatur simulque ostenditur quemadmodum motus lunae cum omnibus inaequalitatibus innumeris aliis modis repraesentari atque ad calculum revocari possit.

Theoria motus lunae exhibens omnes eius inaequalitates: In additamento hoc idem argumentum aliter tractatur simulque ostenditur quemadmodum motus lunae cum omnibus inaequalitatibus innumeris aliis modis repraesentari atque ad calculum revocari possit.

・ISBN 978-1-108-06535-1 paper GB£ 43.99

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電子版あり 大学・学術機関向け電子ブック(eBook)ISBN 9781107323872
著者・編者Euler, Leonhard,
シリーズ (Cambridge Library Collection - Astronomy)
出版社 (Cambridge University Press, UK)
出版年月2014
ページ数362 pp.
言語ENG
ニュース番号<A00-5337>

解説

The problem of the moon's orbit was one that Leonhard Euler (1707-83) returned to repeatedly throughout his life. It provided a testing ground for Newton's theory of gravitation. Could the motion of the moon be entirely accounted for by Newton's theory? Or, as Euler initially suspected, did other forces need to be invoked? For practical purposes, if the moon's orbit could be accurately predicted, its motion would provide the universal timekeeper required to solve the longitude problem. In addition to the mathematical 'three-body problem', a topic still under investigation today, Euler was faced with the statistical problem of reconciling observations rendered inconsistent by experimental error. The present work, published in Latin in 1753, is Euler's triumphant solution. It may not be the last word on a subject which has occupied mathematicians and astronomers for over three centuries, but it showed that Newton's laws were sufficient to explain lunar motion.