| 000 | 02425nam a22003498i 4500 | ||
|---|---|---|---|
| 001 | CR9781107323872 | ||
| 003 | UkCbUP | ||
| 005 | 20200124160200.0 | ||
| 006 | m|||||o||d|||||||| | ||
| 007 | cr|||||||||||| | ||
| 008 | 130122s1753||||enk o ||1 0|eng|d | ||
| 020 | _a9781107323872 (ebook) | ||
| 020 | _z9781108065351 (paperback) | ||
| 040 |
_aUkCbUP _beng _erda _cUkCbUP |
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| 050 | 4 |
_aQB391 _b.E85 1753 |
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| 082 | 0 | 4 |
_a521 _223 |
| 100 | 1 |
_aEuler, Leonhard, _d1707-1783, _eauthor. |
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| 245 | 1 | 0 |
_aTheoria motus lunae exhibens omnes eius inaequalitates : _bIn additamento hoc idem argumentum aliter tractatur simulque ostenditur quemadmodum motus lunae cum omnibus inaequalitatibus innumeris aliis modis repraesentari atque ad calculum revocari possit / _cLeonhard Euler. |
| 264 | 1 |
_aPlace of publication not identified : _bpublisher not identified, _c1753. |
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| 264 | 1 |
_aCambridge : _bCambridge University Press |
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| 300 |
_a1 online resource (viii, 347 pages) : _bdigital, PDF file(s). |
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| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
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| 338 |
_aonline resource _bcr _2rdacarrier |
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| 490 | 1 | _aCambridge library collection. Astronomy | |
| 520 | _aThe 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. | ||
| 650 | 0 |
_aLunar theory _vEarly works to 1800. |
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| 650 | 0 |
_aCelestial mechanics _vEarly works to 1800. |
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| 776 | 0 | 8 |
_iPrint version: _z9781108065351 |
| 830 | 0 |
_aCambridge library collection. _pAstronomy. |
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| 856 | 4 | 0 | _uhttps://doi.org/10.1017/CBO9781107323872 |
| 999 |
_c514758 _d514756 |
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