## An Elementary Treatise on the Lunar Theory: With a Brief Sketch of the History of the Problem Up to the Time of Newton |

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according action angle angular applied approximation apse argument assume attraction becomes bodies calculated called Cambridge carried centre CHAPTER cloth coefficient College considered constant contains correct cos2 Crown 8vo described determined difference differential equations direction distance disturbing force earth eccentricity ecliptic Edition effect ELEMENTARY epicycle equal evection Examination Examples explain expression fixed fourth give given Hence higher HISTORY important inclination increased inequality integration introduced latitude least longitude Mathematical mean method moon moon's moon's orbit motion moving nearly neglected node Notes numerous observations obtained orbit particle period plane position present principle problem quadrature quantity radius referred retained Schools Second Edition second order solution sphere student substituted sun's suppose syzygy theory third order TREATISE true uniform University variation whole

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