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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accelerating forces according action angle anomaly applied approximation apse argument assume attraction become 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 examine Examples expression fixed fourth give given Hence HISTORY important inclination increased inequality integration introduced knowledge latitude least longitude mass mean method moon moon's moon's orbit motion moving nearly neglected node Notes numerous observations obtained orbit parallel period plane position present principle problem quadrature quantity radius vector referred rest retained Schools Second Edition second order solution student substituted sun's suppose syzygy taken theory third order TREATISE true University variation whole
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