An Elementary Treatise on the Lunar Theory: With a Brief Sketch of the History of the Problem Up to the Time of NewtonMacmillan, 1859 - 119 σελίδες |
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Σελίδα 2
... neglected , except in extreme It had been seen by Dr. Lamont at Munich , one year before its being known to be a planet . " Solar System , by J. R. Hind . " Since the sun attracts both the earth and moon , it is clear that its effects ...
... neglected , except in extreme It had been seen by Dr. Lamont at Munich , one year before its being known to be a planet . " Solar System , by J. R. Hind . " Since the sun attracts both the earth and moon , it is clear that its effects ...
Σελίδα 3
... neglected compared with the original path AP . There- fore PQ is parallel and equal to PP Hence the projection of the whole disturbance PQ on any straight line , being equal to the algebraical sum of the pro- 1 jections of PP , and P ...
... neglected compared with the original path AP . There- fore PQ is parallel and equal to PP Hence the projection of the whole disturbance PQ on any straight line , being equal to the algebraical sum of the pro- 1 jections of PP , and P ...
Σελίδα 8
... neglected , being of an order higher than that to which we intend to carry the present investi- gation : the error however , though very small , is appre- ciable , and if a nearer approximation were required , it would be necessary to ...
... neglected , being of an order higher than that to which we intend to carry the present investi- gation : the error however , though very small , is appre- ciable , and if a nearer approximation were required , it would be necessary to ...
Σελίδα 14
... neglected . * S- M E G W Let S , E , M be the centres of the sun , earth , and moon , G the centre of gravity of the last two . Now the motion of G is the same as if the whole mass E + M were collected there and acted on by forces equal ...
... neglected . * S- M E G W Let S , E , M be the centres of the sun , earth , and moon , G the centre of gravity of the last two . Now the motion of G is the same as if the whole mass E + M were collected there and acted on by forces equal ...
Σελίδα 15
... neglect these forces in this approximate determination of the path of G , the error being of a still higher order than that introduced EM \ 2 by the neglect of ( TG ) . SG Again , the accelerating force in GS = = m'SG PLANE OF REFERENCE ...
... neglect these forces in this approximate determination of the path of G , the error being of a still higher order than that introduced EM \ 2 by the neglect of ( TG ) . SG Again , the accelerating force in GS = = m'SG PLANE OF REFERENCE ...
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Συχνά εμφανιζόμενοι όροι και φράσεις
accelerating forces Algebra angle angular velocity annual equation apogee approximation apse line argument astronomers attraction Author has endeavoured body calculated CAMBRIDGE CLASS BOOKS centre chapter cloth coefficient Collection of Examples connexion considered correction cos2 Crown 8vo determine differential equations distance disturbing force E-Ma E+Ma earth eccentricity ecliptic elliptic inequality epicycle equal evection expression fixed plane h2u³ higher order Hipparchus inclination ISAAC TODHUNTER John's College late Fellow Latin latitude Lunar M.A. Fellow mean motion mean place mean value method moon moon's mean longitude moon's motion moon's orbit nearly node numerous Examples observations obtained octants order of approximation particle perigee periodical terms position Ps-S Ptolemy quadrature quantity radius vector revolution Schools Second Edition second order shew sidereal month solution sphere student syzygy Theory third order tions true anomaly true longitude Tycho Brahé V₁ variation že²
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