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 1
... calculated on the assumption of its truth , agree more and more closely with the observed motions as our calcu ... calculation and observation to instrumental errors , to an incomplete analysis , or to our ignorance of the existence of ...
... calculated on the assumption of its truth , agree more and more closely with the observed motions as our calcu ... calculation and observation to instrumental errors , to an incomplete analysis , or to our ignorance of the existence of ...
Σελίδα 2
... calculation ; and therefore , either the law of universal gravitation was here at fault , or some unknown body was disturbing the path of the planet . This last supposition , in the powerful hands of Messrs . Adams and Le Verrier , led ...
... calculation ; and therefore , either the law of universal gravitation was here at fault , or some unknown body was disturbing the path of the planet . This last supposition , in the powerful hands of Messrs . Adams and Le Verrier , led ...
Σελίδα 13
... calculation , ob- tained on supposition of the sun and earth being the only bodies in the universe , this plane , in which , according to the last section , an elliptic orbit would be described , is a fixed plane : but this is no longer ...
... calculation , ob- tained on supposition of the sun and earth being the only bodies in the universe , this plane , in which , according to the last section , an elliptic orbit would be described , is a fixed plane : but this is no longer ...
Σελίδα 23
... calculated from their hori- zontal parallaxes , found by observations made at remote geographical stations . + That the moon's orbit during one revolution is very nearly a plane inclined as we have stated , will be found by noting her ...
... calculated from their hori- zontal parallaxes , found by observations made at remote geographical stations . + That the moon's orbit during one revolution is very nearly a plane inclined as we have stated , will be found by noting her ...
Σελίδα 23
... , and S ' , G ' , M ' , the projections of S , G , M , then , sin ( sun's lat . ) = sin SES ' = = SS ' = GG ' EG.sin ( moon's lat . ) ES ES ES M A EM = E + M ES sin ( moon's lat . ) B n 7 " , To calculate the values of 16 LUNAR THEORY .
... , and S ' , G ' , M ' , the projections of S , G , M , then , sin ( sun's lat . ) = sin SES ' = = SS ' = GG ' EG.sin ( moon's lat . ) ES ES ES M A EM = E + M ES sin ( moon's lat . ) B n 7 " , To calculate the values of 16 LUNAR THEORY .
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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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