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 vi
... latitude , they , by analogy to Newton's method , employed the differential variations of the motion of the node and of the inclination of the orbit . Laplace , Damoiseau , Plana , and also Herschel and Airy in their more elementary ...
... latitude , they , by analogy to Newton's method , employed the differential variations of the motion of the node and of the inclination of the orbit . Laplace , Damoiseau , Plana , and also Herschel and Airy in their more elementary ...
Σελίδα vii
... latitude . The selection of the method followed in the present work , which is the same as that of Airy , Herschel , & c . , was made on account of its simplicity : moreover , it is the method which has obtained in this university , and ...
... latitude . The selection of the method followed in the present work , which is the same as that of Airy , Herschel , & c . , was made on account of its simplicity : moreover , it is the method which has obtained in this university , and ...
Σελίδα x
... Latitude 77 Discussion of the 83 Discussion of the terms in the Moon's Radius Vector 89 Periodic time of the Moon 61 71 76 • 78 CHAPTER VII . APPENDIX . 91 The Moon is retained in her orbit by gravity 92 The Moon's orbit is everywhere ...
... Latitude 77 Discussion of the 83 Discussion of the terms in the Moon's Radius Vector 89 Periodic time of the Moon 61 71 76 • 78 CHAPTER VII . APPENDIX . 91 The Moon is retained in her orbit by gravity 92 The Moon's orbit is everywhere ...
Σελίδα 16
... latitude always of the same name as that of the moon , and deducible from it , when Τ M M E ES , EM , and the ratio of the masses of the earth and moon are known . For if S'EM ' be this fixed plane through E , and S ' , G ' , M ' , the ...
... latitude always of the same name as that of the moon , and deducible from it , when Τ M M E ES , EM , and the ratio of the masses of the earth and moon are known . For if S'EM ' be this fixed plane through E , and S ' , G ' , M ' , the ...
Σελίδα 17
... latitude never exceeds 5 ° 9 ′ , the sun's latitude will always be less than 1 " . Again , with respect to the sun's longitude : let Er be the direction of the first point of Aries , —that is , a fixed line in our plane of reference ...
... latitude never exceeds 5 ° 9 ′ , the sun's latitude will always be less than 1 " . Again , with respect to the sun's longitude : let Er be the direction of the first point of Aries , —that is , a fixed line in our plane of reference ...
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3m²e accelerating forces Algebra angle angular velocity annual equation anomaly apogee apse line astronomers attraction bodies BROOKE FOSS WESTCOTT calculated Cambridge centre cloth coefficient considered correct cos2 Crown 8vo determined differential equations distance disturbing force E-Ma E+Ma earth eccentricity ecliptic ELEMENTARY TREATISE elliptic inequality epicycle equal evection expression Fcap fixed plane fourth order h²u³ higher order Hipparchus hu³ integration John's College Lunar Theory MACMILLAN AND CO'S Mathematical mean anomaly mean longitude mean motion mean value method moon moon's mean moon's motion moon's orbit nearly neglected Newton node numerous observations obtained order of approximation parallax particle perigee periodical terms position Ps-S Ptolemy quadrature quantity radius vector revolution Schools Second Edition second order shew sidereal month sin2 solution sphere student substituted syzygy third order true anomaly true longitude Tycho variation že²
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