Transactions of the Cambridge Philosophical Society, المجلد 22University Press, 1923 |
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الصفحة 62
... orbital motion is direct or retrograde , and its quasi - statical tidal influence will have a period near the half - day . Accordingly ellipsoids of a shape deviating to some moderate extent from that at the Maclaurin- Jacobi junction ...
... orbital motion is direct or retrograde , and its quasi - statical tidal influence will have a period near the half - day . Accordingly ellipsoids of a shape deviating to some moderate extent from that at the Maclaurin- Jacobi junction ...
الصفحة 66
... orbital revolution have the same period . The connexion with the above seems sufficient to justify the inclusion of this case in the diagrams . The case represented is that in which the liquid mass is extremely small in relation to the ...
... orbital revolution have the same period . The connexion with the above seems sufficient to justify the inclusion of this case in the diagrams . The case represented is that in which the liquid mass is extremely small in relation to the ...
الصفحة 72
... orbital revolution ; the historical order suggested is a passage from the direction of P towards the Jacobian junction , and thence to the spheroidal form . § 7. We proceed to methods of approximation which it is advisable to use near ...
... orbital revolution ; the historical order suggested is a passage from the direction of P towards the Jacobian junction , and thence to the spheroidal form . § 7. We proceed to methods of approximation which it is advisable to use near ...
الصفحة 85
... orbital period equal to that of rotation of the liquid ellipsoid , is represented by the equations a2 ( A - w2 - 2vw2 ) = b2 ( B- w2 + vw2 ) = c2 ( C + vw2 ) , = where v = · M / ( M + m ) may range from 0 to 1. For v = 0 the distant ...
... orbital period equal to that of rotation of the liquid ellipsoid , is represented by the equations a2 ( A - w2 - 2vw2 ) = b2 ( B- w2 + vw2 ) = c2 ( C + vw2 ) , = where v = · M / ( M + m ) may range from 0 to 1. For v = 0 the distant ...
الصفحة 199
... orbit . Differentiating the last equation rú , i X = - - written e , e ( 31Σlå ) / r3 — — mü , and rü / V3 is of ... orbit sufficiently great . In VOL . XXII . No. XI . 26 a conical orbit it is generally true that 2 and THE KINETIC ...
... orbit . Differentiating the last equation rú , i X = - - written e , e ( 31Σlå ) / r3 — — mü , and rü / V3 is of ... orbit sufficiently great . In VOL . XXII . No. XI . 26 a conical orbit it is generally true that 2 and THE KINETIC ...
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a₁ angle approximately asymptotic expansion atmosphere Axiom of Archimedes axis b₁ c₁ calculated coefficients considered constant convergent convex set cordon corresponding cos² curve d₁ definition denote density determined differential equations disturbance diurnal diurnal variations dyadic earth equal escape expression factor finite follows formula free path function G. H. Hardy giant star given h₂ Hence integral equation invariant Jacobian k₁ k₂ magnitude molecules obtained orbit paper parameters partitions plane positive potential Primitive Roots ratio relation respectively result rotation scalar shew shewn sin² solar solid angle solutions substitution suppose surface t₁ theorem theory v₁ values vector velocity w₁ X₁ XXII zero Σ Σ дх