An Elementary Treatise on the Lunar Theory: With a Brief Sketch of the History of the Problem Up to the Time of NewtonMacmillan, 1853 - 103 sider |
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Side 12
... period and to a degree of approximation far beyond that to which we shall carry our investigations , be considered as fixed and coinciding with its position at present . 15. The centre of gravity of the earth and moon describes ...
... period and to a degree of approximation far beyond that to which we shall carry our investigations , be considered as fixed and coinciding with its position at present . 15. The centre of gravity of the earth and moon describes ...
Side 31
... period of the inequality ' denoted by it would be of great length ; then , whatever might be the value ' of the coefficient a , the inequality would still be always confined within ' certain limits , and after many ages would return to ...
... period of the inequality ' denoted by it would be of great length ; then , whatever might be the value ' of the coefficient a , the inequality would still be always confined within ' certain limits , and after many ages would return to ...
Side 40
... period is nearly the same as that of the moon , produces im- portant effects in the radius vector ; and a force whose period is very long will be important in its effect on the longitude . See Airy's Tracts , Planetary Theory , p . 78 ...
... period is nearly the same as that of the moon , produces im- portant effects in the radius vector ; and a force whose period is very long will be important in its effect on the longitude . See Airy's Tracts , Planetary Theory , p . 78 ...
Side 52
... period , may be considered as cancelling themselves in adding up the terms of each set . Let there be r terms in the first set and s terms in the second , and let V ' , V " , Vr be the values of V corre- sponding to positive values of ...
... period , may be considered as cancelling themselves in adding up the terms of each set . Let there be r terms in the first set and s terms in the second , and let V ' , V " , Vr be the values of V corre- sponding to positive values of ...
Side 56
... period of a revolution 2π being which is , therefore , the expression for a mean sidereal Ρ month , or about 271 days . * The value of p is , according to Art . ( 50 ) , given by 1 Ρ = 1 ha ( 1 + §k2 + m2 + že2 ) , and as m is due to ...
... period of a revolution 2π being which is , therefore , the expression for a mean sidereal Ρ month , or about 271 days . * The value of p is , according to Art . ( 50 ) , given by 1 Ρ = 1 ha ( 1 + §k2 + m2 + že2 ) , and as m is due to ...
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An Elementary Treatise on the Lunar Theory: With a Brief Sketch of the ... Hugh Godfray Uten tilgangsbegrensning - 1859 |
An Elementary Treatise on the Lunar Theory: With a Brief Sketch of the ... Hugh Godfray Uten tilgangsbegrensning - 1859 |
An Elementary Treatise on the Lunar Theory: With a Brief Sketch of the ... Hugh Godfray Uten tilgangsbegrensning - 1859 |
Vanlige uttrykk og setninger
2e sin cpt 3m²e angle angular velocity annual equation anomaly apogee apse line astronomers attraction bodies calculated Cambridge central disturbing force centre cloth coefficient College considered correction cos(c Crown 8vo determine differential equation distance E-Ma E+Ma earth eccentric ecliptic Edition effect elliptic inequality epicycle equal Euclid's Elements evection expression fourth order Geometrical Hence higher order Hipparchus hypothesis inclination introduced latitude Lunar Theory m³e mean angular mean longitude mean motion mean value moon moon moves moon's longitude moon's mean moon's motion moon's orbit nearly neglected Newton node numerous observation obtained order of approximation parallax perigee periodical terms position Ptolemy quadrature quantity radius vector revolution second order shew sidereal month sin(g solution Substituting suppose supposition syzygy third order true anomaly true longitude Tycho V₁ variation že² ᏧᎾ
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