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 viii
... calculated by Hipparchus 100 126 Tycho Brahe's discovery of the change of inclination and of the want of uniformity in the motion of the Node 101 127 His construction to represent these changes 102 LUNAR THEORY . CHAPTER I. INTRODUCTION ...
... calculated by Hipparchus 100 126 Tycho Brahe's discovery of the change of inclination and of the want of uniformity in the motion of the Node 101 127 His construction to represent these changes 102 LUNAR THEORY . CHAPTER I. INTRODUCTION ...
Side 1
... calculated on the assumption of its truth , agree more and more closely with the observed motions as our calculations are more strictly performed , we have every reason to consider the law as an established truth , and to attribute any ...
... calculated on the assumption of its truth , agree more and more closely with the observed motions as our calculations are more strictly performed , we have every reason to consider the law as an established truth , and to attribute any ...
Side 2
... calculated places of the planet Uranus . These perturbations were too great to be attributed wholly to errors of instruments or of calculation ; and therefore , either the law of universal gravi- tation was here at fault , or some ...
... calculated places of the planet Uranus . These perturbations were too great to be attributed wholly to errors of instruments or of calculation ; and therefore , either the law of universal gravi- tation was here at fault , or some ...
Side 11
... calculation , obtained 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 , obtained 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 ...
Side 19
... of the luminaries may be calculated from their horizontal parallaxes , found by observations made at remote geographical stations . ( 4 ) During one revolution , the moon moves C 2 Formation of the Differential Equations.
... of the luminaries may be calculated from their horizontal parallaxes , found by observations made at remote geographical stations . ( 4 ) During one revolution , the moon moves C 2 Formation of the Differential Equations.
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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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