The earth's motion of rotation including the theory of precession and nutation |
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Side 31
... day . The second is of great importance to astronomers , since it establishes the fact that the first point of Aries , or vernal equinox , to which they are accustomed to refer celestial longitudes , is not a fixed point . Stability of ...
... day . The second is of great importance to astronomers , since it establishes the fact that the first point of Aries , or vernal equinox , to which they are accustomed to refer celestial longitudes , is not a fixed point . Stability of ...
Side 35
... day or fraction of a day . hitherto failed to pn , Now the most delicate observations have detect any such inequality : hence we must altogether reject such terms , and conclude that @ 3 will always remain sensibly constant . 27 . The ...
... day or fraction of a day . hitherto failed to pn , Now the most delicate observations have detect any such inequality : hence we must altogether reject such terms , and conclude that @ 3 will always remain sensibly constant . 27 . The ...
Side 36
... day or fraction of a day , which are wholly insensible 36 THE EARTH'S MOTION OF ROTATION . tion.
... day or fraction of a day , which are wholly insensible 36 THE EARTH'S MOTION OF ROTATION . tion.
Side 37
Charles Hartwell H. Cheyne. or fraction of a day , which are wholly insensible . If , then , we write and Ø for a and y respectively , these formulæ become αψ dt 1 dv ke sine de ' de 1 dv dt kesin e dy or , since to the same order of ...
Charles Hartwell H. Cheyne. or fraction of a day , which are wholly insensible . If , then , we write and Ø for a and y respectively , these formulæ become αψ dt 1 dv ke sine de ' de 1 dv dt kesin e dy or , since to the same order of ...
Side 43
... integration . This term is independent of the disturbing force ; but having for its period 2π p which does not differ much from a day , it must be re- jected , since , as we have already remarked in PRECESSION AND NUTATION . 43.
... integration . This term is independent of the disturbing force ; but having for its period 2π p which does not differ much from a day , it must be re- jected , since , as we have already remarked in PRECESSION AND NUTATION . 43.
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The Earth's Motion of Rotation: Including the Theory of Precession and Nutation Charles Hartwell Horne Cheyne Uten tilgangsbegrensning - 1867 |
The Earth's Motion of Rotation: Including the Theory of Precession and Nutation Charles Hartwell Horne Cheyne Uten tilgangsbegrensning - 1867 |
The Earth's Motion of Rotation: Including the Theory of Precession and Nutation Charles Hartwell Horne Cheyne Uten tilgangsbegrensning - 1867 |
Vanlige uttrykk og setninger
area conserved axis in space calculating Cambridge centre of gravity Church cloth cos² Crown 8vo denote determine the motion dh dt dh dV differential coefficient disturbing force dk dt dl dh ds dh dt 2n dt dk dt dt dt dv dt dy dV dg dv ds dv dt dV dv dv dy Earth's axis ecliptic Elementary Treatise English equations of Art Extra fcap Fcap fixed plane formulæ Fourth Edition Heir of Redclyffe Hence HENRY KINGSLEY Illustrations integration invariable plane JOSEPH BAYMA longitude M. A. Second Edition maximum areas Moon's orbit motion of translation Nutation obtained order of approximation plane of maximum plane of reference Planetary Theory Poems point of Aries preceding Article Precession principal axes revised Sermons preached sin'i Sir NOEL PATON Spherical substituting Sun's Third Edition tion undisturbed motion Vignette vis viva Vols w₁ w₂ Y₁
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