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" ... the solar parallax.* The transits of Venus will afford a far more accurate determination of this parallax than those of Mercury; for, on account of its greater proximity to the earth, the difference in the duration of the transit at different places... "
A Manual of Spherical and Practical Astronomy: Spherical astronomy - Page 585
by William Chauvenet - 1863
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A Manual of Spherical and Astronomy: Embracing the ..., Part 32, Volume 1

William Chauvenet - Astronomical instruments - 1864 - 726 pages
...in the duration of the transit at different places will be much greater, and the coefficient of AT in the final equations proportionally great. Although...their squares and higher powers may be neglected. LAORANGE'S method for this purpose is the most simple, and, in the improved form which I shall give...
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A Manual of Spherical and Pratical Astronomy: Embracing the ..., Volume 1

William Chauvenet - 1864 - 720 pages
...in the duration of the transit at different places will be much greater, and the coefficient of AT: in the final equations proportionally great. Although...their squares and higher powers may be neglected. LAGRANQE'S method for this purpose is the most simple, and, in the improved form which I shall give...
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A treatise on the dynamics of a particle, by P.G. Tait and W.J. Steele

Peter Guthrie Tait - 1865 - 394 pages
...<j>'. A still greater simplification will be obtained by taking in addition the condition that 0 and ff are so small, that their squares and higher powers may be neglected. With these our equations become m = -T0+ T'ff, m . = mg, e?V md?=~ m Itf = ' And x = x' = 2 = 0, Hence,...
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A Treatise on the Dynamics of a Particle: With Numerous Examples

Peter Guthrie Tait, William John Steele - Dynamics of a particle - 1871 - 462 pages
...<£'. A still greater simplification will be obtained by taking in addition the condition that 6 and ff are so small, that their squares and higher powers may be neglected. With these our equations become m — rr> ,ds -rr dt' And, to a sufficient approximation, x= ad, Hence,...
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A Treatise on the Adjustment of Observations: With Applications to Geodetic ...

Thomas Wallace Wright - Geodesy - 1884 - 450 pages
...to X, Y, . . . and then substituting X' ', Y', . . . for X, Y, . . . If the corrections x, y, . . . are so small that their squares and higher powers may be neglected and they are written dX, dY', . . . and Ff(X', Y', . . .) is written dF, then "-£.*'+ &•"+•.....
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General Physics for Students: A Text-book on the Fundamental Properties of ...

Edwin Edser - Physics - 1913 - 656 pages
...= 3*, and .r = 8/3. In the following investigations it will be assumed that all strains dealt with are so small that their squares and higher powers may be neglected in comparison with the strains themselves. Compressive stress. — A cube of matter can be compressed...
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