Popular Astronomy, Volume 56Goodsell Observatory of Carleton College, 1948 |
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Page 69
hence e29c / 8 and e , = 7e / 8 , i.e. , for 2e - 0.1856 , e2 = 0.1044 , e1 = 0.0812 , somewhat less different than Kepler's values . For e1 = e2 the second term disappears , and in the octants , at E = 45 ° , the error is 14e2 ...
hence e29c / 8 and e , = 7e / 8 , i.e. , for 2e - 0.1856 , e2 = 0.1044 , e1 = 0.0812 , somewhat less different than Kepler's values . For e1 = e2 the second term disappears , and in the octants , at E = 45 ° , the error is 14e2 ...
Page 182
... hence proportional to the force in B. In the simple case of circular motions the versed sines are equal to the squares of the arcs divided by the diameter , hence the forces will be as the squares of the arcs described in the same time ...
... hence proportional to the force in B. In the simple case of circular motions the versed sines are equal to the squares of the arcs divided by the diameter , hence the forces will be as the squares of the arcs described in the same time ...
Page 310
... Hence , since there were 7 planets at the time , it is a linear function of the other component of itself and of all the other six planets . This holds for every planet , so that we have a system of equations such as dh / dt = a11 + ...
... Hence , since there were 7 planets at the time , it is a linear function of the other component of itself and of all the other six planets . This holds for every planet , so that we have a system of equations such as dh / dt = a11 + ...
Contents
FEBRUARY 1948 | 144 |
The Planets in March 1948 Raymond H Wilson Jr 36 97 | 176 |
THE PLANETARY THEORY OF NEWTON A PANNEKOEK | 177 |
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