Mathematical Tracts on the Lunar and Planetary Theories, the Figure of the Earth, Precession and Nutation, the Calculus of Variations, and the Undulatory Theory of Optics: Designed for the Use of Students in the UniversityMacmillan and Company, 1858 - 400 sider |
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Side
... Nearly Ready . MR . DREW'S ( of Blackheath School ) GEOMETRICAL CONIC SECTIONS . 48. 6d . MR . GODFRAY'S TREATISE ON THE LUNAR THEORY . MR . GRANT'S PLANE ASTRONOMY . MR . HEMMING'S DIFFERENTIAL CALCULUS . SECOND EDITION . 58. 6d . 68 ...
... Nearly Ready . MR . DREW'S ( of Blackheath School ) GEOMETRICAL CONIC SECTIONS . 48. 6d . MR . GODFRAY'S TREATISE ON THE LUNAR THEORY . MR . GRANT'S PLANE ASTRONOMY . MR . HEMMING'S DIFFERENTIAL CALCULUS . SECOND EDITION . 58. 6d . 68 ...
Side 12
... nearly , an ellipse in one plane , and the area passed over by its radius vector is very nearly pro- portional to the time . Let E and M , ( fig . 1 ) be the Earth and Moon , m ' the Sun ; G the center of gravity of the Earth and Moon ...
... nearly , an ellipse in one plane , and the area passed over by its radius vector is very nearly pro- portional to the time . Let E and M , ( fig . 1 ) be the Earth and Moon , m ' the Sun ; G the center of gravity of the Earth and Moon ...
Side 14
... nearly , and 400 1 M E + M = 30 ) is quite in- 80 sensible . In the same manner we find the accelerating force perpendicular to Gm ' or m ' 3 EM2 + ME2 g2 12 • 2 m ' 12 • 3 • · ( E + M ) ME 3 2.2 · 72 sin 2w , „ 12 · 2 · ( M + E ' ) 2 ...
... nearly , and 400 1 M E + M = 30 ) is quite in- 80 sensible . In the same manner we find the accelerating force perpendicular to Gm ' or m ' 3 EM2 + ME2 g2 12 • 2 m ' 12 • 3 • · ( E + M ) ME 3 2.2 · 72 sin 2w , „ 12 · 2 · ( M + E ' ) 2 ...
Side 15
... nearly circular , this angle varies as sin a very nearly . And if the Moon be above the plane of the ecliptic , the Earth will be below it , and the Sun will appear to have a latitude , which can be calculated from the latitude of the ...
... nearly circular , this angle varies as sin a very nearly . And if the Moon be above the plane of the ecliptic , the Earth will be below it , and the Sun will appear to have a latitude , which can be calculated from the latitude of the ...
Side 26
... nearly the true one ; substitute this value for u , in the terms of small magnitude ; II will then be a function of 0 only , and the equation may be solved , and a more approximate value of u found . Substitute this for u in II , and ...
... nearly the true one ; substitute this value for u , in the terms of small magnitude ; II will then be a function of 0 only , and the equation may be solved , and a more approximate value of u found . Substitute this for u in II , and ...
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Mathematical Tracts on the Lunar and Planetary Theories, the Figure of the ... George Biddell Airy Uten tilgangsbegrensning - 1858 |
Mathematical Tracts on the Lunar and Planetary Theories, the Figure of the ... George Biddell Airy Uten tilgangsbegrensning - 1858 |
Mathematical Tracts on the Lunar and Planetary Theories: The Figure of the ... George Biddell Airy, Sir Ingen forhåndsvisning tilgjengelig - 2016 |
Vanlige uttrykk og setninger
2π λ analyzing plate angle angular velocity attraction axes axis bright Cambridge cloth co-ordinates coefficient College Consequently constant cos² Crown 8vo crystal curve depending different colours differential direction displacement distance disturbing force dR dR dt dt Earth elliptically polarized ellipticity equal equation expression extraordinary ray Fcap front ƒ² glass Hence inclined integration intensity investigation length longitude mean anomaly Moon motion multiplied nearly node nutation ordinary ray parallel particles perigee perihelion perpendicular plane of incidence plane of polarization plane of reflection precession produced PROP proportion quantity radius vector refraction rhombohedron rings shew sin² spheroid Sun's suppose surface tion tourmaline Trinity College undulation vibration vt-x wave