Mathematical Treatise: Containing I. The Theory of Analytical Functions, II. Spherical Trigonometry, with Practical and Nautical AstronomyOliver & Boyd, 1838 - 574 páginas |
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Mathematical Treatise: Containing I, the Theory of Analytical Functions, II ... John West Sin vista previa disponible - 2015 |
Términos y frases comunes
2a+cos 4a+cos absciss affirmative altitude ANALYTICAL FUNCTIONS angle apparent latitude axis becomes centre circle circumference co-efficients Consequently cosec cosine curve cx² deduced denote derivative functions diameter difference distance dx³ earth eccentric anomaly ecliptic equal equation EXAMPLE expressed f(x+i former fraction given greater Hence horizontal parallax hypotenuse latitude logarithms longitude manner moon moon's multiplied negative parallax perpendicular pole polynomial derivatives preceding prime function primitive PROBLEM putting quadrant radius right ascension right-angled triangle semidiameters side sin BC sine sine and cosine spherical triangle substituting subtangent sun's supposing suvers tangent theorems tion true anomaly vanish variable versed sine Whence whole number zenith α α φα
Pasajes populares
Página 52 - A spherical angle is measured by the arc of a great circle described from its vertex as a pole, and included between its sides, produced if necessary.
Página 124 - Greenwich for this station ; foreigners, the principal observatories of their respective nations. Some geographers have adopted the island of Ferro. Hereafter, when we speak of longitude, we reckon from Greenwich. The longitude of a place is, therefore, measured by the arc of the equator intercepted between the meridian of the place and that of Greenwich ; or, which is the same thing, by the spherical angle at the pole included between these meridians.
Página 49 - a circle of a sphere is the diameter of the sphere which is perpendicular to the plane of the circle. The ends of the axis are called the poles of the circle.
Página 37 - To divide a given number (a) into two such parts, that the product of the mth power of the one into the wth power of the other shall be a maximum. We have x'" (a — *•)" a maximum, and therefore mtf" -1 (a — #)" — nxm (a — #)"-' = o ; whence^ m (a — x) = nx.
Página 123 - Azimuth, or vertical circles are great circles passing through the zenith and nadir. They cut the horizon at right ' angles. The altitudes of the heavenly bodies are measured on these circles.
Página 55 - C= 540° — (a' + b' + c'). But a' + b' + c' < 360° (86) ; therefore, A + B + C > 180°; that is, the sum of the three angles is greater than two right angles.
Página 180 - ... soberness of description and precision of language which characterize the science of the nations of Europe. It appears from the astronomical tables that the ancient Hindoos knew that the intersection of the equator and ecliptic is not always in the same point, but that it is constantly retrograding on the ecliptic in a direction contrary to the order of the signs...
Página 125 - Ursa Minoris. This varying direction of the earth's axis is occasioned by the varying influence of the sun and moon on the protuberant matter of the earth's equator, in necessary correspondence with the earth's variations of distance in different parts of its orbit ; and in respect of which varying influence the earth may be described, if I may use a homely figure, as in the situation of a man held by the collar between two policemen, and swayed to the...
Página 194 - ... sun. In eclipses of the moon, the shadow is found to be a little greater than this rule gives it, owing to the atmosphere of the earth. This augmentation of the semidiameter is, according to M. Cassini, 20"; according to M.