Instructions Given in the Drawing School Established by the Dublin Society: Course of mathematicks. System of the physical world. System of the moral world. Plan of the military art. Plan of the marcantile arts. Plan of naval art. Plan of mechanic arts. The elements of EuclidA. M'Culloch, 1769 |
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Resultat 1-5 av 100
Side lxiii
... wherefore by the Compofition of Ratios g X Y X T is to YX GX or the Gravity ( g ) of the Earth , at the Pole , is to the Gravity ( G ) at the Equator as 126 X 126 X 100 to 125 × 125 × 101 that is as 501 to 500 . But he had demonstrated ...
... wherefore by the Compofition of Ratios g X Y X T is to YX GX or the Gravity ( g ) of the Earth , at the Pole , is to the Gravity ( G ) at the Equator as 126 X 126 X 100 to 125 × 125 × 101 that is as 501 to 500 . But he had demonstrated ...
Side lxvii
... wherefore the Height ( b ) at the Poles will be 19573064 and the Height ( b + c ) at the Equator 19658536 Feet . X. the different regions of After determining the Relation of the Axes of the Earth fuppofed Ho- What are mogeneous ...
... wherefore the Height ( b ) at the Poles will be 19573064 and the Height ( b + c ) at the Equator 19658536 Feet . X. the different regions of After determining the Relation of the Axes of the Earth fuppofed Ho- What are mogeneous ...
Side lxviii
... Wherefore by the Compofition of Ratios exE is to EXD , or the Excefs [ e ] of a Degree in the Latitude of Paris is to the Length of the Degree [ D ] at the Equator , as 895448337 is to 12008989000 ; ând the Length [ e + D ] of a Degree ...
... Wherefore by the Compofition of Ratios exE is to EXD , or the Excefs [ e ] of a Degree in the Latitude of Paris is to the Length of the Degree [ D ] at the Equator , as 895448337 is to 12008989000 ; ând the Length [ e + D ] of a Degree ...
Side lxxiv
... ) The ratio of the motion of the ring to the motion of the interior globe affigned by Newton , is 4590 to 485223. which is erroneous as shall be shewn hereafter . heres , ( b ) wherefore the annual Motion ( LXXIV . , SYSTEM OF THE.
... ) The ratio of the motion of the ring to the motion of the interior globe affigned by Newton , is 4590 to 485223. which is erroneous as shall be shewn hereafter . heres , ( b ) wherefore the annual Motion ( LXXIV . , SYSTEM OF THE.
Side lxxv
Joseph Fenn. heres , ( b ) wherefore the annual Motion ( P. ) of the equinoctial Points of the Body compofed of the Ring and Globe to which it adheres , will be to the an- aual Motion of the Nodes ( N ) of the Moon , in the compounded ...
Joseph Fenn. heres , ( b ) wherefore the annual Motion ( P. ) of the equinoctial Points of the Body compofed of the Ring and Globe to which it adheres , will be to the an- aual Motion of the Nodes ( N ) of the Moon , in the compounded ...
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Instructions Given in the Drawing School Established by the Dublin Society ... Joseph Fenn Uten tilgangsbegrensning - 1769 |
Vanlige uttrykk og setninger
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Populære avsnitt
Side 4 - A circle is a plane figure contained by one line, which is called the circumference, and is such that all straight lines drawn from a certain point within the figure to the circumference, are equal to one another.
Side 164 - When of the equimultiples of four magnitudes (taken as in the fifth definition), the multiple of the first is greater than that of the second, but the multiple of the third is not greater than the multiple of the fourth; then the first is said to have to the second a greater ratio than the third magnitude has to the fourth : and, on the contrary, the third is said to have to the fourth a less ratio than the first has to the second. VIII. 'Analogy, or proportion, is the similitude of ratios.
Side 165 - When four magnitudes are continual proportionals, the first is said to have to the fourth the triplicate ratio of that which it has to the second, and so on, quadruplicate, &c., increasing the denomination still by unity, in any number of proportionals.
Side 8 - Let it be granted that a straight line may be drawn from any one point to any other point.
Side xxviii - This depends upon three suppositions: — first, that all celestial bodies whatsoever have an attraction or gravitating power towards their own centres, whereby they attract not only their own parts and keep them from flying from them, as we may observe the earth to do, but that they do also attract all the other celestial bodies that are within the sphere of their activity...
Side 164 - VII. When of the equimultiples of four magnitudes (taken as in the fifth definition), the multiple of the first is greater than that of the second, but the multiple of the third is not greater than the multiple of the fourth ; then the first is said to have to the second a greater ratio than the third magnitude has to the fourth : and, on the contrary, the third is...
Side 29 - Therefore if two straight lines, &c. QED COR. 1. From this it is manifest, that, if two straight lines cut one another, the angles they make at the point where they cut, are together equal to four right angles.
Side 29 - Cor. 2. And consequently that all the angles made by any number of lines meeting in one point, are together equal to four right angles.
Side xxviii - Saturn also, by their attractive powers, have a considerable influence upon its motion, as in the same manner the corresponding attractive power of the earth hath a considerable influence upon every one of their motions also.
Side xxviii - The third supposition is that these attractive powers are so much the more powerful in operating, by how much the nearer the body wrought upon is to their own centers. Now what these several degrees are I have not yet experimentally verified...