Spherical Astronomy Electronic Resource
Spherical Astronomy Electronic Resource
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In our eReader you can find the full English version of the book. Read Spherical Astronomy Electronic Resource Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book Spherical Astronomy Electronic Resource
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6377843.
If we compute again the numerical values of the coef- ficients and take a = 1, we find: log $ == 9 . 9992747 -H 0. 0007271 cos 2 y 0. 0000018 cos 4 y (F) and from this we get for instance for the latitude of Berlin : log ^ = 9. 9990880.
144 If we know therefore the latitude of a place, we can compute from the two series (C) and (F) the geocentric la- titude and the distance of the place from the centre of the earth and these two quantities in connection with the sidereal time define th...e position of the place with respect to the centre of the earth at any moment. If we now imagine a system of rectangular axes passing through the centre of the earth, the axis of z being vertical to the plane of the equator, whilst the axes of x and y are situated in the plane of the equator so that the positive axis of x is directed towards the point of the vernal equinox, the positive axis of y to the point whose right ascension is 90, we can express the position of the place with respect to the centre by the following three co-ordinates : X = () COS' COS y = $ cos y> sin (6r).
What to read after Spherical Astronomy Electronic Resource?
You can find similar books in the "Read Also" column, or choose other free books by F Franz Brnnow to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
6377843.
If we compute again the numerical values of the coef- ficients and take a = 1, we find: log $ == 9 . 9992747 -H 0. 0007271 cos 2 y 0. 0000018 cos 4 y (F) and from this we get for instance for the latitude of Berlin : log ^ = 9. 9990880.
144 If we know therefore the latitude of a place, we can compute from the two series (C) and (F) the geocentric la- titude and the distance of the place from the centre of the earth and these two quantities in connection with the sidereal time define th...e position of the place with respect to the centre of the earth at any moment. If we now imagine a system of rectangular axes passing through the centre of the earth, the axis of z being vertical to the plane of the equator, whilst the axes of x and y are situated in the plane of the equator so that the positive axis of x is directed towards the point of the vernal equinox, the positive axis of y to the point whose right ascension is 90, we can express the position of the place with respect to the centre by the following three co-ordinates : X = () COS
What to read after Spherical Astronomy Electronic Resource?
You can find similar books in the "Read Also" column, or choose other free books by F Franz Brnnow to read onlineMoreLess
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