Spherical Trigonometry: for Colleges And Secondary Schools
Spherical Trigonometry: for Colleges And Secondary Schools
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In our eReader you can find the full English version of the book. Read Spherical Trigonometry: for Colleges And Secondary Schools 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 Trigonometry: for Colleges And Secondary Schools
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In an analogous manner the positions of bodies on the celestial sphere are described by means of, or by reference to, certain points and great circles on that sphere. There are four different systems of circles of reference. As in the case of the terrestrial sphere, each system consists of two circles, each of which passes through the pole of the other, and, accordingly, is at right angles to the other. Two of these systems are described in Arts. 70, 71, a third in Art. 76, and the fourth in Ar...t. 77. A point which will be referred to in these systems is the north celestial pole. This is the point where the earth's axis, if prolonged, would pierce the celestial sphere. It is near the pole star, being about 1\^ from it.
**'... imagine the entire solar system as represented by a tiny circle the size of the dot over this letter i.'* (Neptune the outermost planet known of the solar system is 2790 millions of miles from the sun ; i.e. 30 times as far as the earth.) " Even the sun itself, on this exceedingly reduced scale, could not be detected with the most powerful microscope ever made.
What to read after Spherical Trigonometry: for Colleges And Secondary Schools?
You can find similar books in the "Read Also" column, or choose other free books by Daniel a Daniel Alexander Murray to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
In an analogous manner the positions of bodies on the celestial sphere are described by means of, or by reference to, certain points and great circles on that sphere. There are four different systems of circles of reference. As in the case of the terrestrial sphere, each system consists of two circles, each of which passes through the pole of the other, and, accordingly, is at right angles to the other. Two of these systems are described in Arts. 70, 71, a third in Art. 76, and the fourth in Ar...t. 77. A point which will be referred to in these systems is the north celestial pole. This is the point where the earth's axis, if prolonged, would pierce the celestial sphere. It is near the pole star, being about 1\^ from it.
**'... imagine the entire solar system as represented by a tiny circle the size of the dot over this letter i.'* (Neptune the outermost planet known of the solar system is 2790 millions of miles from the sun ; i.e. 30 times as far as the earth.) " Even the sun itself, on this exceedingly reduced scale, could not be detected with the most powerful microscope ever made.
What to read after Spherical Trigonometry: for Colleges And Secondary Schools?
You can find similar books in the "Read Also" column, or choose other free books by Daniel a Daniel Alexander Murray to read onlineMoreLess
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