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Elements of theoretical and descriptive astronomy, for the use of colleges and academies (1901)

White, Charles J · New York: J. Wiley & sons · leaf 150

An illustration from Elements of theoretical and descriptive astronomy, for the use of colleges and academies, 1901, leaf 150
point where it touches. When the apex falls short ofthe surface, there will be no total eclipse; but at the point inwhich the axis of the cone, prolonged, meets the earth, the SOL Ul ECLIPSE. 141 observer will see what is called an annular eclipse, the moonbeing- projected upon the disc of the sun,… … Fig. 60. and QDt drawn tangent to the sun and the earth: that is, unlessthe moons geocentric latitude is less than the angle MES.Now we have, MES = ME A + AEB -f BES, and, also, AEB = CAE — CBE.BES is the suns semi-diameter, MEA that of the moon, CAEthe moons horizontal parallax, and CBE the suns:…

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