See next that which the observations of Peucerus giveth us, in which the inferiour distance from the Pole is 28 gr. 21 m. and the superiour 28 gr. 2 m. the difference 0 gr. 19 m. and the distance from the vertical point 66 gr. 27 m. from which particulars is gathered the stars distance from the centre almost 166 semediameters.
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Here take what Tycho his observation holdeth forth to us, interpreted with greatest favour to the adversary; to wit, the inferiour distance from the pole is 28 gr. 13 m. and the superiour 28 gr. 2 m. omitting the difference which is 0 gr. 11 m. as if all were one Parallax; the distance from the vertical point 62 gr. 15 m. Behold here below the operation, and the distance of the star from the centre found to be 976 916 semidiameters.
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The observation of Reinholdus, which is the next ensuing, giveth us the distance of the Star from the Centre 793. Semidiameters.
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