Salusbury, Thomas
,
Mathematical collections and translations (Tome I)
,
1667
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caſe is not to be ſuppoſed. </
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<
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>But becauſe (obſerve well) the diſtance
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of the Firmament, in relation to the ſmallneſſe of the Earth, as
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hath been ſaid, is to be accounted, as if it were infinite; therefore
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the angle conteined betwixt the two rayes, that being drawn from
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the points A and E, go to determine in a fixed Star, is eſteemed
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nothing, and thoſe rayes held to be two parallel lines; and
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fore it is concluded, that then only may the New Star be affirmed
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to have been in the Firmament, when from the collating of the
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Obſervations made in divers places, the ſaid angle is, by
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tion, gathered to be inſenſible, and the lines, as it were, parallels.
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<
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>But if the angle be of a conſiderable quantity, the New Star muſt
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of neceſſity be lower than thoſe fixed; and alſo than the Moon, in
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caſe the angle A B E ſhould be greater than that which would be
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made in the Moons centre.</
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>SIMP. </
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>Then the remoteneſſe of the Moon is not ſo great, that
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a like angle ſhould be ^{*}inſenſible in
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* Imperceptible.</
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>SALV. </
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>No Sir; nay it is ſenſible, not onely in the Moon, but
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in the Sun alſo.</
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>SIMP. </
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>But if this be ſo, it's poſſible that the ſaid angle may
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be obſerved in the New Star, without neceſſitating it to be
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our to the Sun, aſwell as to the Moon.</
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>SALV. </
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>This may very well be, yea, and is in the preſent caſe,
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as you ſhall ſee in due place; that is, when I ſhall have made plain
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the way, in ſuch manner that you alſo, though not very perfect in
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Aſtronomical
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calculations, may clearly ſee, and, as it were, with
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your hands feel how that this Authour had it more in his eye to
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write in complacency of the
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Peripateticks,
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by palliating and
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ſembling ſundry things, than to eſtabliſh the truth, by producing
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them with naked ſincerity: therefore let us proceed forwards. </
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<
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>By
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the things hitherto ſpoken, I ſuppoſe that you comprehend very
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well how that the diſtance of the new Star can never be
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made ſo immenſe, that the angle ſo often named ſhall wholly
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appear, and that the two rayes of the Obſervators at the places
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A and E, ſhall become altogether parallels: and you may
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quently comprehend to the full, that if the calculations ſhould
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collect from the obſervations, that that angle was totally null, or
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that the lines were truly parallels, we ſhould be certain that the
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obſervations were at leaſt in ſome ſmall particular erroneous:
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But, if the calculations ſhould give us the ſaid lines to be
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ted not only to equidiſtance, that is, ſo as to be parallel, but to
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have paſt beyond that terme, and to be dilated more above than
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below, then muſt it be reſolutely concluded, that the obſervations
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were made with leſſe accurateneſſe, and in a word, to be
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ous; as leading us to a manifeſt impoſſibility. </
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<
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>In the next place,
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you muſt believe me, and ſuppoſe it for true, that two right lines </
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