Salusbury, Thomas
,
Mathematical collections and translations (Tome I)
,
1667
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Two ſorts of
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motions of the
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taining Veſſel, may
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make the
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ned water to riſe
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and fall.
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The Cavities of
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the Earth cannot
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approach or go
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ther from the
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tre of the ſame.
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The progpeſſive
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and uneven motion
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may make the
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ter contained in a
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Veſſel to run to
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and fro.
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+ A Town
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ing S. E. of
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Venice
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The parts of the
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terreſtrial Globe
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accelerate and
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tard in their
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on.
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<
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>SIMP. </
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>This Propoſition, at firſt ſight to me, that am neither
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Geometrician nor Aſtronomer, hath the appearance of a very
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great Paradox; and if it ſhould be true, that the motion of the
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whole,
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being regular, that of the parts, which are all united to
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their
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whole,
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may be irregular, the Paradox will overthrow the
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Axiome that affirmeth,
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Eandem eſſe rationem totius &
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tium.
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<
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>SALV. </
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<
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>I will demonſtrate my Paradox, and leave it to your
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care,
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Simplicius,
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to defend the Axiome from it, or elſe to
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concile them; and my demonſtration ſhall be ſhort and
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miliar, depending on the things largely handled in our
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dent conferences, without introducing the leaſt ſyllable, in
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vour of the flux and reflux.</
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<
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>We have ſaid, that the motions aſſigned to the Terreſtrial
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Globe are two, the firſt Annual, made by its centre about the
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circumference of the Grand Orb, under the Ecliptick, according
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to the order of the Signes, that is, from Weſt to Eaſt; the other
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made by the ſaid Globe revolving about its own centre in twenty
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four hours; and this likewiſe from Weſt to Eaſt: though
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bout an Axis ſomewhat inclined, and not equidiſtant from that
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of the Annual converſion. </
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<
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>From the mixture of theſe two
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tions, each of it ſelf uniform, I ſay, that there doth reſult an
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uneven and deformed motion in the parts of the Earth. </
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<
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>Which,
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that it may the more eaſily be underſtood, I will explain, by
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drawing a Scheme thereof. </
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<
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>And firſt, about the centre A [
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in
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Fig. </
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<
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>1. of this Dialogue
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] I will deſcribe the circumference of
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the Grand Orb B C, in which any point being taken, as B,
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about it as a centre we will deſcribe this leſſer circle D E F G,
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repreſenting the Terreſtrial Globe; the which we will ſuppoſe
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to run thorow the whole circumference of the Grand Orb, with
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its centre B, from the Weſt towards the Eaſt, that is, from the
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part B towards C; and moreover we will ſuppoſe the
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ſtrial Globe to turn about its own centre B likewiſe from Weſt
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to Eaſt, that is, according to the ſucceſſion of the points
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D E F G, in the ſpace of twenty four hours. </
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<
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>But here we
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ought carefully to note, that a circle turning round upon its
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own centre, each part of it muſt, at different times, move with
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contrary motions: the which is manifeſt, conſidering that whilſt
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the parts of the circumference, about the point D move to the
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left hand, that is, towards E, the oppoſite parts that are about F,
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approach to the right hand, that is, towards G; ſo that when
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the parts D ſhall be in F, their motion ſhall be contrary to what
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it was before. </
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<
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>when it was in D. Furthermore, the ſame time
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that the parts E deſcend, if I may ſo ſpeak, towards F, thoſe in
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G aſcend towards D. </
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<
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>It being therefore preſuppoſed, that </
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