Salusbury, Thomas
,
Mathematical collections and translations (Tome I)
,
1667
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motion ſtraight forwards, it goeth to the matutine conjunction;
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and moreover it being true, that when it appeareth bigge it ſhews
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with a corniculate figure, and when it appeareth little, it ſeems
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perfectly round, theſe appearances, I ſay, being true, I do not ſee
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how one can chooſe but affirm the ſaid ſtar to revolve in a circle
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bout the Sun, for that the ſaid circle cannot in any wiſe be ſaid
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to encompaſſe or to contain the Earth within it, nor to be
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our to the Sun, that is between it and the Earth, nor yet
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riour to the Sun. </
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<
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>That circle cannot incompaſſe the Earth,
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cauſe
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Venus
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would then ſometimes come to oppofition with the
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Sun; it cannot be inferiour, for then
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Venus
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in both its
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ons with the Sun would ſeem horned; nor can it be ſuperiour,
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for then it would alwayes appear round, and never cornicular;
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and therefore for receit of it I will draw the circle CH, about
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the Sun, without encompaſſing the Earth.</
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Venus
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very greas
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towards the
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ctive conjunction
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and very ſmall
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wards the
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tine.
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Venus
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rily proved to move
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about the Sun.
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>SALV. </
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>Having placed
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Venus,
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it is requiſite that you think of
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Mercury,
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which, as you know, alwayes keeping about the Sun,
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doth recede leſſe diſtance from it than
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Venus
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; therefore conſider
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with your ſelf, what place is moſt convenient to aſſign
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The revolution of
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Mercury
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concluded
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to be about the Sun,
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within the Orb of
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Venus.</
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<
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>SIMP. </
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>It is not to be queſtioned, but that this Planet
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ing
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Venus,
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the moſt commodious place for it will be, a leſſer
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cle within this of
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Venus,
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in like manner about the Sun, being
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that of its greateſt vicinity to the Sun, an argument, an evidence
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ſufficiently proving the vigour of its illumination, above that of
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Venus,
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and of the other Planets, we may therefore upon theſe
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conſiderations draw its Circle, marking it with the Characters
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BG.</
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Mars
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neceſſarily
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includeth within its
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Orb the Earth, and
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alſo the Sun.
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>SALV. </
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>But
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Mars,
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Where ſhall we place it?</
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<
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>SIMP.
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Mars,
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Becauſe it comes to an oppoſition with the Sun,
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its Circle muſt of neceſſity encompaſs the Earth; But I ſee that it
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muſt neceſſarily encompaſs the Sun alſo, for coming to
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on with the Sun, if it did not move over it, but were below it, it
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would appear horned, as
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Venus
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and the Moon; but it ſhews
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wayes round, and therefore it is neceſſary, that it no leſs includ</
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eth the Sun within its circle than the Earth. </
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<
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>And becauſe I
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member that you did ſay, that when it is in oppoſition with the
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Sun, it ſeems 60 times bigger than when it is in the conjunction,
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me thinks that a Circle about the Centre of the Sun, and that
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eth in the earth, will very well agree with theſe
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Phænomena,
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which I do note and mark D I, where
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Mars
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in the point D, is near
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to the earth, and oppoſite to the Sun; but when it is in the point
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I, it is at Conjuction with the Sun, but very far from the Earth.
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And becauſe the ſame appearances are obſerved in
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Jupiter
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and
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Saturn,
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although with much leſſer difference in
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Jupiter
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than in
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Mars,
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and with yet leſſe in
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Saturn
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than in
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Jupiter
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; me thinks I </
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