Salusbury, Thomas
,
Mathematical collections and translations (Tome I)
,
1667
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141 - 150
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181 - 190
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>From the following obſervation of the
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Landgrave,
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the diſtance
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of the Star from the Centre is made to be 1057,
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m.
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<
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>Angles</
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<
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>I A C</
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<
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>66</
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<
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>57</
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>Sines</
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<
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>92012</
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<
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>I E C</
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<
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>0</
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>3</
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>87</
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>1057 53/87</
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>87</
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>92012</
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>5663</
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>Two of the moſt favourable obſervations for the Authour
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ing taken from
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Camerarius,
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the diſtance of the Star from the
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tre is found to be 3143
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>I A C</
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>65</
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>43</
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>Sines</
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<
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>91152</
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>I E C</
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>0</
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<
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>1</
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<
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>29</
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>29</
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>91152</
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>4295</
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<
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<
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>The Obſervation of
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Munoſius
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giveth no
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Parallax,
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and
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fore rendreth the new Star amongſt the higheſt of the fixed. </
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<
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>That
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of
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Hainzelius
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makes it infinitely remote, but with the correction
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of an half
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min. </
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<
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>prim.
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placeth it amongſt the fixed Stars. </
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<
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>And the
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ſame is collected from
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Vrſinus,
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with the correction of 12.
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min. </
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>
<
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>prim.
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The other Aſtronomers have not given us the diſtance above and
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below the Pole, ſo that nothing can be concluded from them. </
s
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<
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>By
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this time you ſee, that all the obſervations of all theſe men conſpire
<
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againſt the Author, in placing the Star in the Heavenly and
<
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eſt Regions.</
s
>
</
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<
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>SAGR. </
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>
<
s
>But what defence hath he for himſelf againſt ſo manifeſt
<
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contradictions?</
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>
</
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<
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<
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>SALV. </
s
>
<
s
>He betakes himſelf to one of thoſe weak threads which
<
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I ſpeak of; ſaying that the
<
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Parallaxes
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come to be leſſened by means
<
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of the refractions, which opperating contrarily ſublimate the
<
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<
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nomenon,
<
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whereas the
<
emph
type
="
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Parallaxes
<
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type
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abaſe it. </
s
>
<
s
>Now of what little
<
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ſtead this lamentable refuge is, judge by this, that in caſe that effectof
<
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the refractions were of ſuch an efficacy, as that which not long time
<
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ſince ſome Aſtronomers have introduced, the moſt that they could
<
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work touching the elevating a
<
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Phæuomenon
<
emph.end
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above the Horizon </
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>
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