Salusbury, Thomas
,
Mathematical collections and translations (Tome I)
,
1667
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<
1 - 30
31 - 60
61 - 90
91 - 120
121 - 150
151 - 180
181 - 210
211 - 240
241 - 270
271 - 300
301 - 330
331 - 360
361 - 390
391 - 420
421 - 450
451 - 480
481 - 510
511 - 540
541 - 570
571 - 600
601 - 630
631 - 660
661 - 690
691 - 701
>
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040/01/308.jpg
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gr.
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m.
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<
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<
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<
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>I O T</
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<
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>67</
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>
<
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>20</
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>
<
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>Sines</
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>
<
cell
>92276</
cell
>
</
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<
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<
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<
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>I F T</
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<
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>0</
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<
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<
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<
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>582</
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>9227600000</
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<
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<
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<
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<
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<
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>325414</
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<
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<
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>100000</
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<
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>158</
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<
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>54982</
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</
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<
row
>
<
cell
/>
<
cell
>158</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
>582</
cell
>
<
cell
>92276</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
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>34070</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
cell
>492</
cell
>
<
cell
/>
</
row
>
<
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>
<
cell
/>
<
cell
>3</
cell
>
<
cell
/>
</
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>
</
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<
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<
s
>See next that which the obſervations of
<
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type
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Peucerus
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giveth us, in
<
lb
/>
which the inferiour diſtance from the Pole is 28
<
emph
type
="
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"/>
gr. </
s
>
<
s
>21 m.
<
emph.end
type
="
italics
"/>
and the
<
lb
/>
ſuperiour 28
<
emph
type
="
italics
"/>
gr. </
s
>
<
s
>2 m.
<
emph.end
type
="
italics
"/>
the difference 0
<
emph
type
="
italics
"/>
gr. </
s
>
<
s
>19 m.
<
emph.end
type
="
italics
"/>
and the diſtance
<
lb
/>
from the vertical point 66
<
emph
type
="
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"/>
gr. </
s
>
<
s
>27 m.
<
emph.end
type
="
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"/>
from which particulars is
<
lb
/>
thered the ſtars diſtance from the centre almoſt 166
<
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/>
<
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<
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<
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type
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gr.
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type
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</
cell
>
<
cell
>
<
emph
type
="
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"/>
m.
<
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type
="
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"/>
</
cell
>
<
cell
/>
<
cell
/>
</
row
>
<
row
>
<
cell
>Angles</
cell
>
<
cell
>I A C</
cell
>
<
cell
>66</
cell
>
<
cell
>27</
cell
>
<
cell
>Sines</
cell
>
<
cell
>91672</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>I E C</
cell
>
<
cell
>0</
cell
>
<
cell
>19</
cell
>
<
cell
/>
<
cell
>553</
cell
>
</
row
>
</
table
>
<
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<
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id
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<
row
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<
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<
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>165 427/553</
cell
>
</
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<
row
>
<
cell
>553</
cell
>
<
cell
>91672</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>36397</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>312</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>4</
cell
>
</
row
>
</
table
>
<
p
type
="
main
">
<
s
>Here take what
<
emph
type
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italics
"/>
Tycho
<
emph.end
type
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italics
"/>
his obſervation holdeth forth to us,
<
lb
/>
terpreted with greateſt favour to the adverſary; to wit, the
<
lb
/>
our diſtance from the pole is 28
<
emph
type
="
italics
"/>
gr. </
s
>
<
s
>13 m.
<
emph.end
type
="
italics
"/>
and the ſuperiour 28
<
emph
type
="
italics
"/>
gr.
<
lb
/>
</
s
>
<
s
>2 m.
<
emph.end
type
="
italics
"/>
omitting the difference which is 0
<
emph
type
="
italics
"/>
gr. </
s
>
<
s
>11 m.
<
emph.end
type
="
italics
"/>
as if all were one
<
lb
/>
Parallax; the diſtance from the vertical point 62
<
emph
type
="
italics
"/>
gr. </
s
>
<
s
>15 m.
<
emph.end
type
="
italics
"/>
Behold
<
lb
/>
here below the operation, and the diſtance of the ſtar from the
<
lb
/>
centre found to be 976 9/16
<
lb
/>
<
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n
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<
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<
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n
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table65
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</
s
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</
p
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<
table
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<
table.target
id
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<
row
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<
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/>
<
cell
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<
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>
<
emph
type
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"/>
gr.
<
emph.end
type
="
italics
"/>
</
cell
>
<
cell
>
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
</
cell
>
<
cell
/>
<
cell
/>
</
row
>
<
row
>
<
cell
>Angles</
cell
>
<
cell
>I A C</
cell
>
<
cell
>62</
cell
>
<
cell
>15</
cell
>
<
cell
>Sines</
cell
>
<
cell
>88500</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>I E C</
cell
>
<
cell
>0</
cell
>
<
cell
>11</
cell
>
<
cell
/>
<
cell
>320</
cell
>
</
row
>
</
table
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<
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>
<
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id
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<
row
>
<
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/>
<
cell
>276 9/16</
cell
>
</
row
>
<
row
>
<
cell
>320</
cell
>
<
cell
>88500</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>2418</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>1</
cell
>
</
row
>
</
table
>
<
p
type
="
main
">
<
s
>The obſervation of
<
emph
type
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italics
"/>
Reinholdus,
<
emph.end
type
="
italics
"/>
which is the next enſuing,
<
lb
/>
eth us the diſtance of the Star from the Centre 793.
<
lb
/>
<
lb
/>
<
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n
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<
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/>
<
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</
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</
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</
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</
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