Galilei, Galileo
,
The systems of the world
,
1661
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121 - 130
131 - 140
141 - 150
151 - 160
161 - 170
171 - 180
181 - 190
191 - 200
201 - 210
211 - 220
221 - 230
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<
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<
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xlink:href
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065/01/298.jpg
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pagenum
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288
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<
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<
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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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</
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<
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<
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type
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m.
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</
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<
cell
/>
<
cell
/>
</
row
>
<
row
>
<
cell
>Angles</
cell
>
<
cell
>I O T</
cell
>
<
cell
>67</
cell
>
<
cell
>20</
cell
>
<
cell
>Sines</
cell
>
<
cell
>92276</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>I F T</
cell
>
<
cell
>0</
cell
>
<
cell
>20</
cell
>
<
cell
/>
<
cell
>582</
cell
>
</
row
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</
table
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<
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<
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<
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>T I</
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<
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<
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>T I</
cell
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<
cell
>T F</
cell
>
</
row
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<
row
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<
cell
>582</
cell
>
<
cell
>10000</
cell
>
<
cell
>92276</
cell
>
<
cell
>0</
cell
>
</
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</
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<
table
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<
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id
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<
row
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<
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<
cell
>15854982</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
>582</
cell
>
<
cell
>9227600000</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
cell
>3407002746</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
cell
>49297867</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
cell
>325414</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
>100000</
cell
>
<
cell
>158</
cell
>
<
cell
>54982</
cell
>
</
row
>
<
row
>
<
cell
/>
<
cell
>158</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
>582</
cell
>
<
cell
>92276</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
cell
>34070</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
cell
>492</
cell
>
<
cell
/>
</
row
>
<
row
>
<
cell
/>
<
cell
>3</
cell
>
<
cell
/>
</
row
>
</
table
>
<
p
type
="
main
">
<
s
>See next that which the obſervations of
<
emph
type
="
italics
"/>
Peucerus
<
emph.end
type
="
italics
"/>
giveth us, in
<
lb
/>
which the inferiour diſtance from the Pole is 28
<
emph
type
="
italics
"/>
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
="
italics
"/>
gr. </
s
>
<
s
>27 m.
<
emph.end
type
="
italics
"/>
from which particulars is
<
lb
/>
thered the ſtars diſtance from the centre almoſt 166
<
lb
/>
<
lb
/>
<
arrow.to.target
n
="
table62
"/>
<
lb
/>
<
arrow.to.target
n
="
table63
"/>
</
s
>
</
p
>
<
table
>
<
table.target
id
="
table62
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<
row
>
<
cell
/>
<
cell
/>
<
cell
>
<
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
>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
>
<
table
>
<
table.target
id
="
table63
"/>
<
row
>
<
cell
/>
<
cell
>165 427/553</
cell
>
</
row
>
<
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
="
italics
"/>
Tycho
<
emph.end
type
="
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
/>
<
arrow.to.target
n
="
table64
"/>
<
lb
/>
<
arrow.to.target
n
="
table65
"/>
</
s
>
</
p
>
<
table
>
<
table.target
id
="
table64
"/>
<
row
>
<
cell
/>
<
cell
/>
<
cell
>
<
emph
type
="
italics
"/>
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
>
<
table
>
<
table.target
id
="
table65
"/>
<
row
>
<
cell
/>
<
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
="
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
/>
<
arrow.to.target
n
="
table66
"/>
<
lb
/>
<
arrow.to.target
n
="
table67
"/>
</
s
>
</
p
>
</
chap
>
</
body
>
</
text
>
</
archimedes
>