Salusbury, Thomas
,
Mathematical collections and translations (Tome I)
,
1667
Text
Text Image
Image
XML
Thumbnail overview
Document information
None
Concordance
Figures
Thumbnails
Page concordance
<
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
>
Scan
Original
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
<
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
>
page
|<
<
of 701
>
>|
<
archimedes
>
<
text
>
<
body
>
<
chap
>
<
p
type
="
main
">
<
s
>
<
pb
xlink:href
="
040/01/276.jpg
"
pagenum
="
256
"/>
underſtand the ſame, I have upon this paper tranſcribed the
<
lb
/>
cluſions that he inferreth from his twelve indagations; the firſt of
<
lb
/>
which is upon the two
<
lb
/>
<
arrow.to.target
n
="
table1
"/>
</
s
>
</
p
>
<
p
type
="
margin
">
<
s
>
<
margin.target
id
="
marg510
"/>
<
emph
type
="
italics
"/>
The greateſt and
<
lb
/>
leaſt elevations of
<
lb
/>
the new ſtar differ
<
lb
/>
not from each
<
lb
/>
ther more than the
<
lb
/>
polar allitudes, the
<
lb
/>
ſaid ſtar being in
<
lb
/>
the Firmnment.
<
emph.end
type
="
italics
"/>
</
s
>
</
p
>
<
table
>
<
table.target
id
="
table1
"/>
<
row
>
<
cell
>Of
<
emph
type
="
italics
"/>
Maurolicus
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Hainzelius,
<
emph.end
type
="
italics
"/>
from which the Star is collected to have been diſtant from the centre leſſe than 3 ſemidiameters of the Earth, the difference of Parallaxes being 4
<
emph
type
="
italics
"/>
gr. 42 m.
<
emph.end
type
="
italics
"/>
30
<
emph
type
="
italics
"/>
ſec.
<
emph.end
type
="
italics
"/>
</
cell
>
<
cell
>3
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>2. And is calculated on the obſervations of
<
emph
type
="
italics
"/>
Hain-zelius,
<
emph.end
type
="
italics
"/>
with Parall. of 8.
<
emph
type
="
italics
"/>
m. 30 ſec.
<
emph.end
type
="
italics
"/>
and its di-ſtance from the centre is computed to be more than</
cell
>
<
cell
>25
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>3. And upon the obſervations of
<
emph
type
="
italics
"/>
Tycho
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Hain-zelius,
<
emph.end
type
="
italics
"/>
with Parall. of 10
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
and the diſtance of the centre is collected to be little leſſe than</
cell
>
<
cell
>19
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>4. And upon the obſervations of
<
emph
type
="
italics
"/>
Tycho
<
emph.end
type
="
italics
"/>
and the
<
emph
type
="
italics
"/>
Landgrave,
<
emph.end
type
="
italics
"/>
with Parall. of 14
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
the diſtance from the centre is made to be about</
cell
>
<
cell
>10
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>5. And upon the obſervations of
<
emph
type
="
italics
"/>
Hainzelius
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Gemma,
<
emph.end
type
="
italics
"/>
with Parall. of 42
<
emph
type
="
italics
"/>
m. 30 ſec.
<
emph.end
type
="
italics
"/>
whereby the diſtance is gathered to be about</
cell
>
<
cell
>4
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>6. And upon the obſervations of the
<
emph
type
="
italics
"/>
Landgrave
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Camerarius,
<
emph.end
type
="
italics
"/>
with Parall. of 8
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
the di-ſtance is concluded to be about</
cell
>
<
cell
>4
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>7. And upon the obſervations of
<
emph
type
="
italics
"/>
Tycho
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Hage-cius,
<
emph.end
type
="
italics
"/>
with Parall. of 6
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
and the diſtance is made</
cell
>
<
cell
>31
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>8. And upon the obſervations of
<
emph
type
="
italics
"/>
Hagecius
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Vr-ſinus
<
emph.end
type
="
italics
"/>
with Parall. of 43
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
and the ſtars diſtance from the ſuperficies of the Earth is rendred</
cell
>
<
cell
>1/2
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>9. And upon the obſervations of
<
emph
type
="
italics
"/>
Landgravius
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Buſchius,
<
emph.end
type
="
italics
"/>
with Parall. of 15
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
and the di-ſtance from the ſuperficies of the Earth is by ſupputation</
cell
>
<
cell
>1/48
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>10. And upon the obſervations of
<
emph
type
="
italics
"/>
Maurolice
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Munocius,
<
emph.end
type
="
italics
"/>
with Parall. of 4
<
emph
type
="
italics
"/>
m. 30 ſec.
<
emph.end
type
="
italics
"/>
and the compnted diſtance from the Earths ſurface is</
cell
>
<
cell
>1/5
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
<
row
>
<
cell
>11. And upon the obſervations of
<
emph
type
="
italics
"/>
Munocius
<
emph.end
type
="
italics
"/>
and
<
emph
type
="
italics
"/>
Gemma,
<
emph.end
type
="
italics
"/>
with Parall. of 55
<
emph
type
="
italics
"/>
m.
<
emph.end
type
="
italics
"/>
and the diſtance from the centre is rendred</
cell
>
<
cell
>13
<
emph
type
="
italics
"/>
ſemid.
<
emph.end
type
="
italics
"/>
</
cell
>
</
row
>
</
table
>
</
chap
>
</
body
>
</
text
>
</
archimedes
>