Borelli, Giovanni Alfonso
,
De motionibus naturalibus a gravitate pendentibus
,
1670
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 - 579
>
Scan
Original
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
<
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 - 579
>
page
|<
<
of 579
>
>|
<
archimedes
>
<
text
>
<
body
>
<
chap
>
<
p
type
="
main
">
<
s
id
="
s.001525
">
<
pb
pagenum
="
291
"
xlink:href
="
010/01/299.jpg
"/>
<
arrow.to.target
n
="
marg389
"/>
<
lb
/>
petit diſtantiæ eius ab axe, tunc neceſſariò talis par
<
lb
/>
ticula erit à rota disiuncta, & ſegregata. </
s
>
<
s
id
="
s.001526
">Vt in rotą
<
lb
/>
<
figure
id
="
id.010.01.299.1.jpg
"
xlink:href
="
010/01/299/1.jpg
"
number
="
114
"/>
<
lb
/>
AEH reuoluta circa cen
<
lb
/>
trum D ſi eius particulæ
<
lb
/>
A, B, C eodem
<
expan
abbr
="
tẽpore
">tempore</
expan
>
<
expan
abbr
="
de-ſcribũt
">de
<
lb
/>
ſcribunt</
expan
>
orbes AEH, BFI,
<
lb
/>
CGL,
<
expan
abbr
="
eãdem
">eandem</
expan
>
proportio
<
lb
/>
nem habentes quam di
<
lb
/>
ſtantiæ à centro AD, BD,
<
lb
/>
& CD tunc diſtingui non
<
lb
/>
poteſt an prędictæ parti
<
lb
/>
culæ ſint diſciſſæ vt arena,
<
lb
/>
vel ſint agglutinatæ rotæ ſolidæ, propterea quòd id
<
lb
/>
ipſum ſymptoma particulis duriſſimæ rotæ competit.
<
lb
/>
</
s
>
<
s
id
="
s.001527
">Si verò
<
expan
abbr
="
circũducta
">circunducta</
expan
>
rota particula A relicto orbe AHE
<
lb
/>
excurrit per tangentem rectam AM, aut curuam ſpi
<
lb
/>
ralem AN euidentiſſimum ſignum erit particulam A
<
lb
/>
non eſſe annexam, & vnitam, ſed diuiſam à rota ſo
<
lb
/>
lida, quia continentèr à centro D magis, & magis re
<
lb
/>
mouetur vt in N, vel M. </
s
>
</
p
>
<
p
type
="
margin
">
<
s
id
="
s.001528
">
<
margin.target
id
="
marg389
"/>
Cap. 7. dę
<
lb
/>
natura flui
<
lb
/>
ditatis.</
s
>
</
p
>
<
p
type
="
main
">
<
s
id
="
s.001529
">Præterea ſi particulæ eamdem à centro
<
expan
abbr
="
diſtantiã
">diſtantiam</
expan
>
<
lb
/>
retinuerint, & eodem tempore, quo rota integram̨
<
lb
/>
reuolutionem BFB abſoluit, alia particula A, vel
<
lb
/>
maius, vel minus ſpatium, quàm circulum AEA per
<
lb
/>
ſicit, ſcilicèt percurrit arcum AEH, vel AEO, tunc
<
lb
/>
euidentèr conſtat particulam A non eſſe agglutina
<
lb
/>
tam, ſed diuiſam à rota ſolida. </
s
>
</
p
>
<
p
type
="
main
">
<
s
id
="
s.001530
">Similitèr in motu directo aggregati AEH, ſi eius
<
lb
/>
particulæ inæqualibus velocitatibus feruntur, ſcili-</
s
>
</
p
>
</
chap
>
</
body
>
</
text
>
</
archimedes
>