Valerio, Luca
,
De centro gravitatis solidorvm libri tres
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 - 283
>
Scan
Original
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
<
1 - 30
31 - 60
61 - 90
91 - 120
121 - 150
151 - 180
181 - 210
211 - 240
241 - 270
271 - 283
>
page
|<
<
of 283
>
>|
<
archimedes
>
<
text
>
<
body
>
<
chap
>
<
p
type
="
main
">
<
s
>
<
pb
xlink:href
="
043/01/265.jpg
"
pagenum
="
86
"/>
æquale erit cono KBL. </
s
>
<
s
>Rurſus quia eſt vt EB ad BD, ita
<
lb
/>
quadratum GD ad quadratum DK, hoc eſt circulus cir
<
lb
/>
ca GH ad circulum circa KL, hoc eſt conus GBH ſi
<
lb
/>
deſcribatur ad conum KBL: ſed vt FB ad BE ita eſt co
<
lb
/>
noides GBH ad conum GBH; ex æquali igitur erit vt
<
lb
/>
FB ad BD, ita conoides GBH ad conum KBL, hoc
<
lb
/>
eſt ad ſolidum AGBHC. </
s
>
<
s
>Manifeſtum eſt igitur
<
expan
abbr
="
propoſitũ
">propoſitum</
expan
>
. </
s
>
</
p
>
<
p
type
="
head
">
<
s
>
<
emph
type
="
italics
"/>
COROLLARIVM.
<
emph.end
type
="
italics
"/>
</
s
>
</
p
>
<
p
type
="
main
">
<
s
>Ex huius Theorematis demonſtratione manife
<
lb
/>
ſtum eſt, ijſdem poſitis cylindros deficientes, ex
<
lb
/>
quibus conſtat exceſſus, quo figura conoidi hyper
<
lb
/>
bolico circumſcripta ſuperat circumſcriptam co
<
lb
/>
noidi parabolico, ita ſe habere, vt quorumlibet
<
lb
/>
trium inter ſe proximorum minor proportio ſit
<
lb
/>
minimi ad medium, quam medij ad maximum:
<
lb
/>
æquales enim ſunt ſinguli ſingulis cylindris, ex
<
lb
/>
quibus conſtat figura cono BKL circumſcripta,
<
lb
/>
qui ſunt inter eadem plana parallela. </
s
>
<
s
>Quod ſi
<
lb
/>
ita eſt, ſimul illud manifeſtum erit, & ex hoc, &
<
lb
/>
ex ijs, quæ in ſecundo libro demonſtrauimus; præ
<
lb
/>
dictum exceſſum ex tot cylindris deficientibus
<
lb
/>
eiuſdem altitudinis, quos diximus componi poſſe,
<
lb
/>
vt ipſius centrum grauitatis in axe BD diſtet à
<
lb
/>
centro grauitatis coni KBL, hoc eſt à puncto in
<
lb
/>
quo axis BD ſic diuiditur, vt pars, quæ ad ver
<
lb
/>
ticem ſit reliquæ tripla, ea diſtantia, quæ minor
<
lb
/>
ſit quantacum que longitudine propoſita. </
s
>
</
p
>
</
chap
>
</
body
>
</
text
>
</
archimedes
>