Newton, Isaac
,
Philosophia naturalis principia mathematica
,
1713
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 - 524
>
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 - 524
>
page
|<
<
of 524
>
>|
<
archimedes
>
<
text
>
<
body
>
<
chap
>
<
subchap1
>
<
subchap2
>
<
p
type
="
main
">
<
s
>
<
pb
xlink:href
="
039/01/297.jpg
"
pagenum
="
269
"/>
tur jam diſtantiæ quælibet, puta
<
emph
type
="
italics
"/>
SA, SD, SF
<
emph.end
type
="
italics
"/>
in progreſſione Mu
<
lb
/>
<
arrow.to.target
n
="
note245
"/>
ſica, & differentiæ
<
emph
type
="
italics
"/>
Aa-Dd, Dd-Ff
<
emph.end
type
="
italics
"/>
erunt æquales; & propter
<
lb
/>
ea differentiis hiſce proportionales areæ
<
emph
type
="
italics
"/>
thlx, xlnz
<
emph.end
type
="
italics
"/>
æquales erunt
<
lb
/>
inter ſe, & denſitates
<
emph
type
="
italics
"/>
St, Sx, Sz,
<
emph.end
type
="
italics
"/>
id eſt,
<
emph
type
="
italics
"/>
AH, DL, FN,
<
emph.end
type
="
italics
"/>
conti
<
lb
/>
nue proportionales.
<
emph
type
="
italics
"/>
<
expan
abbr
="
q.
">que</
expan
>
E. D.
<
emph.end
type
="
italics
"/>
</
s
>
</
p
>
<
p
type
="
margin
">
<
s
>
<
margin.target
id
="
note244
"/>
DE MOTU
<
lb
/>
CORPORUM</
s
>
</
p
>
<
p
type
="
margin
">
<
s
>
<
margin.target
id
="
note245
"/>
LIBER
<
lb
/>
SECUNDUS</
s
>
</
p
>
<
p
type
="
main
">
<
s
>
<
emph
type
="
italics
"/>
Corol.
<
emph.end
type
="
italics
"/>
Hinc ſi dentur Fluidi denſitates duæ quævis, puta
<
emph
type
="
italics
"/>
AH
<
emph.end
type
="
italics
"/>
<
lb
/>
&
<
emph
type
="
italics
"/>
CK,
<
emph.end
type
="
italics
"/>
dabitur area
<
emph
type
="
italics
"/>
thkw
<
emph.end
type
="
italics
"/>
harum differentiæ
<
emph
type
="
italics
"/>
tw
<
emph.end
type
="
italics
"/>
reſpondens; &
<
lb
/>
inde invenietur denſitas
<
emph
type
="
italics
"/>
FN
<
emph.end
type
="
italics
"/>
in altitudine quacunque
<
emph
type
="
italics
"/>
SF,
<
emph.end
type
="
italics
"/>
ſumen
<
lb
/>
do aream
<
emph
type
="
italics
"/>
thnz
<
emph.end
type
="
italics
"/>
ad aream illam datam
<
emph
type
="
italics
"/>
thkw
<
emph.end
type
="
italics
"/>
ut eſt differentia
<
lb
/>
<
emph
type
="
italics
"/>
Aa-Ff
<
emph.end
type
="
italics
"/>
ad differentiam
<
emph
type
="
italics
"/>
Aa-Cc.
<
emph.end
type
="
italics
"/>
</
s
>
</
p
>
<
p
type
="
main
">
<
s
>
<
emph
type
="
center
"/>
<
emph
type
="
italics
"/>
Scholium.
<
emph.end
type
="
italics
"/>
<
emph.end
type
="
center
"/>
</
s
>
</
p
>
<
p
type
="
main
">
<
s
>Simili argumentatione probari poteſt, quod ſi gravitas particu
<
lb
/>
larum Fluidi diminuatur in triplicata ratione diſtantiarum a centro;
<
lb
/>
& quadratorum diſtantiarum
<
emph
type
="
italics
"/>
SA, SB, SC,
<
emph.end
type
="
italics
"/>
&c. </
s
>
<
s
>reciproca (nem
<
lb
/>
pe
<
emph
type
="
italics
"/>
(SAcub./SAq), (SAcub./SBq), (SAcub./SCq)
<
emph.end
type
="
italics
"/>
) ſumantur in progreſſione Arithme
<
lb
/>
tica; denſitates
<
emph
type
="
italics
"/>
AH, BI, CK,
<
emph.end
type
="
italics
"/>
&c. </
s
>
<
s
>erunt in progreſſione Geome
<
lb
/>
trica. </
s
>
<
s
>Et ſi gravitas diminuatur in quadruplicata ratione diſtan
<
lb
/>
tiarum, & cuborum diſtantiarum reciproca (puta
<
emph
type
="
italics
"/>
(SAqq/SAcub), (SAqq/SBcub),
<
lb
/>
(SAqq/SCcub.),
<
emph.end
type
="
italics
"/>
&c.) ſumantur in progreſſione Arithmetica; denſitates
<
lb
/>
<
emph
type
="
italics
"/>
AH, BI, CK,
<
emph.end
type
="
italics
"/>
&c. </
s
>
<
s
>erunt in progreſſione Geometrica. </
s
>
<
s
>Et ſic in
<
lb
/>
infinitum. </
s
>
<
s
>Rurſus. </
s
>
<
s
>ſi gravitas particularum Fluidi in omnibus di
<
lb
/>
ſtantiis eadem ſit, & diſtantiæ ſint in progreſſione Arithmetica,
<
lb
/>
denſitates erunt in progreſſione Geometrica, uti Vir Cl.
<
emph
type
="
italics
"/>
Edmundus
<
lb
/>
Hælleius
<
emph.end
type
="
italics
"/>
invenit. </
s
>
<
s
>Si gravitas ſit ut diſtantia, & quadrata diſtantia
<
lb
/>
rum ſint in progreſſione Arithmetica, denſitates erunt in progreſ
<
lb
/>
ſione Geometrica. </
s
>
<
s
>Et ſic in infinitum. </
s
>
<
s
>Hæc ita ſe habent ubi Fluidi
<
lb
/>
compreſſione condenſati denſitas eſt ut vis compreſſionis, vel, quod
<
lb
/>
perinde eſt, ſpatium a Fluido occupatum reciproce ut hæc vis. </
s
>
<
s
>
<
lb
/>
Fingi poſſunt aliæ condenſationis Leges, ut quod cubus vis com
<
lb
/>
primentis ſit ut quadrato-quadratum denſitatis, feu triplicata ra
<
lb
/>
tio Vis æqualis quadruplicatæ rationi denſitatis. </
s
>
<
s
>Quo in caſu, ſi gra
<
lb
/>
vitas eſt reciproce ut quadratum diſtantiæ a centro, denſitas erit
<
lb
/>
reciproce ut cubus diſtantiæ. </
s
>
<
s
>Fingatur quod cubus vis compri
<
lb
/>
mentis ſit ut quadrato-cubus denſitatis, & ſi gravitas eſt reciproce
<
lb
/>
ut quadratum diſtantiæ, denſitas erit reciproce in ſuſquiplicata ra-</
s
>
</
p
>
</
subchap2
>
</
subchap1
>
</
chap
>
</
body
>
</
text
>
</
archimedes
>