Fabri, Honoré
,
Dialogi physici in quibus de motu terrae disputatur
,
1665
Text
Text Image
Image
XML
Thumbnail overview
Document information
None
Concordance
Figures
Thumbnails
List of thumbnails
<
1 - 10
11 - 20
21 - 30
31 - 40
41 - 50
51 - 60
61 - 70
71 - 80
81 - 90
91 - 100
101 - 110
111 - 120
121 - 130
131 - 140
141 - 150
151 - 160
161 - 170
171 - 180
181 - 190
191 - 200
201 - 210
211 - 220
221 - 230
231 - 240
241 - 248
>
21
22
23
24
25
26
27
28
29
30
<
1 - 10
11 - 20
21 - 30
31 - 40
41 - 50
51 - 60
61 - 70
71 - 80
81 - 90
91 - 100
101 - 110
111 - 120
121 - 130
131 - 140
141 - 150
151 - 160
161 - 170
171 - 180
181 - 190
191 - 200
201 - 210
211 - 220
221 - 230
231 - 240
241 - 248
>
page
|<
<
of 248
>
>|
<
archimedes
>
<
text
>
<
body
>
<
chap
>
<
p
type
="
main
">
<
s
id
="
s.000285
">
<
pb
pagenum
="
24
"
xlink:href
="
025/01/028.jpg
"/>
ctus in Perigæo, à circulo decurſo in Apogæo ; Eſt enim minor propor
<
lb
/>
tio vnius ad alium; hinc per plures dies ſtare videtur; quia licèt reipſa
<
lb
/>
non ſtet, tam parum tamen promovetur & recedit à Stella, seu versùs
<
lb
/>
Ortum, ſeu versùs Occaſum, vt eandem à Stella diſtantiam ſervare vi
<
lb
/>
deatur; Cuncta hæc ita perſpicua ſunt, vt negari profectò non poſſint, quale
<
lb
/>
do vltrò in hac tua hypotheſi, huiuſmodi paſſiones Planetarum æquè facilè
<
lb
/>
explicari atque in mea. </
s
>
</
p
>
<
p
type
="
main
">
<
s
id
="
s.000286
">
<
emph
type
="
italics
"/>
Antim.
<
emph.end
type
="
italics
"/>
</
s
>
<
s
id
="
s.000287
"> Imò longè faciliùs & cum multiplici prærogativa: Nam pri
<
lb
/>
mò ſimpliciſſimum motum adhibeo; realem ſcilicet & æquabilem, circa
<
lb
/>
mundi Centrum; tu verò duos, & fortè plures, eóſque minimè æquabi
<
lb
/>
les; vtrumque in Excentrico circa centra ad libitum excogitata & ficta.
<
lb
/>
</
s
>
<
s
id
="
s.000288
">Secundo, nunquam vides Planetam extrà Perigæum & Apogæum, in eo
<
lb
/>
vero loco in quo eſt, ac proinde perpetuæ fallaciæ ſubjaces; ego in eo
<
lb
/>
loco, in quo reverà eſt, Planetam video. </
s
>
<
s
id
="
s.000289
">Tertiò, tu ſenſum decipi
<
lb
/>
aſſeris, quamvis rectè applicatum; ego vt & in aliis minimè falli repo
<
lb
/>
no, nec quiſquam hoc jure adſtruat, niſi aliqua ratione fretus. </
s
>
<
s
id
="
s.000290
">Quartò;
<
lb
/>
denique habeo in mea cauſas Phyſicas, eáſque tritas & vulgares in doctri
<
lb
/>
na motuum, iſtorum omnium effectuum, Apogæi ſcilicet, Perigæi, accelera
<
lb
/>
tionis, retardationis, &c. </
s
>
<
s
id
="
s.000291
">Tu verò meras fallacias, & oculorum illuſiones
<
lb
/>
eſſe contendis. </
s
>
<
s
id
="
s.000292
">Igitur non æquè facilè in tua hypotheſi, ac in mea, res iſta ex
<
lb
/>
plicatur, ſed in mea longè faciliùs, planiùs, &, vt ſic loquar, connaturaliùs. </
s
>
</
p
>
<
p
type
="
main
">
<
s
id
="
s.000293
">
<
emph
type
="
italics
"/>
Auguſtin.
<
emph.end
type
="
italics
"/>
</
s
>
<
s
id
="
s.000294
"> Vt vt ſit, quoad hæc, antequam ad alia, quæ fortè magis vrgent,
<
lb
/>
accedam, ex te ſcire vellem, quonam modo latitudinem Planetarum in tua
<
lb
/>
hypotheſi explices; quod eò libentiùs audiam, quò mirabilior mihi videtur
<
lb
/>
ille modus, quo in hypotheſi noſtra explicatur; in qua ſuppoſita orbitæ ex
<
lb
/>
centricæ Planetæ inclinatione ad planum Eclypticæ, latitudinis variatio per
<
lb
/>
diverſum terræ mobilis
<
expan
abbr
="
ſitũ
">ſitum</
expan
>
optimè explicatur; nempè arcus, qui maximam
<
lb
/>
latitudinem metitur, in limitibus ſub majore vel minore angulo apparet,
<
lb
/>
quo remotior, vel propior oculus ſtatuetur; quod vt in ſchemate explicem,
<
lb
/>
<
figure
id
="
id.025.01.028.1.jpg
"
xlink:href
="
025/01/028/1.jpg
"
number
="
8
"/>
<
lb
/>
Sit centrum mundi A, planum ecli
<
lb
/>
pticæ EGKH, excentricus FGI
<
lb
/>
H, cuius centrum eſt in D ; nodi G
<
lb
/>
H, arcus inclinationis excentrici F
<
lb
/>
E, IK, Telluris orbita BLCM.
<
lb
/>
</
s
>
<
s
id
="
s.000295
">Sit Terra in B, Planeta in limite Bo
<
lb
/>
reali F ; apparebit prædictus arcus
<
lb
/>
ſub angulo FBE, poſita verò Terra
<
lb
/>
in C, apparebit ſub angulo FCE,
<
lb
/>
qui priore minor eſt; Si verò ſtatua
<
lb
/>
tur in limite Auſtrali, I & Terra ſit
<
lb
/>
in C, videbitur arcus IK ſub an
<
lb
/>
gulo ICK, & ex B ſub angulo
<
lb
/>
IBK, ſed ex Optica, perſpi
<
lb
/>
cuum eſt, angulum ICK majorem
<
lb
/>
eſſe angulo FBE, quia CI minor </
s
>
</
p
>
</
chap
>
</
body
>
</
text
>
</
archimedes
>