Fabri, Honoré
,
Dialogi physici in quibus de motu terrae disputatur
,
1665
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 - 248
>
Scan
Original
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
<
1 - 30
31 - 60
61 - 90
91 - 120
121 - 150
151 - 180
181 - 210
211 - 240
241 - 248
>
page
|<
<
of 248
>
>|
<
archimedes
>
<
text
>
<
body
>
<
chap
>
<
p
type
="
main
">
<
s
id
="
s.000998
">
<
pb
pagenum
="
88
"
xlink:href
="
025/01/092.jpg
"/>
nec enim mutationem obliquitatis Eclipticæ admittendam eſſe putarem,
<
lb
/>
præceſſionem Æquinoctiorum lentiſſimus ille ſtellarum motus ſatis ex
<
lb
/>
plicat. </
s
>
</
p
>
<
p
type
="
main
">
<
s
id
="
s.000999
">
<
emph
type
="
italics
"/>
Antim.
<
emph.end
type
="
italics
"/>
</
s
>
<
s
id
="
s.001000
"> Ingenuitati meæ, opinor, tribues, quòd tibi ea ſuggeſſerim,
<
lb
/>
quibus moleſtum illud, vt ais, argumentum refellere valeas. </
s
>
<
s
id
="
s.001001
">Vnum tibi
<
lb
/>
perſuadeas velim, cuncta hæc non obeſſe quidem veſtræ hypotheſi, ſed non
<
lb
/>
prodeſſe; ſicuti noſtræ nec obſunt, nec proſunt; de obliquitatis Eclipticæ
<
lb
/>
mutatione, idem tecum ſentio; præceſſionetis Æquinoctiorum rectè omni
<
lb
/>
no explicas per lentiſſimum illum fixarum motum; nec in tua hypotheſi
<
lb
/>
alius modus eſſe videtur; Licet enim Copernicus, Keplerus, aliíque ex veſtris
<
lb
/>
velint fixarum motum non eſſe realem, ſed apparentem, eo quòd, inquiunt,
<
lb
/>
Æquinoctialia puncta tantulùm adducantur versùs occaſum, ſcilicet in an
<
lb
/>
tecedentia, quia libratio terreſtri globi citiùs abſolvitur, quàm motus in
<
lb
/>
Zodiaco, hoc tamen, in eo ſaltem iudicio, non ſubſiſtit, nempe prædicta li
<
lb
/>
bratio, vt ſic loquar, oritur ex motu orbis integro, circa axem axi Eclipticæ
<
lb
/>
parallelum, ſeu ex paralleliſmo axis terræ, circa quem orbes diurni erunt;
<
lb
/>
hoc autem in iiſdem punctis Eclipticæ Æquinoctialia puncta eſſe ſuppo
<
lb
/>
nit, ſed hæc ad rem noſtram nihil faciunt. </
s
>
</
p
>
<
p
type
="
main
">
<
s
id
="
s.001002
">
<
emph
type
="
italics
"/>
Auguſtin.
<
emph.end
type
="
italics
"/>
</
s
>
<
s
id
="
s.001003
"> Expecta tantulùm, Antime, hic enim ſtellarum motus
<
lb
/>
in tua hypotheſi difficilè, ſaltem, vt audio, explicatur; vnde for
<
lb
/>
tè meam vel hoc nomine, tuæ quiſpiam præferendam eſſe putaret. </
s
>
</
p
>
<
p
type
="
main
">
<
s
id
="
s.001004
">
<
emph
type
="
italics
"/>
Antim.
<
emph.end
type
="
italics
"/>
</
s
>
<
s
id
="
s.001005
"> Longè faciliùs, Auguſtine, ſtellarum motus, quàm Planeta
<
lb
/>
rum, in qualibet hypotheſi explicatur pro quo ſuppono 1. fixum æter
<
lb
/>
numque eſſe Naturæ inſtitutum, vt ſtellæ omnes eundem inter ſe ordinem
<
lb
/>
& ſitum ſervent. </
s
>
<
s
id
="
s.001006
">2. Nunquam mutari illarum latitudinem: His poſitis,
<
lb
/>
cogita ſtellam quampiam in ipſa Ecliptica, cogita etiam circulum quem
<
lb
/>
libet immobilem, puta meridiànum, in quo ſtella, primùm ſita ſit, co
<
lb
/>
gita denique ipſam Eclipticam, circa Axem mundi, ſuum
<
expan
abbr
="
motũ
">motum</
expan
>
abſolvere,
<
lb
/>
ita vt idem punctum, quod erat in dicto meridiano ad illum redeat, orbe
<
lb
/>
peracto ab ortu, in occaſum 24.horis. </
s
>
<
s
id
="
s.001007
">Iam cogita ſtellam illam ſimul cum
<
lb
/>
Ecliptica ab ortu in occaſum ferri, & circumduci, & paulo tardiùs, vt eo
<
lb
/>
momento, quo dictum punctú Eclipticæ, in quo erat, attingit meridianum,
<
lb
/>
ipſa tantulùm versùs ortum remaneat, non quidem extra Eclipticam,
<
lb
/>
ſed in ipſamet Ecliptica: nec enim perfectum orbem deſcribit, ſed
<
lb
/>
talem ſpiram, vt ſemper Ecliptice reſpondeat; aliæ verò, quæ ſunt extra Ecli
<
lb
/>
pticam, eandem ſemper ab illa diſtantiam retineant, vnde præter circularé
<
lb
/>
motum, altera ſaltem inclinatioue opus eſt, cujus terminus ſit æquator,
<
expan
abbr
="
nõ
">non</
expan
>
<
lb
/>
Ecliptica; ita tamen moventur, vt ſemper eandem ab Ecliptica diſtantiam
<
lb
/>
retineant: inde præceſſio Æquinoctiorum facilè explicatur, quæ tamen
<
lb
/>
ex eo explicari non poteſt, quod Sol in diverſis punctis Æquatorem ſecet;
<
lb
/>
quia cum Sol ſemper Eclipticæ inſiſtat, licèt versùs occaſum ſectio Ecli
<
lb
/>
pticæ cum Æquatore, ipſo Æquinoctij momento ſingulis, annis promo
<
lb
/>
veatur, non tamen ex hoc ſequitur Æquinoctiorum præceſſio, ne
<
lb
/>
que propterea ſtella quæpiam ab Æquinoctij puncto versùs Ortum remove-</
s
>
</
p
>
</
chap
>
</
body
>
</
text
>
</
archimedes
>