Gassendi, Pierre
,
De motu impresso a motore translato epistulae duae
,
1642
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027/01/006.jpg
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ſeu Copernicanus. </
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<
s
id
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id.000142
">Sol in centro, Fixæ in
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circumſerentia immotæ. </
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>
<
s
id
="
id.000143
">Medio in spatio
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Planetæ mobiles, ac in ipſis Terra inter Ve
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nerem, & Martem. </
s
>
<
s
id
="
id.000144
">Diſtantia Fixarum tan
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ta, vt magnus orbis, cuius ſemidiameter ſit
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à sole ad Terram, pro puncto habeatur, com
<
lb
/>
paratus ad ipſam. </
s
>
<
s
id
="
id.000145
">Duplex Terræ motus,
<
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/>
Diurnus circa proprium axem, Annuus
<
lb
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ſub Zodiaci ſignis, in quorum vno dum eſt,
<
lb
/>
apparet Solin oppoſito eſſe. </
s
>
<
s
id
="
id.000146
">Continetur ſem-
<
lb
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per axis Terræ in ſui paralliliſmo & duci
<
lb
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in Formamentum congruus, deſcribit qui
<
lb
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dem circulum tantum circa polum mundi,
<
lb
/>
quantus circulus magni orbis eſt, ſed qui
<
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heinc tamen appareat vt punctum. </
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>
<
s
id
="
id.000147
">Conti
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nentia hac non omninô aſſequuta motum
<
lb
/>
centri, retrahit ſenſim æquinoctialia puncta
<
lb
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in ſignorum antecedentia.
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emph.end
type
="
italics
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p.122. </
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</
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<
s
id
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id.000148
">X.
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emph
type
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italics
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Tranſlata per Eclipticam Terra, Sol
<
lb
/>
perinde videbitur Eclipticam percurrere,
<
lb
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& Eclipſes haud ſecùs contingent, quàm ſi
<
lb
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in centro quieſceret. </
s
>
<
s
id
="
id.000149
">Si Terra habetur Pla
<
lb
/>
netarum vnus, omnes tam motu, quàm ma
<
lb
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gnitudine congruunt; ſi non habetur, diſſo
<
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nant. </
s
>
<
s
id
="
id.000150
">Luna videtur altera Terra. </
s
>
<
s
id
="
id.000151
">Licet
<
lb
/>
Terra
<
expan
abbr
="
exiracentrũ
">extra centrum</
expan
>
Firmamentiſ et, videtur
<
lb
/>
tamen hemiſphærium, quod duæ parallelæ,
<
lb
/>
vna per centrum, alia per terræ ſuperficiem
<
lb
/>
traductæ, ad ſenſum tandem
<
expan
abbr
="
coẽant
">coeant</
expan
>
. </
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>
<
s
id
="
id.000152
">Axis
<
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Terræ continentia, & Fixarum diſtantia
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facit, vt vbicumque in Zodiaco Terræ ſit,
<
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/>
eædem ſtellæ verticales, eadem altitudo po
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laris appareat. </
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>
<
s
id
="
id.000153
">Eadem axis, at ſimùl æqua
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toris continentia & dierum, noctiumque
<
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/>
inqualitatem, & æſtatis, ac hiemis vicißi
<
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/>
tudinem parit. </
s
>
<
s
id
="
id.000154
">Stellæ Fixæ apparent pro
<
lb
/>
moveri, iuxta ſignorum ſeriem, quòd ſectio
<
lb
/>
nes aquinoctiales regrediantur aduerſus
<
lb
/>
easdem.</
s
>
<
s
id
="
id.a00154
">Sol Apogeius, ac Perigeius appares,
<
lb
/>
quod Terrra Aphelia & Perihelia fiat.
<
emph.end
type
="
italics
"/>
<
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<
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<
emph
type
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italics
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Motus Planetarum circæ Solem ellipticus,
<
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non circularis.
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type
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italics
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p.132. </
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<
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id
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">XI.
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emph
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Tranſlata per Zodiacum
<
expan
abbr
="
Terrã
">Terra</
expan
>
, nullus
<
lb
/>
eſt Planetarum, qui non vno tenore, ac ſuam
<
lb
/>
ſemper viam procedat. </
s
>
<
s
id
="
id.000156
">Regreßiones illæ,
<
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/>
Stationeſque, quæ in vulgari ſententia tan
<
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/>
tæ inconcinnitatis ſunt, non-niſi apparenter
<
lb
/>
fiunt. </
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>
<
s
id
="
id.000157
">Res declaratur in Mercurio, & Ve
<
lb
/>
nere; itemque in Marte, Ioue, ac Saturne.
<
lb
/>
</
s
>
<
s
id
="
id.000158
">Sol in medio omnium congruè collocatus.
<
lb
/>
</
s
>
<
s
id
="
id.000159
">Conſtitutus in centro Sol, & nihilominùs
<
lb
/>
ſibi ipſi motu circiter menſtruo circumdu
<
lb
/>
ctus (quod monſtrant eius Macula) vide
<
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/>
tur Planetas omneis ſuis veluti magneticis
<
lb
/>
radiis circumagere, propriores rapidiùs, re
<
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/>
motiores ſegus.
<
emph.end
type
="
italics
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p.142. </
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<
s
id
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id.000160
">XII.
<
emph
type
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italics
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Ex motu Terræ attributo æſtus maris
<
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deducitur, & exemplo nauiculæ aqua ſemi
<
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/>
plenæ declaratur. </
s
>
<
s
id
="
id.000161
">Ex motu diurno, & an
<
lb
/>
nuo coniunctes oritur bis in die in æqualitas,
<
lb
/>
ob quam mare quotidie bis fluat, at refluat.
<
lb
/>
</
s
>
<
s
id
="
id.000162
">Res mediterraneo mars applicatur. </
s
>
<
s
id
="
id.000163
">In eræ
<
lb
/>
Prouinciæ attollitur mare, ac deprimitur ad
<
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ſeſqui-pedem. </
s
>
<
s
id
="
id.000164
">Creata ſpeciali inæqualitate
<
lb
/>
circa ſolſtitia, & æquinoctia, fit aſtus vehe
<
lb
/>
mentior, ſed circa æquinoctia præſertìm.
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/>
</
s
>
<
s
id
="
id.000165
">Creatâ aliâ ob conſtitutam in coniunctione,
<
lb
/>
aut oppoſitione Lunam, fit quoque æſtus in
<
lb
/>
nouiluniis, ac in pleniluniis maior. </
s
>
<
s
id
="
id.000166
">Ex motu
<
lb
/>
Terra æſtus maris, ex aſtu maris motus
<
lb
/>
Terræ efficitur probabilis. </
s
>
<
s
id
="
id.000167
">Declaratur res
<
lb
/>
iterum nauiculæ comparatione.
<
emph.end
type
="
italics
"/>
p.149. </
s
>
</
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type
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<
s
id
="
id.000168
">XIII.
<
emph
type
="
italics
"/>
Statur decreto Cardinalium de
<
lb
/>
Terra quieſcente, non mota. </
s
>
<
s
id
="
id.000169
">Epiſtola con
<
lb
/>
cluditur.
<
emph.end
type
="
italics
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p.155. </
s
>
</
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<
s
id
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id.000170
">Poſt ſcriptum.
<
emph
type
="
italics
"/>
Explicatur Problema;
<
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Quam ob cauſam fiat, vt res flexilis, veluti
<
lb
/>
virga, aut lamina, vbi manu deflexa eſt, di
<
lb
/>
mittente manu moueatur, ſuumque ſitum
<
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repetat?
<
emph.end
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p.157. </
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