Benedetti, Giovanni Battista de
,
Io. Baptistae Benedicti ... Diversarvm specvlationvm mathematicarum, et physicarum liber : quarum seriem sequens pagina indicabit ; [annotated and critiqued by Guidobaldo Del Monte]
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IO. BAPT. BENED.
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peiæ tam lucida, vt ipſo lucifero videretur rutilantior
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cæterarum (abſque vlla
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aſpectus diuerſitate) magis ſcintillans. </
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rum diſtant, alioqui multo maiores, non etiam illa clariores apparuerint? </
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<
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xml:space
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quis diceret eam exhalationem non ita fortaſſe dilatari, vt inter nos, & aliam ali-
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quam ſtellam interponeretur. </
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<
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xml:space
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lem exhalationem, tantam latitudinem occupare, quod aliquibus populis aliam
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circunuicinãhac ipſa de qua mentionem ſecimus redderet lucidiorem.
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<
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xml:space
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">Sed cum hoc perſpectum fuerit nulli, ſequebatur lucem illam ab ipſis exhalatio-
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nibus elementaribus haud poſſe oriri: </
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xml:space
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gno fuit inditio, ſi phas eſt credere,
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quo magis aliquod coeleſte corpus ſcintillat,
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eo longius à nobis diſtare.</
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<
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ſcribam, idcirco tibi morem gerere volens paucis ſubiungam.</
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<
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xml:space
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<
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>
ſignatur pro
<
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Globo terreſtri cuius
<
var
>.i.</
var
>
centrum ſit et
<
var
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>
pro conuexo ignis, ſed
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>
pro orbe
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octauo
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autem pro ſtella iam ſuperius dicta, quæ ſemper fuit, eſt, & erit, quamuis
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cæteris tribus nunc obſcurior ſit. </
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quę ſint
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et
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diametraliter inuicem oppoſita, ita quod circa eorum orizontes poſ
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ſibile ſit ſtellam
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videre, radijs ipſius ſtellæ mediantibus
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et
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par-
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tes
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et
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ita breues ſint, reſpectu eorum
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, vt vix ſexcenteſima pars ſit vna
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illarum, nec non
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ita breuis reſpectu ſemidiametri octauæ ſphæræ, quod
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vix ſit vna ex partibus decemmillibus, vt ſcis, ſequitur quod recta terminata ab
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>
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et
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minor ſenſibiliter non ſit ipſo terræ diametro
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cum duo hæc interualla ex
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triangulorum ſimilitudine ſe habeant vt
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ad
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hoc eſt ferè vt .602. ad .601. vn-
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de anguli
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et
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à rectis minime differre videbuntur, cum eorum differen-
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tia certo modo minima ſit. </
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fuerint duæ diagonales
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et
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angulos
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et
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ferè ęquales,
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aſſero de angulis
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et
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.</
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<
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xml:space
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tes elementaris regionis circum circa lineam
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: </
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<
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xml:space
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">tunc clarum eſſet quod ſi ratione hu
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iuſmodi exhalationis ſtella
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ita lucida viſa fuerit tam aſpicientibus ab
<
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var
>
quam ab
<
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c. exhalatio minoris latitudinis quam
<
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>
eſſe non poterat, hoc eſt, quam terræ dia-
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lb
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meter, cum idem in longitudine ferè ſit, ſed punctum
<
var
>.u.</
var
>
ſatis videri poteſt ab oculo
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lb
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in
<
var
>.e.</
var
>
& punctum
<
var
>.n.</
var
>
ab oculo in
<
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var
>
vt alias tibi probaui, ratione refractionis radiorum
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per diuerſa diafana tranſeuntium. </
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<
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xml:space
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et
<
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>.c.
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n.</
var
>
vſque ad octauum orbem ad puncta
<
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var
>
et
<
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>
reliquum erit nos videre quantitates
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graduum arcus
<
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>.s.x.</
var
>
et
<
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>.k.x.</
var
>
ſed
<
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>.s.x.</
var
>
ſubiacet a ngulo
<
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>.s.e.x.</
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>
et
<
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>.k.x.</
var
>
angulo
<
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>.k.c.x.</
var
>
qui qui
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quidem anguli nihil differunt ſenſibiliter ac ſi eſſent in centro
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. </
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xerimus angulos
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et
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ſenſibiliter mi nime differre ab angulis
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>
et
<
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>.e.
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u.c.</
var
>
ſi cognouerimus quantitatem iſtorum, cognita etiam nobis erit quantitas
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ill orum.</
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<
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xml:space
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33. ad vnum, & cogitata
<
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>
vt dicta ſemidiameter, quia ſenſibiliter ab ea minime
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diffe
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rt, nunc ſi ſupponatur dicta
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vt
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orthogonij eſſe
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.100000
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& dixerimus ſi
<
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>
vt partium .33. præbet nobis
<
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>.c.e.</
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>
duarum partium, quid nobis
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pręſtabit eadem
<
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>
vt partium .100000. vnde proueniet nobis
<
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>.c.e.</
var
>
vt
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.6060.
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cuius angulus
<
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>.c.n.e.</
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>
erit graduum .3. & min .29. ita etiam erit angulus
<
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>.k.</
var
>
e
<
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<
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>
cuius ar- </
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