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# Title: Leibniz-Handschriften zur Mathematik LH 35, 10, 18
# Folio 13v, page id 00068172:0026
# Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=00068172&page=26
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# Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 54 lines, status machine
# Lines: 54 recognised, mean confidence 0.88
# Machine transcription. Not an edition. Errors are expected: about 8% character error rate on Latin and French lines, higher on German.
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# After the first blank line: the recognised lines in reading order, one per line.

Res non ratis bene vic exaricata
mole
rigido pondere carens
sit vectis excussorius (LM
cujus centrum N. a
tndum ad angulos rectos
incurrat in eodem horizonse
peum
mobile A, veniens
ex u veniens ex 1A incurrat
ad angulos rectos in 2f.
si deve emobilisa sitque ab alter
rectis parte aliud mobile B.. Cajer jam certum
st aliquem esse posse situm ipsius B tam reruotum
a centro N, ut A post incursum pergat, si B.
sit admodum vicinum ipsi N, contra alium
amissa tamen perium parte, et in p translata
t
nisi B sit in N quo casu A totam oim servabit. 
si B infinite nR remotum ab N reflectetur totis
giribus servatisu si finite remotum ab N, sed
acubi frope N perget glas amissa virium parte
dalicubi longe ab N reflectetur amissa virium parte.
Ergo alicubi nec reflectetur nec perget, sed totam vim
transferet in B. 1a punctum ipsius B quaeritur
qaeritur ergo quis sit ille locus 1B, ubi hoc contrngat
 Ante omnia assumo cutrum celeritatis
commune eadem qua venerat celeritate reflecto
Et primum situm esse cC, semdo spulo funto primo
situm ejus, initro primi sempuli temporis esse 1C, initio 2di
D
esse 2C, initro tertii 3C, et coincidere, it rec
3C itaque
exit juncta 3A3C3B, seu 2A 1C3B.  recta eritque
edit 3A3C ad 3B3C, ut 1AIC ad 1B. C seu ut 2A2C ad 2B2C. jum
qua  ipsius A ccleriles qua venerat sit m, et ipsius
B qua excatitur sit n, debet esse Amm = B nn
es autem A 2A ad 2B3B ut m ad n ut 1A = A ad 2B3B
seu (ob triangula 1C1A2A, 1C2B3B simillia )ut Ctad sR
Ut  +AICIA ad 1(1B seu ut 2AC 2C2A, ad 2C2B
Ergo distantiae non debent esse reciproce ut dorpora
seu in subduplicata
reciptoca corporum ratione
ud videtur orin obsurdu, nam 2BZB
et figura
ostendit isse 1A2A: EBBB:: 1A. C: 1BIC:: B. A:
i
fit Bm= Bn quod
absurdum ilateum
non servareter
pmclitas vis
A2a
32
a