# Leibniz Legible — https://leibnizlegible.com
# Page: https://leibnizlegible.com/page/00068193:0411
# Permalink to this reading: https://leibnizlegible.com/page/00068193:0411?run=74
# Title: Leibniz-Handschriften zur Mathematik LH 35, 11, 18C
# Folio 203r, page id 00068193:0411
# Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=00068193&page=411
# Source image: https://digitale-sammlungen.gwlb.de/content/00068193/jpgs/default/00000411.jpg
# Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 60 lines, status machine
# Lines: 60 recognised, mean confidence 0.91
# Machine transcription. Not an edition. Errors are expected: about 8% character error rate on Latin and French lines, higher on German.
# Licence: CC BY 4.0, Leibniz Legible. Machine output: do not ingest it as verified text; keep this provenance with the text.
# Wording rule: say "the machine reads it as …", never "Leibniz wrote".
# After the first blank line: the recognised lines in reading order, one per line.

per
pro-
et au
eorum
ionis
Spro
adem
retset,
is. Ht
te pro
 cele
uod
loqui
nmo.
nem,
ama
tun
Sect. VI. De Concurcu Corporum.
tunc centrum gravitatis eadem semper celeritate ibit m
eadem rectâ od etsdem partes. Nam intelligantur extingui
corporum vires respectivae, quod fieri potest, si intelligarus
corpori cuilibet et corparibus sen respicientibus reuproce
propotionalmceleritatem respectivam aequalem et contra
riam priori (recedendi si accesserat et contra) et corporibus
sese respicientibus reuproce proportionalem esse additam.
ita enim ea tinquitur ille motus, qui ut prop. g. ostendimus
vim respectivam constituit, quippe unus contrario aequali com
pensatus; tuno igitur fota massa cessante mutatione di-
stantia inter partes masae movebitur per motum unius ri
gidi motu rectilineo aequiditributo. Adeoque centrum gravita-
mapotius
tis uniformiter et directe progredietur. Utor autem hic hy-
porseri motus compensati quam conneaionis in rigidum,
ne m casu obrigescentiae progressio pro parte in circulatio-
les
nem conventatur, quae rectilinea manebit, si motibus uni–
cormibus rectilincis jam exirtentibus (ea hypotheti) nihil
s. . 
aliud quam conatus compensantes rectilinet addantur peri
prop. 3. Cap. 2. Sert. 5..
Porro ante hanc imnovationem,
qua dutantiarum mutationum surtulit, totius matsa cen
trum gravitatis eodem ut nunc modo movebatur; quod inde
ortendo, quia duorum quorumlibet corporum centrum eodem
modo movebatur ut nunc. Ergo et centrum gravitatis totius
aggregati. De centro autem duorum quorum libet res no
patet, quia sive conpora à se non recedant, sive recedant
celeritatibus reciproce proportionalibus ad corpora, eodem
loco manet centrum gravitatis. Hinc ergo denuo demon-
etratum habemus, quod supra cap. De directione prop. 11. pri-
mum
itas
et pro
videm
ralle
esc
ranquat
ntin
itur
libere