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# Title: Leibniz-Handschriften zur Mathematik LH 35, 14, 2
# Folio 18r, page id 00068202:0035
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quando conatus aequales puncta A. B. Cee
sunt in cudcamferentia circuli nstur ergo
generalis methodus definiendi centrum
Gravitatis rectarum in circulo positarum
B BC
esc ponam
in inossignabiles linea Lma
ocus centiorum gravitatis
et recta ex  d ducta LX
Hic de lom
positione dire
ctionum etiam
isfinitarum.
Cgvam my tanu ens occuvit et mira, de
 in puncto X centro gm modo descrbendi
generalissimum, et sit et  non sit rircutus
ed curvo quaecunque quod est summe considerantu
ed hinc sequitur aliquid verum, nempe dar
et punctum et tangentem transcendentis cam
lineae, procontrs genvi
eut
lineam centrotum
gravitatis curvo
item data linea
centrotum, invene
endi curvam
ssensum etiam
hic vulgarem
directionum
compositionem
non procedere
Et elegantia de
e
positione
 rationum
et de carundem
additione
duo
si sint tr conatus corporis in D positi, in unum componendi
se nempl A ND, DC quaerim qua li ea sennt D. et
qua coleritale seu, si corpus D simul conctur celeritatibus
et directionibus  DA, DB, DC quaeritur qua ceteritate
DM
et dinc linea sive directione, et qua coleritate moveatur d.
iel Hoc ut videntur fiat consideretur du corpus
Dduplicari, et unum tendene in ire un ceter motu DA, alterum
motao DB, et centrum centrum gravitatis eorum perveniet in L
bisecans rectam AB. cum vero reveraduo corpira
compositumibit
in unum coalescere intelliuantur, ibant via sui centri gravitatis
hoc est in rect directione et celeritate DL, et quoniam
corpus D ver revera dimidium est compositifer ipso duplicato
ibit dupla celeritate. e nempe DK.
si sint tres conatus DA, DB, DC quaeratur eadem Methodo
Centrum gr. commune trium aequalium ipsi D, corporum, 
in A, B, C positorum. idque ita fiet centrum ipsorum A et B est L,
ipsorum. jungatur CL. et sumtur et secetur s in M, sic ut LM
sit dimidia ipsius MC, et erit DM quidem directio ipsius D, seu linea
in qua feretur mobile, fpla ipsa autem DK) tripla ipsius dM,
talis enim intelliqus: debet licet chartae spatium non permiserit,
Eodem cuodo autem invenietur M, si BC fuisset bisecta in ()
erit directio et celeritas ipsius. D.
et juncta A(L) vel AC bisecta in () et juncta B(L), nam rectae
A(L), C L, B(L) se intersecabunt in communi puncto M. quod est
in effici poterit continuat
centrum gravitatis trium aeque gravium A, B, C. i motium copositione vagar
Vidaamus an idem, effici posit continuata motuum compositione palgari
ponamus dA DB dC alte nmales conis directionibus  A, DB
oit directo DL sie eoneannutum A Assumamus angulum
ADB graduum 2d Angulum BdC grad. 60 compolita directone
et ang. ADC grad. 80 componatur directio AB et dA et dB, eit
Dx bisecet angulum ADB, erit DL directio composita.
componenda adhuc cum directione De quae superest bisecetir ergo aggulus CDL per
OL direstio
et directio totalis prit DV. et angulus ADV trit id dimidius ejus qui restet detracta ADL, 10
ab ADC ∞,
quae porio compogatum cum d
restat dehaleato c) as a bote na pa absidere henge i2
V
imo sals
ada
val
an
sih
2s