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# Title: Leibniz-Handschriften zur Mathematik LH 35, 10, 3
# Folio 8v, page id 00068156:0016
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autem ex Phorographicis dynamica definiri
invenim. Nempe regula haec est, quaecunque
theorematalocum habent constanter in etphorographicis,
in quibus, ita ut et aequali jure tractant utrumque corpus
et eiusque progressum, eodem et locum habent in dynamicis
Reperietur autem semper aequal et prcontinuatione vel
retro sumta, vel porta (quasi dintius pro arbitrio durasset
apraesens motus) vel porro sumta (quasi diutius pro arbitrio duret,
seu cocursu; non impediuntur. ea etiam in dynamicis, locum
habent Talis est constantia ipsius progres sus centri
gravitatis, seu ie, C(C) et constantia mutatio
nis intervalli sive velocitatis respectivae seu AB - (B) (A)
sit stotus aute ocursum 1A, +B, B; et post concursum
3A, 3B, 3C; et +A, 2B, 2C sit vel ante concursum vel cocursum;
vera manebunt nostra theoremata dissimulato etiam con-
cursu intercurrente. Exempli gratia sit A per se quatur fugien
sitque concursus in D. sumatur paula anteocarsum Repraesentetur
tempus per  motum aequabilem ipsius C, itaque temp momento 2C
respondeat t 2A, 2B ante ocursam. Patet cum aqualiter decrescant
terro C procpediente usque ad 3C, ut sit 1C2C = Z
tempore, fiat sit
a aequm
seu tota mutatio facta tempore 2C3C aequatur eidem facta tempore
erdo
+C2C. Nepe tempore C3C duo finat primum mutatur inter-
valum 2A2B, donec concurrant A et B, quantum possunt, seu donec
amalius sibi accedere nequeant, quamutatio est 2A2B, demto
tamm spalio inter centra gravitatis ob motem corporum intercepto
quo intervallum sit H Ergo mytati quae maratio est est 1B
hoc intervallum vacetur H. cessario reliaquendam vocetur X
et it t et itarmutatus tempose y d erit 7A2B = K. Rursus
matat poste rursus a seinvicem necedere oportet mobilia, et mutatus
intervalli tempore D3C , 3A3B K. ergo
tempe 1A1B - 2PA = 3A3B - 2B2A. Ergo fit 1AB- 3
ac proinde infigura alia sit 2A2BZC, cocursus, et r sed retrotrahatur
quarta parte temporis, ex iC in (2C) retrotrahentur et A, B, pro 24, 2B in (_) 2p)
et 3A, 3B, 3C, similiter in (3A), (3C) (3B))rAB = 3A3B
A+ B=  D (EA) EB) et ifa A A) _ C iC(C) = 2C3C) ja m
2A3A 2ABA)L
2 2ABA): 2A3A:: rCBC): 1C2C
BABB) = 2CBB = 2C (A) sit 2, 2A, 2B, ide. Ergo 2BBB] 2ABA) 
EA, : 2B3B = 2A3A : 1CFC): 1C 2C seu (3ABB): 3A3B: : 1C(2C): 1 C2C
sn (3A (3A (3B) = 3A3B. 1C(2C): 1C2C. simiiter A( A). +AeA, et
1B2B A(2A) = 1A2A, 1C (2C): 1C2C et 1B(B) = 1 B2B. 1(2C): 1C2C. ergo
et 2C(A) = 1 A2A = 1AEA) = 1A2A, 1C2C= 1C(C) : 12C et similiter
2C(2B) = 1B2BD 1C2C - 1C 2Ch: 1C2C jam (2AEB) = 2(2A - 2AEB).
Ergo (EA) (2B) = 1A2A = 1B2B, 1C2C - 1 C): 1CIC
est autem
1AEA - 1B2B = 1AIB, et fiet 1AIB = (2A) EB) = 1A. B, 1CEG): 1C2C = BA) BB)
sed quod senfit 1A. B = EA) 2B) + (3A) (3B). Ergo similiter
in oraecedente figura fit 1A1B = 2A2B + 3A3B. Sed haec
aliquando accuratius elaboranda, et universalius
concisienda
seu non obstante
concursu