# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/00068051:0029 # Permalink to this reading: https://leibnizlegible.com/page/00068051:0029?run=73 # Title: Leibniz-Handschriften zur Mathematik LH 35, 6, 6 # Folio 15r, page id 00068051:0029 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=00068051&page=29 # Source image: https://digitale-sammlungen.gwlb.de/content/00068051/jpgs/default/00000029.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 73, 2026-08-27T15:28:38Z — 107 lines, status machine # Lines: 107 recognised, mean confidence 0.82 # 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. ot musur hinc si Recta AC in plano ujus paginae rotetur circa Centrum A; continueque inter rotandum diminuatur, atque ita describat lineam EE; via centr gravitatis et ita post se relinqual partes EF tunc via centri e line ae AB gavitatis totius hujus linea utcunque divulso, ducta in ipsam totam AC, aquabitur sectori CAEC ut vero Khanc viam. Uentri gravitatis inveniamus quaerendus est unus ejus situs indefinitus, ut in casu A+ E quo linea _AC divu sa est in partes A4F, 3E3F, 2E2F, 1E1F sit AG, X et GE, y; AE,Z; EF de quaeritur centrum gr. hujus situs. ynE Xx + g et AC, C EFes fit et Zdz = Xdx+ yduu Et ut centrum gravitatis omnia ZZ habeatur, fiet quaeritur quaeretur fdq y et (due qua sit omnium EF, centrum gr. sit p. et fiet p R (distantia ab axe) AE (ut A+E) bisecetur in H. Erit H centrum ipsius AE. jungatur HP. seceturque in puncto q, ita ut PQ sit adAque (dqy: c - Z et AR= (dzX :, c- Z ut AE ut AC -AE (quae est summa omnium EF) eritquequeCentrum gravitatis praesentis siliis divulsae rectae AC, sit Bisecetur AC in S, et erit linea sq via centrigravitatis rectae AC, usque ad rasum 4E, et rectangulum sub AC, et Sq aequabitur sectori CACC CA+EC. Verum Ex _ H ducatur ad axem normatis XL: RL :: C- Z,: Z 0bf HK, et ex Z normalis gL. quaeruntur AL, et LQ 1Z Y seu AL - DK: ARL AL:: c -Z:Z Et similiter +pE Ex 6 fit (Z.A E - Z. AK = AR. C - A L. C e seu fit ALL +C+ H F A +C. Z AR + ZAK;: C ( similique ratione LQ = KH RP = LG . c- Z, : Z ex 7 fit (ZLD - ZXH = cKP - c t Q - Z RP (+ ZLq) seu fit LG = c. Z R P + Z KH;C (4 jam AR ZX et KH Z y. Ergo ex 9 per 4 et 12 fit AL = (dz. X + = ZX,: C = M taque ous Et ex 11 per 3 et 13 fit Lg= f 4Z. y + +) LZ7,: C =n est mo quadaturas summari ipsas idzue et ipsas Ha est antem per 2. ipsas dZ = xax tydy,: ExX+yy et fiet Xdy = XX dx + Xydy, : XX + 9y Hinc m= E SXxdR AE Sagdu + + ZX (21) sxatyus raxtgus yq= Xydx +gydy: Sxxtyy Hinc ubi sumcmae sumeniae decrescendo += (Xydx +1Zy incipsendo a prim maxima z. Quod si velumue inciperae e infima, loco seu 2c Cyydus finc n=. C rtgus C saxtgus mi a minima, tunc pro sectore supradicto; sumi debebit DAIOAET si esset XX+yy = XXyy: aa Et quin _ ex ryus voletur 2Y, hinc Xx qu gs et iu = Xa + =y + 1 Xxy ex speciali curvae natura, fieret m = E) sy feret n = a sudy + ~ X + + xyy adeoque fiet n = (Inx-aa dx + a y + Xxy Xx = ay aagys e:, yy-aa seu X = ay: ryy -aa et HH = XXaa: XX- aa seu y = ax: Ixx - aa et smuliter n = = (Syg aady +ax + Xyy Hni pateo m etn pendere ex Est. Hyp. Taegus -2 (22) postremo (C Sdmam + sandn = Areae dictae dm = L xxdx 1 + xy dy + qla 1 L xtq + ic tax +qu dx + Xxdx g tercyus Nec dubito quin hinc quod querimus etiam calculo facile demonstrebur Sagy e tkxcgus nostram theorema. rertur quadraturoe quaesita Tar et cyntaatro ad etur ali Ex coptemus exemplum pmondetur fit XX ~gy = bov seu Z= Bi et Xy. Z- sp - a: A XXd. Z ax: Y b X requisitae ipsius vero sareae soi Ngu x aa v (od rrxcoruto Erpo YY dx. Z es summatilis yydy: Z bv- a dus va aa- tol,: X _ 2Hy = 2a∞ = Xa L , _ na- vv = ya y veaaa + ygaa = aa + vV sit v - +x f vy v arvo- yA co = v ~ XX + Hy = vV XX + Yy =geri X = K K sec m WB+ nB + p y = fvV + gB +h Jin. 5. 2np V + + ffW + 2fg0 + 2fk VV + gguv +2g0 + hh rumv + 2mnv + 2mp VV fit m 20 et f20 sit. p = 0 et AC0 et mmVB + Emno + nn es quadeuto a Lmmiss V + Tnntgue 2 mns, + nn vr seu fiet mmante + mingue +Hfun (Hgg)- (mmun) H99) +2mntq seu mg - fn = 0, adeoque x = mbP 19m: fB y = f4 9b (hinc g. x H = v mult. per est.) Ergo xxagus = Sum+VV mmog. H+99V X = 1v, 1+ g. f V 3 = su, 1+GFV ExRFy = V 1t g. V Ssm Z axb. Z = mn ∞, 1+g.+ B (. F 4yA - A 1d. s0 entm haque isitum NoE ngus Xy. Z = Sasv, 241. v itax et y forent ad rectam Cas prayrlu rXtV Cm +7 =aa av ma-c0a apsatv, a ua eco + aud an- vy- at, a 6a-