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# Title: Philosophical Principles Of Natural Religion (shelfmark Leibn. Marg. 53)
# Folio 115, page id 797370323:0273
# Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=797370323&page=273
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# Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 43 lines, status machine
# Lines: 43 recognised, mean confidence 0.86
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OrMer,
TanCeS,
t0 it;
u than
Noon i5
S. OF aII
Chap.
Farth,
C rich
ny pri
2t5.
Bodies
MerS. a.
them.
NVe
dE satura
We sec hon fainely in respect ot some
oF the fixt Stars, Saturn Cines For aIl his
Bulk; and vec tris Distance is but a Poine
in relpect oF the nearest fixt Star, FrOm
ehe Sun. The RayS Ot the sun won d De
Co distixated betore chiey reactid (O re-
more an Obieet, thac the best Lye ot
theWVorld, cond nocby ic; dilcover chem.
Pheir Distance is (0 great, thac the best
Telescope, instead oE magnitrins em above
Wrhae cher appear eo the nated lyc (25
therdoany Object, remov dby auy mentu-
rable Distance, hor great loerer) does con-
Siderablr lessen them, (o chat eher appear
lisce lucid Points. Besides, tho wre in this
GlobC, approach MCareF TheM POMCLVeNEY
Four chouland Diameters of che Farth, (OF
188304000 Miles, allorming sire thou-
Tana FCCE EO che MIilc) one time oF the
Zear than another, ret their Parallax is
Scarce sensible, iF anY ac all, Wrtich eon d noc
De, ifthey vere aemy moderare Distance:
By NIr. TlngenS Computation, the Distance
OF thc Sun From us, is co the Distance ot
che nearest fixt Star Erom uS, ad Y 10
NCE
7C