# Leibniz Legible — https://leibnizlegible.com
# Page: https://leibnizlegible.com/page/1040780814:0023
# Permalink to this reading: https://leibnizlegible.com/page/1040780814:0023?run=74
# Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124)
# Folio 5, page id 1040780814:0023
# Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=23
# Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000023.jpg
# Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 76 lines, status machine
# Lines: 76 recognised, mean confidence 0.87
# 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.

ex alio
ipeleu.
LIb. I.
2t2S 
limatan
FOD. L
Cxoncit
l incll
ta let
ma lla
ita C
ronom
5, Lua
ta5 tal-
ItX LLu
lancta,
carum
deferri
ProdII
Oris OI
Orbita
jus sche
nUtacI
Leliplle
eCbituI
I5 eAt IN
nde rUL
alECTUM
appellatus
Lib.
nappellal, ao Lalu eraltelett. Supelala Rocon lalnue
Dit Planeta Ldclelao; al Mullald denomattone, quonam nune tl
ad alteras Felipticx partes; auseturque ulque ad Limitem l, unde
rursusminuitur, donec in Nodo e secundo craneleat.
Planetarum Orbes (hoc est Orbitarum plana) inclinantur du pla
num Ecliptica modo sequenti. 1Tempe Saturni Oibis angulo 22 gra-
duu: Toris 13 grad. Martis paulo minus quam 2 grad. Veneris
paulo majus quam 3: grad. Nercurii denigue fere 7 gradibus. De
Positione Linca Nodorum Planctx cujusque alibi dicetur.
In duabus ultimis propositionibus considerarimus Planetas quasI e
Sole vilos: Icud enim neceltarium est ad intellisendum motum illo.
rum e Terra vitorun.
PROPOSTTTO IV.
Flaenomena, à Pelluris e inferio  Planetarum, Veneris es
Mercurii, motu ot Pellure egu describere.
 cema lCa LititLALac
Cum Venus et Mercuriio cerorraur circa Solem in minoribus
Orbitis quant Lcrla, ut in schemate, I quo T retert lellurem, in
Propria Orbita T 8, ab occidente in orientem delatam; A C F COr.
Ditam a Venere, versus ealdem partes, breriori tempore percurlam;
Datet quod, cum Venus in D P F, Orbitx sux parte à Tellure remo.
tiore inrenitur, haec e Terra in r videbitur mota in consequentia Sig
norum; quo catu Directa dicitur. Cum vero Venus pervenerit ad l-
tum respectu solis ex Telluris qualis eAt a; dum à C ad H moretur,
aequali celeritate cum Sole ferri ridebitur: Nam tunc recta versus
Terram tendit; nec aliter moveri ridetur, quam quatenus ejus Or-
bita detertur a Sole rertus ortum
moto; adeoque cardior quidem
eA quam prius, scd etiamnum
Directa.
Vonus illtapel a au b 610
srella, ex, quia Soli propior cA,
relocius mota quam ipsa Telluo,
(cujus rationem inferius redde
muS,) hanc inter es Solem me
dia transit; e proinde e Tellure
risa locum, inter Fixas, mutare
quidem videbitur, at COnEra
Signorum Ceriem, i. c. in Ante-
cedentia; unde cum temporis
Retroeradta dicitur, licet eSole spectata etiamnum Directa ridere.
tur. PF incer Directionem _ Retrosradationem, prope  seilicet, Sta-
tionaria apparet; rectis nempe Terram _ Venerem, eodem mo
Similiter, post Retrosradationem, antequam rurtus Directa Fat, se
cundo Scationaria, prope B, videbitur; dt quidem Stationaria ad Di
rectionem.