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History of Science Department University of Aarhus

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82 5. COPERNICUS' PLANETMODELLER I DE REVOLUTIONIBUS<br />

= 198 1 og =391, med A =159 .<br />

Modellens kon guration til tidspunktet t4 er afbildet i Fig. 5.22.<br />

C<br />

J<br />

Z<br />

4<br />

A h<br />

O<br />

E<br />

M<br />

S<br />

y<br />

v<br />

Figur 5.22<br />

I 4CMS: Da MS = e1 = 687 p nar MC = r = 10000 p og \CMS =<br />

180 ; = 140 59 kan SC og \SCM ndes. Copernicus angiver ikke selv<br />

udregningerne, men den anvendte metode er beskrevet i bog 1,XIII pkt. V:<br />

Betragt Fig. 5.23.<br />

+<br />

C<br />

Figur 5.23.<br />

M<br />

S<br />

D<br />

Γ<br />

C<br />

D<br />

J<br />

4<br />

Figur 5.24.<br />

I 4MDSrO = 1<br />

2 MS = 10000p : \MDS =90 og \SMD = = 39 1<br />

^SD = 78 2<br />

^MD = 101 58<br />

1:1:1<br />

)<br />

SD = 12591 p<br />

MD=15539 p :<br />

I enheden hvor r = 10000 p fas nu<br />

SD = 433 p , MD = 534 p og DC = MD + MC = 10534 p<br />

+Pythagoras<br />

Fra<br />

SC = [(DC) 2 +(SD) 2 ] 1<br />

2 = 10543 p .<br />

MS<br />

crd2(\SCM) =<br />

SC<br />

crd2(\CMS)<br />

S

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