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Ad Quadratum Construction and Study of the Regular Polyhedra

Ad Quadratum Construction and Study of the Regular Polyhedra

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We have:<br />

Noting that cos Di<br />

2<br />

65<br />

R s OB <strong>and</strong> OB OL 2 BL 2<br />

<br />

a 1 <br />

Now OL <br />

2<br />

a2<br />

2<br />

<strong>and</strong> BL a1 3 a<br />

<br />

2 2<br />

OB a<br />

2 2 1 2<br />

with a 3<br />

3<br />

5 1R<br />

3 2<br />

3 R<br />

OB 3<br />

3 1 2 R<br />

R s<br />

R<br />

<br />

3 <strong>and</strong> sin I i<br />

2 <br />

3<br />

2R 3<br />

2<br />

3<br />

(or R s<br />

R 1.776)<br />

1<br />

2 , we can write Rs R <br />

cos Di 2<br />

sin Ii 2<br />

, which we can<br />

define as a growth factor gd1 . If instead, we consider <strong>the</strong> ratio <strong>of</strong> Rs to <strong>the</strong> insphere<br />

radius as will be established for <strong>the</strong> GSD, we can define a new growth factor :<br />

g d R R cos<br />

s r h<br />

<br />

r r<br />

Di 2 cos Ii 2 a cos Ii 2<br />

with cos D i<br />

2<br />

<br />

3<br />

b. The Great dodecahedron: (GD)<br />

a 3<br />

<strong>and</strong> <br />

R 3<br />

Rcos D i<br />

2 cos I i<br />

2<br />

1<br />

a<br />

R cos D i<br />

2<br />

5 1<br />

it comes g d Rs 5 .<br />

r<br />

The same basic geometry will obtain for <strong>the</strong> GD as for <strong>the</strong> SSD since <strong>the</strong> GD can be<br />

considered as made up on <strong>the</strong> basis <strong>of</strong> <strong>the</strong> SSD by extending <strong>the</strong> planes <strong>of</strong> <strong>the</strong> stellated<br />

faces so as to fill <strong>the</strong> gaps between <strong>the</strong> star branches, thus forming a convex pentagram<br />

(fig. 46A <strong>and</strong> 46B). Alternatively, it can be viewed as made up <strong>of</strong> twelve intersecting<br />

pentagonal planes <strong>and</strong> <strong>the</strong> figure <strong>of</strong> <strong>the</strong> enveloping icosahedron clearly appears on fig.<br />

47A <strong>and</strong> 47B.<br />

g d

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