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Know_files/FINGERPRINTS OF THE GODS.pdf - D Ank Unlimited

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Graham Hancock – <strong>FINGERPRINTS</strong> <strong>OF</strong> <strong>THE</strong> <strong>GODS</strong><br />

cause the earth’s ‘paper bag’ to bulge outwards at the equator. The<br />

corollary is a flattening at the poles. In consequence, our planet deviates<br />

slightly from the form of a perfect sphere and is more accurately<br />

described as an ‘oblate spheroid’. Its radius at the equator (3963.374<br />

miles) is about fourteen miles longer than its polar radius (3949.921<br />

miles). 14<br />

For billions of years the flattened poles and the bulging equator have<br />

been engaged in a covert mathematical interaction with the recondite<br />

influence of gravity. ‘Because the Earth is flattened,’ explains one<br />

authority, ‘the Moon’s gravity tends to tilt the Earth’s axis so that it<br />

becomes perpendicular to the Moon’s orbit, and to a lesser extent the<br />

same is true for the Sun.’ 15<br />

At the same time the equatorial bulge—the extra mass distributed<br />

around the equator—acts like the rim of a gyroscope to keep the earth<br />

steady on its axis. 16<br />

Year in, year out, on a planetary scale, it is this gyroscopic effect that<br />

prevents the tug of the sun and the moon from radically altering the<br />

earth’s axis of rotation. The pull these two bodies jointly exert is,<br />

however, sufficiently strong to force the axis to ‘precess’, which means<br />

that it wobbles slowly in a clockwise direction opposite to that of the<br />

earth’s spin.<br />

This important motion is our planet’s characteristic signature within the<br />

solar system. Anyone who has ever set a top spinning should be able to<br />

understand it without much difficulty; a top, after all, is simply another<br />

type of gyroscope. In full uninterrupted spin it stands upright. But the<br />

moment its axis is deflected from the vertical it begins to exhibit a<br />

second behaviour: a slow and obstinate reverse wobble around a great<br />

circle. This wobble, which is precession, changes the direction in which<br />

the axis points while keeping constant its newly tilted angle.<br />

A second analogy, somewhat different in approach, may help to clarify<br />

matters a little further:<br />

1 Envisage the earth, floating in space, inclined at approximately 23.5°<br />

to the vertical and spinning around on its axis once every 24 hours.<br />

2 Envisage this axis as a massively strong pivot, or axle, passing<br />

through the centre of the earth, exiting via the North and South Poles<br />

and extending outwards from there in both directions.<br />

3 Imagine that you are a giant, striding through the solar system, with<br />

orders to carry out a specific task.<br />

4 Imagine approaching the tilted earth (which, because of your great<br />

size, now looks no bigger to you than a millwheel).<br />

5 Imagine reaching out and grasping the two ends of the extended axis.<br />

6 And imagine yourself slowly beginning to inter-rotate them, pushing<br />

14 Figures from Encyclopaedia Britannica, 1991, 27:530.<br />

15 Ibid.<br />

16 Path of the Pole, p. 3.<br />

227

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